The Tapeats Sandstone beds are severely bent in the Carbon Canyon fold exposed in a side canyon in eastern Grand Canyon. Conventional geologists accept that this folding occurred during the Laramide orogeny at ~35–70 Ma when the Colorado Plateau was uplifted. However, the Tapeats Sandstone had been deposited at 507–508 Ma, so after ~450 million years it should have been fully cemented and lithified. Yet the sandstone beds look as though they were bent smoothly while they were still unlithified and soft. Such a conclusion is preposterous if there were ~450 million years between deposition of the Tapeats Sandstone and its deformation in the Carbon Canyon fold. So, Tapeats Sandstone samples were collected from the hinge and limb zones of the Carbon Canyon fold, as well as samples several miles from the fold. The macroscopic features that should be present if the Tapeats Sandstone beds in the fold had been bent via ductile deformation over millions of years are bedding plane slip that produced slickensides on bedding plane surfaces and thickening of hinge zones and thinning of limb zones, as well as more fracturing in the hinge zones compared to the limbs. At the microscopic scale there should be evidence of grain boundary sliding, rotation and fracturing of grains, and within many quartz grains there should be sub-grains, undulose extinction, deformation lamellae and deformation kink bands. Field observations were inconsistent with ductile deformation. While bedding plane slip most likely occurred, slickensides were only found on one bedding plane surface, and there was only trivial thickening of one bed in one hinge zone. Also, fracturing was more prevalent in the limbs than in the hinge zones. All these features have been replicated using damp soft sediment layers in experiments simulating compressional folding, which equates to soft-sediment deformation. None of the microscopic features expected from ductile deformation are present in any of the samples. There are no deformation lamellae or deformation kink bands in the quartz grains which rarely displayed even trivial undulose extinction, and there is no obvious evidence of any rotation of grains or grain boundary sliding. The few quartz grains containing sub-grains are likely derived from metamorphic source rocks rather than being a product of ductile deformation, and the few subtle fractures in rare quartz grains are consistent with fracturing due to compaction of the sand grains under the confining overburden pressures. Instead, the poorly to moderately well-sorted, sub-angular to sub-rounded quartz and K-feldspar grains, and muscovite flakes comprising the sandstone are still in their detrital condition with no indications of the silica cement having been disturbed since lithification of the sandstone or of any metamorphic changes to these constituent minerals or the rock fabric. Furthermore, SEM images clearly demonstrate that the quartz cement has not been disrupted since lithification, with many cement crystals still being pristine with terminal faces intact. Both the macroscopic and microscopic evidence are conclusively consistent only with soft-sediment deformation before cementation and lithification. Therefore, it is concluded that the Tapeats Sandstone had to be folded while still relatively damp and soft soon after deposition and before cementation and lithification. Problems with the radioisotope dating methods and the U-Pb dates obtained for the Tapeats Sandstone rule out the vast claimed ages. This can all be easily reconciled with rapid deposition of the Tapeats Sandstone early in the biblical global Flood cataclysm only ~4,350 years ago and rapid deposition of ~3,300–4,500 m (~10,800–14,750 ft) of overlying sedimentary layers caused by the catastrophic plate tectonics of the Flood year. It is proposed that late in the Flood year, the Farallon plate underplated the western North American plate, causing isostatic reequilibration which resulted in the Laramide uplift of the Colorado Plateau and the monocline folding in the Grand Canyon region. Because the Tapeats Sandstone beds were still relatively damp and soft less than a year after rapid burial, they easily responded to the soft-sediment deformation to form the smooth bending in the Carbon Canyon fold before the beds dried and were cemented and lithified to sandstone. Altogether, more than 500 million years of claimed geologic history are thus eliminated.
Keywords: Tapeats Sandstone, Carbon Canyon fold, Laramide orogeny, East Kaibab Monocline, soft-sediment deformation (SSD), ductile deformation, bedding slip, grain-boundary sliding, microstructures, quartz, detrital grains, textures, cement, global Flood cataclysm
Summary of Findings
(1) The Tapeats Sandstone samples within the Carbon Canyon fold, whether from the hinge zones or the limbs, are no different to the distal samples in their mineral constituents, textures, and porosities, still being in their essentially detrital and original sedimentary condition.
(2) The detrital muscovite flakes are still bent around quartz and K-feldspar grains and sometimes still have frayed ends, confirmation that the sandstone samples are all still in their original sedimentary condition.
(3) There is no evidence of any grain-boundary sliding between the quartz and the other sand grains, nor are there any deformation lamellae or even undulose extinction within quartz grains that should be there if ductile deformation had occurred in the sandstone layers in the Carbon Canyon fold, nor is there any evidence of any metamorphism due to deep burial and the deformation.
(4) The quartz cement is pristine with no evidence of any disruption in any of the samples, but instead the quartz cement crystals have overgrown the original detrital grains and meet at triple points, often with good crystal terminations, thus infilling pore spaces, all indicating the cement formed after the folding.
(5) Thus, conditions in the history of the sandstone have not been different during its deformation in this fold compared to the same sandstone distant from this fold.
(6) All the macroscopic features in the Carbon Canyon fold, including very minor bedding plane or flexural slippage between some beds, minor rare fracturing, and sporadic joints, as well as one instance of slickensides, have all been readily replicated in soft-sediment deformation experiments at laboratory scale.
(7) There is no macroscopic or microscopic evidence consistent with the conventional explanation that the Carbon Canyon fold was produced by ductile deformation over millions of years some 450 million years after deposition and cementation of the Tapeats Sandstone.
(8) Instead, all the macroscopic and microscopic evidence combined is only consistent with the Carbon Canyon fold having been produced by soft-sediment deformation of the Tapeats Sandstone soon after deposition and before cementation.
Many structures in sedimentary rock layers result from the primary depositional processes, such as graded bedding and cross-bedding (Boggs 1995). On the other hand, soft-sediment deformation or penecontemporaneous structures are so called because they develop at the time of deposition or shortly thereafter, during the early stages of the sediment’s consolidation and before full lithification. This is because the sediments need to be unsolidified or “liquid-like” for such deformation to occur (Boggs 1995).
However, other structures in sedimentary rocks are caused by deformation long after lithification and diagenesis have occurred. Rocks buried deep in the earth may be under confining pressures or stress and temperatures to deform plastically. Prolonged, incremental strain over a long period can also cause plastic deformation. These processes are believed to be able to fold rock layers. This type of behavior is known as ductile deformation. It is the ability of a rock to accumulate strain (folding) on a mesoscopic scale. Under the confining pressures and accompanying elevated temperatures, the rock grains may recrystallize and/or the minerals undergo metamorphism, causing new minerals such as micas to grow perpendicular to the maximum principal stress direction to accommodate it. Hand and thin section analysis should be able to determine if rocks have experienced ductile deformation. Paleozoic rocks, including the Tonto Group of Grand Canyon, most likely were not buried deep enough to experience ductile deformation as they were well above the brittle-ductile transition zone. Incremental strain over sustained periods of time is harder to differentiate. As noted above, it can also result in ductile deformation.
On the other hand, under some near surface conditions, rock layers may remain coherent because the grains and/or layers within them can facilitate the folding. This type of deformation is most common in near surface rocks and is a type of brittle deformation. Most near surface rock layers undergo brittle fracturing and faulting, leaving the rock’s grains fractured. Some coherent units may slide past one another along bedding planes as the rocks are folded. This helps accommodate folding through flexural slip. Telltale signs of this should be thus clearly evident in outcrops and from microscope examination of the rock fabric and the sediment grains.
There are several prominent locations in Grand Canyon where the Paleozoic sedimentary rock layers are folded, sometimes in conjunction with faulting in the underlying Precambrian basement rocks, where there apparently are unresolved questions as to whether the folding represents soft-sediment deformation folding or later tectonic folding (ductile or brittle) well after the whole strata sequence was deposited. In most instances the folding is usually claimed to be the result of ductile (plastic) behavior of the lithified sedimentary rocks under prolonged stress due to Late Mesozoic-Early Cenozoic deformation during the Laramide orogeny, hundreds of millions of years after the whole Paleozoic strata sequence was deposited (Huntoon 2003; Karlstrom and Timmins 2012). However, the macroscopic fabric of the Tapeats Sandstone, Bright Angel Formation, and Muav Formation of the Cambrian Tonto Group sedimentary rock layers involved in these folds might suggest, and seems to be more consistent with, the folding being due to soft-sediment deformation. Any soft-sediment deformation should have occurred soon after deposition of these sedimentary units in the Cambrian (499–508 Ma) (Karlstrom et al. 2020), well before the tectonic activity associated with the Laramide orogeny that began in the terminal Mesozoic and earliest Cenozoic (60–70 Ma). This poses an apparent paradox that obviously needs resolving, and thus a focused study was designed to determine the timing and nature of this folding, beginning with a thorough investigation of the petrology of each of these rock units generally, and subsequent detailed examination of these rock units in each fold.
It has been extensively documented that lithified rocks which have suffered ductile deformation will exhibit outcrop evidence of bedding plane slip and attenuation, such as flexural slippage (Ramsay 1967). However, field examination of these folds is insufficient to determine whether they were due to such ductile behavior of the lithified rocks under much later prolonged stress or due to soft-sediment deformation soon after deposition. Detailed microscopic examination is thus absolutely necessary to document the character of the sandstone, specifically, the textural relationships between the constituent grains and the timing of the formation of the cement (lithification). Telltale microscopic textures would be evident, such as grain boundary sliding, the preferred orientation and recrystallization of the original detrital grains, as well as deformation lamellae and undulose extinction in those grains, and the original sedimentary cement between them would be broken or fractured or metamorphosed. Such textural features would be absent if the folding were due to soft-sediment deformation, as the original detrital grains and the cement binding them together in the sandstone in the folds would be essentially identical to those in the same sandstone distant from the folds.
Yet it appears that no previous investigators have done any thin section investigations of the Tapeats Sandstone, Bright Angel Formation, and Muav Formation to substantiate their claims of ductile deformation of these rock units in these folds. Obviously, more detailed field and laboratory studies (especially intensive microscope examination) are needed to resolve the questions of what condition the sandstone, shale, and limestone were in when they were deformed into these folds, and thus how soon after deposition the deformation occurred, before or after lithification of the sandstone, shale, and limestone. Any field and laboratory study of the Tapeats Sandstone, Bright Angel Formation, and Muav Formation in the folds should thus also include a field and laboratory study of these rock units in other locations distant from these folds. This would enable observations and conclusions at the one location to be confirmed in the studies at the other locations, because the evidence seen in thin section examination of these rock units in these folds should be different from that in the distant sandstone, shale, and limestone samples if the folding was due to ductile behavior under the stress of deformation of the lithified sandstone, shale, and limestone in the folds. On the other hand, the microscope evidence should be essentially identical in all samples if the folding was due to soft-sediment deformation.
Therefore, on a research and sampling trip through the Grand Canyon to investigate these folds with National Park Service approval, 12 samples of the Tapeats Sandstone within the Carbon Canyon fold and its vicinity and four samples from the Tapeats Sandstone at similar stratigraphic positions within the formation at sufficient distances away from that fold were collected so as to provide comparative control samples for the subsequent detailed thin section examination (fig. 1). Thus, Snelling (2021) reviewed extensively what is already known about the petrology of the Tapeats Sandstone and reported detailed microscope observations made on the collected samples. From the mineralogy and textures of these samples, inferences were drawn about the sand source, its transport and deposition, and the sandstone’s subsequent history, providing the documentation that can now be referred to and built on in this subsequent paper focused on the timing of lithification (cementation) of the Tapeats Sandstone in the Carbon Canyon fold before or after the folding occurred, that is, soft-sediment deformation or ductile deformation, respectively.
The Laramide Orogeny
The Laramide orogeny occurred in western North America during the latest Cretaceous (70–80 Ma) through the Eocene (35–55 Ma) (Huntoon 2003; Karlstrom and Timmins 2012). It is named after the Laramie Mountains of eastern Wyoming and should not be confused with the Siever orogeny with which it overlaps in space and time. Conventional geologists place the Grand Canyon region near sea level from 100 to 70 Ma, during which time the Sierra Nevada magmatic arc was building a series of volcanic peaks near the margin of the North American plate. The Laramide orogeny included widespread uplift of the Colorado Plateau an average of ~2 km (~6,500 ft) (Karlstrom and Timmins 2012) and a significant eastward expansion of the belt of Cordilleran deformation beyond previous limits of accretion, orogenesis, and magmatism. Laramide deformation was characterized by crustal contraction and northeast to eastward transport in a zone extending from the subduction trenches along the West Coast to the eastern limits of the Rocky Mountains (in the Black Hills). Types of deformation included east-verging thrust faulting and reverse displacements along many reactivated Precambrian basement faults. Faulting was accompanied by the development of monoclines and anticlines in the covering sedimentary rocks (Huntoon 2003).
The position of the high Rocky Mountains, and the associated and intimately related high-elevation Colorado Plateau adjacent to them, ~1,000 km (~620 mi) from the edge of the North American plate remains poorly understood. Epeirogeny (plateau building) is the uplift of regions without major tilting, folding, or thrusting of strata to build high elevation but relatively flat plateaus, which requires buoyancy of the crust on a regional scale during the Laramide orogeny. The plate tectonic explanation generally favored for Laramide orogenesis was a flattening of the angle of subduction of the oceanic plate known as the Farallon plate under western North America. Several hypotheses have been proposed as the cause of the flat-slab subduction—a more rapid rate of subduction, and/or the oceanic Farallon plate was thickened, and may have consisted of an oceanic plateau (Liu et al. 2010). In addition, Clarey (2020, 330–334) suggested the subducted plate under western North America contained a divergent boundary which caused flattening of the subduction angle due to its high heat and buoyancy. As a consequence of the shallow subduction angle, it has been suggested that no magmatism occurred in the central west of the North American continental plate during the Paleogene (Dickinson and Snyder 1978), and the underlying oceanic lithosphere actually caused drag on the root of the overlying continental lithosphere (Jones et al. 2011). This so-called magmatic gap occurred because the subducted slab was in contact with relatively cool continental lithosphere, rather than hot asthenosphere (Dumitru et al. 1991). And another result of the shallow subduction angle and drag on the continental root was that it caused a broad belt of mountains, some of which became the Rocky Mountains.
Dickinson (1981, 125) summarized how this concept of flat-slab subduction of the Farallon plate under western North America would have “played out” (fig. 2):
(1) The belt of magmatism moved inland as the locus of melting near the top of the subducted slab shifted away from the subduction zone;
(2) Magma generation waned as slab descent became sub-horizontal because the slab no longer penetrated as deeply into the asthenosphere; and
(3) Shallower descent of the slab increased the degree of shear and the area of interaction between the descending slab and the overriding cratonic crust (fig. 2c).
As rapid subduction took place, the subducted hot, buoyant, oceanic Farallon plate would have underplated North America as far east as the Great Plains, thereby contributing to the uplift of the West. The area that was to become the Colorado Plateau was caught in the eastward compressing Laramide cordillera.
Numerous prior major tectonic episodes during and since the Proterozoic had stressed the relatively stable Colorado Plateau region, producing a network of faults (Karlstrom and Timmins 2012). In each case, the stresses were different, and the resulting fault networks had different orientation and style. Walcott (1890) was the first to recognize that reactivation of Proterozoic faults occurred during the Laramide orogeny. Due to the compressional stress during the Laramide orogeny, what had been normal faults in the Proterozoic became high-angle (steeply dipping) contractional reverse faults, such that older Paleozoic rocks on the west sides of fault lines were pushed up over younger Paleozoic strata on the east sides. Hence Laramide compressional structures have been called basement-cored “thick-skinned” structures, referring to the fact that Proterozoic crystalline basement rocks were pushed upward along faults.
The Laramide orogeny thus profoundly impacted the Grand Canyon region (Huntoon 2003; Karlstrom and Timmins 2012). It caused widespread uplift, east-northeast crustal shortening, compartmentalization of the Colorado Plateau into subsidiary uplifts and basins, and widespread erosion. This resulted in the development of generally north-striking, east-dipping monoclines as the underlying basement failed along the major Proterozoic faults in response to east-northeast contraction (fig. 3). These monoclines were essentially “forced folds” of the Paleozoic strata due to the upward movement of the underlying basement blocks on high-angle normal faults forcing the overlying Paleozoic strata to bend passively into steeply dipping limbs (the monoclines) separating flat-lying beds of the upthrown blocks from the flat-lying beds of the downthrown sides. Laramide monoclinal folding in the Grand Canyon region was accompanied by mild regional warping of the intervening structural blocks, resulting in uplifts such as the Kaibab Plateau and downwarps such as the Cataract Basin (fig. 3).
Erosion accompanied the uplift of the Laramide orogeny. It progressively uncovered older rocks to the south and west, including the Precambrian basement along the southwestern edge of the Colorado Plateau region. The enormous volume of detritus from Mesozoic strata eroded off of the Grand Canyon region and areas to the south was apparently transported northeastward into the intracontinental basins of Utah and beyond.
In the Early Eocene there was a northeastward reorientation of Laramide compressive stresses within the Colorado Plateau region (Chapin and Cather 1983). This caused 100 km (~60 mi) of north-northeast translation of the Colorado Plateau along right-lateral, strike-slip faults that partially decoupled the Colorado Plateau from the North American continent along the future Rio Grande Rift. This Early Eocene reorganization of stresses appears to have resulted in minor development, or reactivation, of northwest-trending monoclines in the Grand Canyon region.
Grand Canyon Monoclines
Most Laramide monoclines in Grand Canyon region formed in the Paleozoic sedimentary cover strata in response to reverse movements along favorably oriented faults in the Precambrian basement (Huntoon 2003) (fig. 4). Three lines of evidence demonstrate that most faults under the monoclines were inherited from Precambrian time:
(1) Juxtaposition of Precambrian basement crystalline rocks having different lithologies and fracture-foliation fabrics (Karlstrom et al. 2003) that cannot be restored by removal of Laramide offsets;
(2) Juxtaposition of the overlying Precambrian Supergroup strata that cannot be restored to pre-fault conditions by removal of Laramide offsets; and
(3) Presence of the Early Cambrian, potentially synorogenic, Sixtymile Formation (Karlstrom et al. 2018, 2020) along the west side of the Butte fault in eastern Grand Canyon.
Total crustal shortening resulting from the deformation within the monoclines was less than one percent across the Grand Canyon region (Davis 1978). There are two reasons for this low percentage, namely, the spacings between the monoclines are large in comparison to the local shortening across them, and the dips of the underlying Precambrian faults are steep.
The maximum offset across a Grand Canyon monocline is at least 750 m (~2,500 ft) along the East Kaibab Monocline (Huntoon 2003). The longest monocline, the East Kaibab Monocline, is ~300 km (~190 mi) long. The regional trends of the monoclines in the Grand Canyon region are generally north-south, and the east-west spacings between them vary from 11 to 50 km (7 to 30 mi). They are characterized by great sinuosity but they also tend to branch in en echelon patterns (figs. 3 and 5). For example, branching is well-developed along the East Kaibab Monocline. This includes the prominent northwest-trending Phantom-Grandview branch which splays from the main fold, and the Fossil-Monument-Eremita branch which is a weakly developed detached western extension that is segmented with intervening gaps exhibiting no discernible deformation. Such changes in the trend and the complicated branching are linked directly in outcrops on the floor of Grand Canyon to Precambrian fault patterns which have been reactivated (Huntoon 1993).
Most segments of Grand Canyon monoclines are developed in the Paleozoic section over a single, high-angle reverse fault in the Precambrian basement (Huntoon 2003) (fig. 4). Laramide displacements are along the faults and generally produced abrupt offsets at the top of the Precambrian basement. The dips of the faults are typically between 60° and 70°. In profile, the anticlinal and synclinal axial surfaces in the monoclines converge downward on, and terminate against, the underlying faults at or below the Precambrian-Cambrian contact. Consequently, the dips of the strata increase and the widths of the folds decrease with depth in the monoclines. The heights to which the faults propagated into the overlying Paleozoic strata are proportional to the offsets at the Precambrian-Cambrian contact. The displacements on the faults gradually attenuated with elevation largely through apparent ductile deformation of the Paleozoic rocks so that they rarely extend above the top of the Supai Group. Deformation in close proximity to the faults at the cores of the monoclines includes (fig. 4):
(1) Minor horizontal shortening folds and kink bands in the footwall block;
(2) Highly localized drag-folding adjacent to the fault surface; and
(3) Numerous conjugate sets of minor thrust faults.
Shortening across a monocline at all levels is equal to the heave of the Precambrian-Cambrian contact across the underlying reverse fault (Huntoon 2003).
Where the Paleozoic rocks were deposited directly on the crystalline basement rocks, the strength of the unfaulted crystalline rocks tends to be isotropic, being the same regardless of direction prior to failure. In contrast, the Grand Canyon Supergroup sedimentary strata are highly anisotropic as a result of their bedding, especially in the Chuar Group. However, the Paleozoic beds in the monoclinal limbs can be strongly thinned, owing to slip on bedding planes and braided networks of minor faults, and, with continued slip, can even be overturned and mimic the dips of the master faults (Karlstrom and Timmins 2012).
Monocline profile variations are most easily observed by the degree of folding of the Precambrian-Cambrian contact in the hanging wall block, as well as by the level within the fold where the anticlinal axial surface converges on the reactivated fault. An ideal monocline is one developed over a single reactivated fault that dips at 60° and is contained wholly within isotropic, rigid, crystalline rocks. Reactivation of the fault under the monocline produced a step-like offset at the Precambrian-Cambrian contact (fig. 4a). Both the anticlinal and synclinal axial surfaces in the overlying fold converge downward on the intersection between the Precambrian-Cambrian contact and the fault surface on the respective sides of the structure. Thus, the Precambrian-Cambrian contact remains planar, and the fold does not extend down into the Precambrian crystalline basement.
In contrast, the Precambrian-Cambrian contact in the hanging wall is folded downward toward the reactivated fault in locations where Grand Canyon Supergroup strata are preserved in the hanging wall block (fig. 4b). Dips of the contact in the hanging wall block adjacent to the fault range up to 20°. The degree of flexing and setback of the anticlinal hinge from the fault increase in proportion to the thickness of the underlying Supergroup section. This variant is a function of the considerably greater ductility of the Grand Canyon Supergroup sedimentary strata in contrast to the rigidity of the crystalline rocks. The Precambrian-Cambrian contact in the footwall block remains essentially planar until it very closely abuts the reactivated fault regardless of whether sections of the Supergroup strata are present in the footwall block. Consequently, the synclinal axial surface always converges on the intersection between the contact and the fault surface in the footwall block in the monoclines.
The stress regime responsible for the development of the monoclines involved east-northeast-oriented maximum principal stresses and vertical minimum principal stresses. Orientations of the maximum principal stresses have been deduced from conjugate shear fractures in both Precambrian and lower Paleozoic rocks at numerous locations along the monoclines (Huntoon 1993). According to Huntoon (2003) the conjugate shears occur at all scales from microscopic (for which he provided no photomicrographs as evidence) to mesoscopic, and they appear as intersecting second-order thrust faults. In contrast to the second-order thrusts, the basement failed along steeply dipping first-order Precambrian normal faults that were already in place to accommodate Laramide strain. The presence of these weaknesses rendered the rocks anisotropic, which destroys the relationship between the principal stress and fracture orientations predicated by Hubbert (1951). Consequently, the dips of the reactivated faults do not reveal information about the Laramide stress regime.
It is difficult to establish the timing for the inception of monoclinal folding in the Grand Canyon using stratigraphic evidence because the Late Cretaceous section has been eroded from the region. However, Late Cretaceous rocks containing unconformities are present in the southern high plateaus of Utah and elsewhere in the Rocky Mountains region, and these establish a Maastrichtian initiation for Laramide deformation (Anderson et al. 1975; Dickinson et al. 1987). The Grand Canyon region was undergoing concurrent uplift. The beveling of some Grand Canyon monoclines indicates they were developing concurrently with the regional upwarping that produced those unconformities in Utah.
An analysis of apatite fission-track thermochronology data collected from Grand Canyon rocks led Naeser et al. (1989) to conclude Laramide uplift and monoclinal folding commenced about 60 million years ago followed by a second pulse of uplift beginning in Late Eocene time between 40 and 35 million years ago. Dumitru, Duddy, and Green (1994) also interpreted their apatite fission-track thermochronology data as recording two phases of cooling of Grand Canyon rocks, one during the Laramide deformation at 70 Ma, and another at 50–30 Ma. Flowers, Wernicke, and Farley (2008) used apatite (U-Th)/He thermochronology data to constrain the <70°C cooling history of eastern Grand Canyon as denudation occurred during and after the Late Cretaceous Laramide orogeny with a more recent cooling event occurring after ~25 Ma. Kelley and Karlstrom (2012) added further apatite fission-track thermochronology data for Paleozoic strata of eastern Grand Canyon and likewise concluded exhumation occurred during the Late Cretaceous (90–70 Ma) Laramide deformation, followed by further exhumation at ~25–17 Ma. These findings are consistent with the timing of tectonism deduced from the incomplete stratigraphic record.
The East Kaibab Monocline
One of the largest monoclines in the Colorado Plateau is the East Kaibab Monocline, named by Powell after the Native American word “Kaibab,” which means “mountain buried below” (Reches 1978a). The East Kaibab Monocline structure is ~300 km (~190 mi) long and is composed of flexures, folds and faults (figs. 3, 5, and 6). Its exposure changes laterally from a smooth flexure to a fault to a combination of fault and flexure. It trends generally north-south from the Bryce Canyon area, Utah, to San Francisco Peaks, Arizona, but locally trends east. The maximum offset along the East Kaibab Monocline is at least 750 m (~2,500 ft), the most of any Grand Canyon monocline (Huntoon 2003), while its vertical displacement ranges up to 1,200 m (~3,935 ft) (Reches 1978a).
The East Kaibab Monocline is conspicuously sinuous like so many of the Grand Canyon monoclines, being systematically curvilinear as a composite of north-northwest-and north-northeast-trending segments (Davis 1978). Branching is also well developed along the East Kaibab Monocline, with the prominent Phantom-Grandview branch and the weakly developed, detached Fossil-Monument-Eremita branch that is segmented with intervening gaps exhibiting no discernible deformation (Huntoon 2003).
The Colorado River, Grand Canyon, and their tributaries or side canyons cut through the East Kaibab Monocline and provide three-dimensional exposures for about 30 km (~19 mi) along the structure (Reches 1978a). The Butte Fault is intermittently exposed beneath the flexure for about 18 km (~11 mi), providing opportunities to study the fault-fold relations also. Fig. 5 is a tectonic map of eastern Grand Canyon which shows the main features of the East Kaibab Monocline system, while fig. 7 depicts the geologic history of the underlying Butte Fault. West of Lava Chuar Hill, the East Kaibab Monocline splits into two branches, one of which continues southward, and the second of which trends southeastward into Palisades Creek. About 4 km (~2.5 mi) of the first branch appears as the Butte Fault in Precambrian units. Some remnants of the overlying Paleozoic strata indicate that this segment of the Butte Fault was not active after Precambrian time (Walcott 1890, 56). The second branch is now known as the Palisades Fault because it lies along Palisades Creek, where one can observe the transition from fault to continuous flexure in the Paleozoic strata (fig. 5). The two branches of the East Kaibab Monocline rejoin southeast of Desert View (fig. 3).
The thicknesses of the Cambrian through Pennsylvanian strata (Tapeats Sandstone through the Supai Group) between the anticlinal and synclinal axial surfaces in the East Kaibab Monocline are attenuated between 30% and 60% (Huntoon 2003). This contrasts with comparatively gentle dips of less than 15° with virtually no attenuation at the level of the Permian strata (Hermit through Kaibab Formations). Those Permian strata occupying the anticlinal hinge are rarely thinned by brittle failure in the form of downward propagating grabens because of space-compensating horizontal shortening across the monocline. The Precambrian-Paleozoic contact in the footwall block to the east of the East Kaibab Monocline is broadly flexed for the ~5–8 km (~3–5 mi) in the area immediately north of Grand Canyon. The flexing adds ~300 m (~1,000 ft) of structural relief to the fold where it is best developed. Furthermore, the Precambrian-Paleozoic contact in the hanging wall is folded down toward the reactivated Precambrian Butte Fault, with dips up to 20° adjacent to the fault, in locations where the Grand Canyon Supergroup strata are preserved in the hanging wall block.
Reches (1978a) used a variety of stress indicators to determine that the average orientation of the maximum principal stress was N76°E along the Palisades segment of the East Kaibab Monocline. His analysis used stress orientations deduced from the Paleozoic strata from calcite twinning, minor faults, kink bands, and minor folds.
Davis and Tindall (1996) deduced that there had been a component of right-lateral strike-slip motion along the Precambrian basement fault underlying the northern part of the East Kaibab Monocline. Their findings were based on the orientations and motions along minor faults in the Cretaceous strata within the fold. They estimated that lateral slip was as much as three times the vertical offset at that location, consistent with the motion expected along a reactivated basement fault that was not oriented perpendicular to the minimum principal stress.
The history of tectonic activity along the East Kaibab Monocline was outlined by Walcott (1890) in a study on the eastern Grand Canyon. According to Walcott, movement along the trend of the East Kaibab Monocline began in the Grand Canyon region as a Precambrian fault, downthrowing older, “Algonkian” strata on the west from 15 to 1,500 m (~49 to ~4,920 ft). During the late Paleozoic, the sense of displacement on the Precambrian basement fault reversed and an eastward-facing monoclinal fold was formed, displacing strata a few tens of meters. The same sense of movement resumed during the Cenozoic, producing the East Kaibab Monocline and the accompanying faults. The net displacement aggregated more than 900 m (~2,950 ft) in the vicinity of Grand Canyon.
The Carbon Canyon Fold
The prime example of the folds in question is the folding of the Cambrian Tapeats Sandstone (Middleton and Elliott 2003; Snelling 2021) where those sandstone beds were dragged upwards into, against, and by the Butte Fault at the synclinal hinge of the East Kaibab Monocline in eastern Grand Canyon during the Laramide orogeny (Huntoon 2003; Karlstrom and Timmins 2012). The best exposed fold in this system is in Carbon Canyon (figs. 1 and 8). As the name indicates, the Carbon Canyon fold is exposed in Carbon Canyon, a side canyon to Grand Canyon through which flows Carbon Creek, a tributary of the Colorado River at river mile 65 from Lees Ferry (figs. 1 and 9). Access to the fold requires hiking ~1.6 km (~1 mi) up the usually dry drainage of Carbon Creek from the Colorado River, including a climb up a steep scree slope ~76 m (~250 ft) high to navigate around a usually dry waterfall.
The Proterozoic Nankoweap Formation of the Grand Canyon Supergroup crops out along the Colorado River at the mouth of Carbon Canyon, but the climb up Carbon Creek passes through the Great Unconformity up into the overlying Tapeats Sandstone (fig. 9). Carbon Canyon then narrows with the Tapeats Sandstone forming its walls. The canyon then stops abruptly at the Butte Fault and beyond it is an open valley in which beds of the Proterozoic Galeros Formation of the Grand Canyon Supergroup are exposed in an open syncline. At the Butte Fault the Tapeats Sandstone beds have been dragged up by it and upturned through a ~90° fold (figs. 8 and 9).
Hill and Moshier (2009) claim that evidence from field studies and rock deformation experiments demonstrates that these solid rocks behaved in a ductile manner as the sandstone beds in this fold were deformed slowly under great stress, and that the beds thus were “bent” by microscopic reorientations of mineral grains and by changes in bedding thickness along the fold. They then reference Huntoon (2003) to state that these tight folds in beds of the Tapeats Sandstone in Carbon Canyon can be explained by mechanical crowding at the synclinal hinge of the East Kaibab Monocline during slow deformation under stress of the solid sandstone in a ductile manner.
However, Hill and Moshier (2009) offer no supporting evidence of these claims. They provide no documentation of the quoted rock deformation studies, nor any evidence from any thin section examination of the Tapeats Sandstone from this fold of the claimed microscopic reorientations of mineral grains. And the only documentation they provide of any field studies is a single photograph of the vertical beds of the Tapeats Sandstone at the Carbon Canyon location, but not of the folded beds showing the mechanical crowding. For that they refer to Huntoon (2003), but his field photograph, while showing the bent beds of the Tapeats Sandstone at the location in question, is incorrectly labeled as the south wall of Chuar Canyon, when it is in fact the south wall of Carbon Canyon. Furthermore, Huntoon (2003) also did not provide any thin section evidence for any reorientation of mineral grains.
Subsequently, Tapp and Wolgemuth (2016) similarly focused on the Carbon Canyon fold. They showed a photo of the fold (page 125, their fig. 12–13), describing it as compressional folding in the Tapeats Sandstone (fig. 10). On an overlay they traced some of the sandstone beds through the fold, some of the fractures, and the apparent changing direction of the fold hinges, which they claimed to be due to flexural slippage. They claimed that the bending resulted in numerous fractures in each sandstone bed that did not heal (reseal). They then illustrated what flexural slippage would look like in two hypothetical folds (page 125, their fig. 12–14), describing how flexural slippage creates gaps in the fold hinges that may be filled in later with weathered material or weaker rock may deform into the spaces (fig. 11). Either way, the layering in the fold hinges would be thicker relative to the widths of the sandstone beds along the fold limbs. They claimed that neither of these features would be present if this fold had occurred due to soft-sediment deformation. However, their photo of the fold shows no such thickening of the sandstone beds in the fold hinges, and they fail to discuss alternate explanations for the fractures, such as joints due to horizontal contraction within the beds during dewatering and lithification, and especially due to unloading with erosion of the side canyon. Additionally, there is also no evidence of thickening of shale-rich beds in the Bright Angel Formation where they are folded.
The Tapeats Sandstone
Snelling (2021) provided a detailed review of past investigations of the Tapeats Sandstone, including its stratigraphy, trace fossils, sedimentary structures, U-Pb detrital zircon ages, provenance, and depositional environment. Additionally, based on the detailed petrographic study of his 26 samples collected from two folds and several locations distal to them, Snelling (2021) documented and described in detail the mineral grains and textures within the sandstone, then discussed his findings to draw conclusions as to the petrology of the Tapeats Sandstone.
The Tapeats Sandstone is the generally 30–100 m (98–328 ft) thick cliff-forming unit that prominently crops out through ~500 km (~310 mi) in the walls of the Grand Canyon, Arizona, and beyond (Elston 1989; Hagedorn et al. 2011; McKee 1945; Noble 1914, 1922; Rose 2003, 2006, 2011). Up to 120 m (394 ft) thick, it is usually the basal formation within the fining upwards lithologies of the Cambrian Tonto Group, which has been touted conventionally as the classic example of the time-transgressive “deepening seas” sedimentation model. The Tapeats Sandstone mostly sits directly on a pronounced erosion surface known as the Great Unconformity, but locally unconformably overlies the breccias of the Sixtymile Formation, which has now been included in the Tonto Group (Karlstrom et al. 2018, 2020; Peters and Gaines 2012). The underlying rocks eroded at the Great Unconformity include granitic plutons intruded into the Granite Gorge Metamorphic Suite schists unconformably overlain by the tilted sedimentary strata and basalt layers of the Grand Canyon Supergroup, all dated as Precambrian (Karlstrom et al. 2003). Both the correlated equivalents of the Tapeats Sandstone and the Great Unconformity have been traced across several continents and around the globe, respectively (Clarey 2020; Peters and Gaines 2012).
Within the Tapeats Sandstone are found numerous trace fossils, primarily burrows and trails likely left by various worms and other invertebrates, and trails left by trilobites (Resser 1945). These are mostly found in the uppermost thin alternating sandstone and shale beds of the transition interval with the overlying Bright Angel Formation (McKee 1945). The prominent coarse-grained sandstone cliff-forming unit within the Tapeats Sandstone consists of 0.3–1.0 m (~1–10 ft) thick non-bioturbated beds that are strongly cross-laminated with shallow dips characteristic of water transport of the sand and many lens-shaped scour-and-fill “channels” (McKee 1940, 1945; Rose 2003, 2006; 2011). The predominant paleocurrent direction is between west and southwest. Detrital zircon grains extracted from the Tapeats Sandstone have been U-Pb dated to determine both the maximum depositional age of the formation, as well as the potential provenance of its sand (Gehrels et al. 2011; Karlstrom et al. 2018, 2020; Matthews, Guest, and Madronich 2018). Coupled with biostratigraphic trilobite faunal zones correlated globally, the Tapeats Sandstone has been dated at 507–508 Ma (early middle Cambrian) (Karlstrom et al. 2020). U-Pb age peaks among the detrital zircons matched the nearby Paleoproterozoic Yavapai and Mazatzal provinces, indicating the primary source of the sand grains was the locally underlying granitic plutons and schists, plus a very small portion from the underlying Grand Canyon Supergroup strata (though a long-distance transport of some grains cannot be entirely ruled out). The consensus uniformitarian interpreted depositional environments for accumulation of the Tapeats Sandstone are intertidal to subtidal shallow-marine environments with local beach and fluvial deposits (McKee 1945; Rose 2003, 2006, 2011), yet there is evidence of deep-water deposition (Chadwick and Kennedy 1998; Kennedy, Kablanow, and Chadwick 1997), and it has been described as “one of the most dramatic global marine transgressions in Earth history” (Karlstrom et al. 2018).
Snelling (2021) reported that quartz sand grains are the dominant component of the Tapeats Sandstone, but bulk rock XRD analyses of his 26 samples collected from bottom to top of its main cliff-forming unit confirmed K-feldspar contents ranging from 1.8–33.1%. In thin sections, the sandstone is poorly to moderately well-sorted and dominated by sub-angular to sub-rounded, coarse silt to very coarse sand-sized quartz grains, with some granules and small pebbles. Many variously sized K-feldspar grains are scattered through the rock fabric, with occasional thin edge-on detrital muscovite flakes wedged between quartz and K-feldspar grains, sometimes bent around them with frayed ends. Some samples contain a few plagioclase, rounded tabular zircon, and rare sphene grains. With very few pores remaining and the porosity generally 2–5%, the rock fabric is cemented by silica as quartz overgrowths. Snelling (2021) found no evidence, macroscopic or microscopic, of any metamorphic changes to the detrital mineral grains or textures. It is a well-cemented, unmetamorphosed, sub-mature arkosic sandstone.
Snelling (2021) concluded that these mineral constituents of the Tapeats Sandstone are consistent with the underlying local basement rocks being the source of the sand, as indicated by the detrital zircon U-Pb ages. The rare presence of mica schist and siltstone fragments within the sandstone underscored his conclusion that transport was over a short distance and likely rapid. Indeed, due to the very short-distance transport and deposition of the sand, K-feldspar grains and former laths are scattered randomly through the entire sandstone unit and are not always rounded, while the extremely soft detrital muscovite flakes have survived, sometimes bent with frayed ends. The thin, non-bioturbated, strongly cross-laminated beds, and eroded “channels” filled with cross-laminated sand, both including likely hummocky cross-stratification (McKee 1940, 1945; Rose 2003, 2006, 2011), are consistent with rapid sequential deposition by high-energy storm-like surges. Numerous detrital zircon grain U-Pb ages are considerably less than the designated depositional age of the Tapeats Sandstone (Karlstrom et al. 2018, 2020; Snelling 2021). These coupled with the well-documented problems with the many assumptions undergirding the U-Pb dating method (Snelling 2000), and the well-documented evidence of past grossly accelerated nuclear decay rates (Vardiman, Snelling, and Chaffin 2005), totally undermine the validity of the conventional age for the Tapeats Sandstone. Instead, Snelling (2021) found that when combined, the mineralogical content, textural features, sedimentary structures, continental-scale deposition, paleocurrent directions identical to the same continental pattern, and even the tracks and traces of transitory invertebrates that had to be buried and fossilized rapidly, are all consistent with the catastrophic erosion of the Great Unconformity near the onset of the global Genesis Flood cataclysm about 4,350 years ago and the tsunami-driven rapid short-distance transport and deposition of the Tapeats Sandstone at the base of the fining upwards Sauk megasequence in the first few days or weeks of that year-long event.
Folding Mechanisms in Folds
It has been claimed that the Tapeats Sandstone was bent in the Carbon Canyon fold by ductile deformation (Hill and Moshier 2009; Huntoon 2003; Tapp and Wolgemuth 2016). By ductile deformation they presumably mean continuous deformation at the scale of observation in which the rock flowed under the influence of stress without macroscopic fracturing (Fossen 2016). They make no mention of any possible accompanying metamorphism due to elevated temperatures at the depth of burial. As summarized by Paterson (2001), ductile flow of rocks can occur by the following three mechanisms:
(1) Change of shape of grains by crystal plasticity, which is referred to as dislocation creep;
(2) Change of grain shape by diffusion through or around grains, called diffusion creep; and
(3) Relative movement of grains, referred to as granular flow or grain-boundary sliding.
In (3), in order to minimize the formation of voids (dilatancy), the grains must change their shapes by mechanism (1) or (2). Except for these local accommodations, very large strains may be achieved without change of overall grain shape, as in “superplastic flow” in very fine-grained aggregates.
Thus, where folding of sedimentary rock units has occurred subsequent to their diagenesis and deep burial, ductile deformation during folding of the otherwise brittle rock can be facilitated by grain-boundary sliding and bedding-plane slip and attenuation. The role of grain-boundary sliding has been thoroughly investigated theoretically, experimentally, and in field situations, and the resulting macroscale and microscopic features of rock textures and mineral grain characteristics are well documented (Bestmann and Prior 2003; Billia et al. 2013; Etheridge and Wilkie 1979; Gratier et al. 2011; Hansen, Zimmerman, and Kohlstedt 2011; Hippertt 1994; Hiraga et al. 2013; Jackson 2009; Jackson, Faul, and Skelton 2014; Langdon 1970; Lee and Morris 2010; Lee, Morris, and Wilkening 2011; Massey, Prior, and Moecher 2011; Menegon et al. 2015; Morris and Ree 1994; Sundberg and Cooper 2010; Vernon 2018; Watanabe et al. 2013; Wojtal, Blenkinsop, and Tikoff 2022). Similarly, bedding-plane slip and attenuation have been demonstrated to facilitate folding without brittle fracturing, being simulated with numerical modeling and well-studied in laboratory and field settings (Becker 1994; Behzadi and Dubey 1980; Borja, Sama, and Sanz 2003; Chapple and Spang 1974; Cooke and Pollard 1997; Cooke et al. 2000; Cooke and Underwood 2001; Couples and Lewis 2000; Crook et al. 2006; Epard and Groshong 1995; Horne and Culshaw 2001; Hughes and Shaw 2015; Kuenen and de Sitter 1938; Nino, Philip, and Chery 1998; Ramsay 1974; Roth, Sweet, and Goodman 1982; Sanz et al. 2008; Suppe 1983; Suppe and Medwedeff 1990; Tanner 1989).
Furthermore, the pressures inherent in the folding process have also been shown to cause elastoplasticity and visco-elastic compression of the particle matrices within sedimentary rocks which facilitates accommodation of the volume changes in the hinges and limbs of the resultant folds (Benesh et al. 2007; Borja 2006; Cundall and Strack 1979; Erickson and Jamison 1995; Guiton, Leroy, and Sassi 2003; Matsuoka and Nakai 1974; Mühlhaus et al. 2002; Sanz, Borja, and Pollard 2007; Simo and Taylor 1985). The effects of all of these processes on the rock fabric and texture, and on the rock matrix and its mineral grains, can be observed and documented in the outcropping folds and under the microscope in rock sections.
Rock deformation laboratory studies have demonstrated that solid rock deforms in a ductile manner slowly under stress (Davis and Reynolds 1996; Friedman et al. 1976; Friedman, Hugman, and Handin 1980; Gangi, Min, and Logan 1977; Ghosh 1968; Griggs 1936, 1939; Handin et al. 1976; Weinberg 1979), but mechanical crowding and thinning of sandstone beds at the macroscopic scale is not definitive proof that the folding occurred slowly under stress as the lithified sandstone beds were deformed in a ductile manner. It is also readily demonstrated in such laboratory studies that beds of soft sand will similarly be crowded and thinned mechanically when deformed while still soft due to the confining pressures in the hinges of the folds (Borg and Maxwell 1956). Only if thin section examination of the sandstone reveals deformation lamellae and undulose extinction in the quartz grains under cross-polarized light due to deformation stress (Bailey, Bell, and Peng 1958; Carter 1971; Carter, Christie, and Griggs 1964; Christie and Ardell 1974; Christie, Griggs, and Carter 1964; Davis and Reynolds 1996; Fairbairn 1939; Groshong 1988; Hansen and Borg 1962; Hansen, Borg, and Maxwell 1959; Mitra and Tullis 1979; Tullis, Christie, and Griggs 1973; Twiss 1974, 1976; Whisonant 1970; White 1973a, b) will it have been demonstrated that the mechanical crowding of the sandstone beds in these folds has been due to slow deformation under stress of solid sandstone.
Detailed field and laboratory studies are always needed to resolve the questions of what condition the sandstone was in when it was deformed into folds, and thus how the deformation occurred. Such field studies should involve careful documentation and analysis of the folding and faulting (Aydin and Johnson 1983; Davis and Reynolds 1996; Groshong 1988; Hafner 1951; Reches 1978b; Reches 1983; Reches and Dieterich 1983; Reches and Jessell 1988a, b) and would require sampling of the sandstone so that thin sections could then be prepared for detailed microscope examination. For control purposes the same sandstone beds need to be sampled from areas distant from the folds so as to compare under the microscope the grains and rock fabric/texture in those distal sandstone samples with those in the samples obtained from the folds.
Expected Macroscopic Features Due to Ductile Deformation
Though somewhat similar, two classification schemes of folds have been proposed. Donath and Parker (1964) classified folds according to a generic-mechanical scheme based on mean ductility and ductility contrast within the folded sequence of layers (Hatcher and Bailey 2020) (fig. 12a). Accordingly, there are two broad groups of folds—flexural folds in which the fold shape is determined by the layering in the rocks, and passive folds in which the layering only serves as a displacement marker during folding (fig. 12b). A second, broad twofold subdivision is fundamentally a separation of brittle from ductile behavior. Slip along bedding, cleavage or foliation planes is important in forming brittle folds. The process of ductile flow dominates in passive folds. Thus, in flexural-slip folds, layer thicknesses remain constant, and folding is accomplished by slip along and between layers. They are easily recognized by slickensides, fibers, or other movement indicators such as slip lines or lineations on layer surfaces, and by constant layer thickness (Hatcher and Bailey 2020). In flexural-flow folds, the stronger beds change thickness little or not at all, while the weaker beds undergo appreciable thickness changes, and cleavage is strong in the weak layers but poorly developed in the strong layers. Thus, some beds were thickened in the hinge (axial) zones and thinned into limbs as folding proceeded, indicating a higher contrast in internal ductility. In contrast, passive-slip folds are ideally developed by movement parallel to a strong cleavage or shearing along planes, both of which are inclined to the layering. And finally, passive-flow folds develop by ductile flow due to plastic deformation so that the fold limbs are thinned and the hinges are relatively thickened equally in all rock types, thus producing similar folds.
However, Ramsay (1967) subsequently classified folds into several classes based instead on their descriptive geometric shapes as determined on their profiles perpendicular to their hinge zones (Fossen 2016; Hatcher and Bailey 2020) (fig. 13). His classification involves an indirect relationship between layer thickness, both perpendicular to the layering and parallel to the fold axial surface, and the angle of dip at different points on successive folded surfaces. Lines connecting points of equal dip across a layer are called dip isogons. The relative convergence, divergence, or parallelism of dip isogons is the classification key, with the degree of convergence of isogons directly related to fold tightening. Thus, folds where the isogons converge towards the concave part of the fold are classified as Class 1 folds, folds with parallel isogons belong to Class 2, and folds with isogons that diverge toward the concave part of the fold are in Class 3 (fig. 13). Class 1 folds are further subdivided into three groups. Class 1A folds have strongly convergent isogons which change direction through distance along the bedding more than the dip of the bedding surfaces they connect (fig. 13a). Class 1B folds correspond to parallel-concentric folds with convergent isogons which change direction the same as the bedding surfaces they connect (fig. 13b). And Class 1C folds are modified similar or parallel folds that have weakly convergent isogons which change direction less than the bedding surfaces they connect (fig. 13c). Then, Class 2 folds are ideal similar folds in which the isogons are parallel (fig. 13d), while Class 3 folds have extremely thickened hinges or extremely thinned limbs in which the isogons change direction in the opposite sense to the bedding surfaces they connect (fig. 13e).
Fossen (2016) noted that Class 1B folds are due to active folding, buckling, or bending that was initiated when the layers were shortened parallel to the layering. A contrast in competence or viscosity between the folding layers and their host rock is required for the folding to have occurred, with the folding layers evidently more competent than the host rock or matrix. Fossen (2016) also equated Ramsay’s (1967) Class 1B folds with Donath and Parker’s (1964) flexural folding. Furthermore, Fossen (2016) distinguished bending, where the forces act across layers at a high angle, from buckling, where the main forces act parallel to the layers. He then cited the classic geologic results of bending as the forced folds created in sedimentary layers blanketing faulted rigid basement blocks. Displacement is forced on the sedimentary layers by movements along preexisting faults, and the sedimentary layers are soft enough to respond to monoclinal folding until at some critical point they rupture and the faults start propagating up-section, for example, the Laramide-uplift created monoclines of the Colorado Plateau (fig. 14). In contrast, Fossen (2016) equated Donath and Parker’s (1964) passive folding with Ramsay’s (1967) Class 2 folds in which the layering exerts no mechanical influence on the folding due instead to passive flow occurring. Thus, passive folds form in response to any kind of ductile strain, whether shearing, transpression, or even coaxial strain.
Bedding plane or flexural slip implies slippage along interfaces between layers or along thin layers during folding with bed thickness maintained and is the dominant mode of folding at the low temperatures and pressures at shallow depths in the upper crustal brittle regime (Fossen 2016; Hatcher and Bailey 2020). As already noted, bedding plane or flexural slip has been demonstrated to facilitate folding without brittle fracturing, being simulated with numerical modeling and well-studied in laboratory and field settings, including along the East Kaibab Monocline (Becker 1994; Behzadi and Dubey 1980; Borja, Sama, and Sanz 2003; Chapple and Spang 1974; Cooke et al. 2000; Cooke and Pollard 1997; Cooke and Underwood 2001; Couples and Lewis 2000; Crook et al. 2006; Epard and Groshong 1995; Horne and Culshaw 2001; Hughes and Shaw 2015; Kuenen and de Sitter 1938; Nino, Philip, and Chery 1998; Ramsay 1974; Roth, Sweet, and Goodman 1982; Sanz et al. 2008; Suppe 1983; Suppe and Medwedeff 1990; Tanner 1989).
Furthermore, it is a prerequisite for flexural slip that the deforming medium is layered or has a strong mechanical anisotropy (Fossen 2016; Hatcher and Bailey 2020). Thus, for a layered sequence of beds to maintain constant thickness during folding, it must be uniformly strong rock such as bedded sandstone (for example, the Tapeats Sandstone) or carbonates so the beds can slip past one another. On the other hand, where the mechanical properties of successive layers differ (mechanical anisotropy), as with interlayered sandstone and shale, flexural slippage still occurs, but the shale may become thickened or even crumpled into the hinge zone of the folds without any ductile flow. In both cases the bedding surfaces act like fault planes and thus flexural slippage is easily recognized by slickensides or fibers on the slipped bedding surfaces. Maximum slip occurs at the inflection points and dies out towards the hinge line, where it is zero. The sense of slip is opposite on each limb, and the slip is constant relative to the hinge where the sense of the slip changes. Relative slip on the convex side of a flexural-slip fold is always towards the fold hinge, whereas the concave side slip is opposite. The net result is that the layering plays a pivotal role in parallel folding, the bending of massive sandstone or carbonate beds being an ideal example.
In contrast, a layered sequence of beds is said to deform by flexural flow if some beds flow ductilely, while others remain brittle and buckle or bend (Hatcher and Bailey 2020). Flexural flow requires moderate-to high-ductility contrast between layers. The whole rock mass may be in a state of ductile flow, but some rocks have higher viscosities under moderate temperatures (300–500°C) and higher pressures than interlayered weaker rocks. Such conditions do not apply to unmetamorphosed sedimentary rocks. The products of flexural flow are also mostly similar-type folds (Classes 1C and 3), and rarely ideal similar folds (Class 2). Similarly, passive flow involves uniform ductile flow of an entire rock mass, but there is no mechanical contribution from the rock material being deformed. Furthermore, there must be little or no ductility contrast between beds or layers, even if their compositions differ markedly, and there must be flow across the layering. Yet the necessary conditions for passive flow to occur similarly do not apply to unmetamorphosed sedimentary rocks, and the products are again similar and similar-type folds (Classes 2 and 3 and 1C respectively). And finally, passive slip as described by Donath and Parker (1964) and Ramsay (1967) as slip at an angle to the layering that produces new cleavage and schistosity does not apply to unmetamorphosed sedimentary rocks. In any case, it is now often considered as a problematical fold mechanism (Hatcher and Bailey 2020).
Therefore, the focus needs to be on what details might apply to the Tapeats Sandstone within the Carbon Canyon fold that should be observed at the macroscopic field scale. Such field observations that would classify the type of fold are also critical in determining the mechanism and the conditions under which the folding occurred. If flexural slip occurred after lithification during ductile deformation, then slickensides should be observed on the surfaces of the beds that moved relative to one another. Was there bed attenuation in the limbs or bed thickening in the hinges, and any mechanical crowding? Yet even after such field observations are made, it is the microstructures that are the best clues as to the conditions under which the folding occurred.
Expected Microstructures Due to Ductile Deformation
Vernon (2018) and Wojtal, Blenkinsop, and Tikoff (2022) reviewed the various mechanisms by which minerals and rocks undergo deformation, that is, change of shape and strain, at the scale of grains or small aggregates, with particular reference to the optical microstructures produced by each mechanism. To relate microstructures to deformation mechanisms, Vernon (2018) concluded:
(1) The microstructures produced by different deformation mechanisms must be known from natural and especially experimental observations; and
(2) The microstructures must be stable enough to survive subsequent deformation and/or heating events.
Furthermore, deformation mechanisms can be classified in various ways, but brittle and ductile deformation can be distinguished at the microscope scale.
In brittle deformation, fractures occur across and/or between grains, and the resulting fragments move relative to one another. Fig. 15 depicts the textures that would be observed under the microscope as a result of brittle deformation either by granular flow grain rotation and frictional sliding, which is common during deformation at shallow depths of porous sediments, or by cataclastic flow, which also produces micro-fracturing of grains during deformation of well-consolidated sedimentary and non-porous rocks (Fossen 2016). In ductile deformation, the grains change their shapes or move relative to one another without fracturing (loss of cohesion) at the grain scale (Passchier and Trouw 1996). In both situations, but especially during brittle deformation, a change of shape of an aggregate may be accomplished or assisted by dissolution of minerals at some sites, transfer of dissolved chemical components in solution, and deposition at other sites in the deforming aggregate, known as stress-induced solution transfer.
There is much documentation of the grain shapes and rock fabrics/textures in undeformed and deformed sandstones in both field, laboratory, and theoretical studies (Adams, MacKenzie, and Guildford 1984; Borg et al. 1960; Davis and Reynolds 1996; Etchecopar and Vasseur 1987; Friedman 1963; Gallagher et al. 1974; Hobbs 1968; Ingerson and Ramisch 1942; Jessell 1988a, b; Kamb 1959; Lister and Hobbs 1980; Lister, Paterson, and Hobbs 1978; Means 1990; Rowland 1946). There are also ample published studies on the effects on sand grains of their deformation under stress—deformation lamellae in the quartz grains and undulose extinction in quartz grains under cross-polarized light (Bailey, Bell, and Peng 1958; Carter 1971; Carter, Christie, and Griggs 1964; Christie and Ardell 1974; Christie, Griggs, and Carter 1964; Davis and Reynolds 1996; Fairbairn 1939; Groshong 1988; Hansen and Borg 1962; Hansen, Borg, and Maxwell 1959; Mitra and Tullis 1979; Tullis, Christie, and Griggs 1973; Twiss 1974, 1976; Whisonant 1970; White 1973a, b). Attention also needs to be paid during thin section examination of the samples from the folds for any evidence of thermal effects on the quartz grains, such as recrystallization, and on the matrix, such as conversion to metamorphic minerals (Carter, Christie, and Griggs 1964; Groshong 1988; Hobbs 1968; Lister and Hobbs 1980; Lister, Paterson, and Hobbs 1978; Mitra and Tullis 1979; Tullis, Christie, and Griggs 1973; White 1973a; Yardley, MacKenzie, and Guildford 1990).
Vernon (2018) and Wojtal, Blenkinsop, and Tikoff (2022) have provided details of the specific microstructures each of these mechanisms produces and which should be visible in petrographic examination of thin sections (fig. 16). Even though many of the illustrated examples they provide are of metamorphic rocks, the same observations are applicable to sandstones, and in particular, potentially to the Tapeats Sandstone within the Carbon Canyon fold.
Crystal Plasticity or Dislocation Creep
Crystal plastic flow is permanent deformation by non-cataclastic (ductile) flow, which involves slip (translation gliding) and/or deformation twinning, without loss of cohesion on the grain scale. These processes enable a grain to change its shape by allowing one part of the crystal to undergo shear with respect to a neighboring part (Hobbs, Means, and Williams 1976). Microstructural evidence of such crystal plastic deformation includes kink bands, deformation lamellae, and deformation twins (fig. 16).
These microstructures have been duplicated experimentally—for example, Carter, Christie, and Griggs (1964); Drury and Urai (1990); Etheridge and Hobbs (1974); Etheridge, Hobbs, and Paterson (1973); Griggs et al. (1960); Hirth and Tullis (1992); Hobbs (1968); Hobbs, McLaren, and Paterson (1972); Mares and Kroenenberg (1993); Tullis (1983); Tullis, Christie, and Griggs (1973); and Wilson and Bell (1979). Individual grains may become very elongated or may become converted to stretched out aggregates of much smaller grains formed by recrystallization during deformation. The mechanisms of crystal plastic flow in mineral deformation are summarized by Barber (1985); Barber and Meredith (1990); Gottstein and Mecking (1985); Green (1992); Hobbs, Means, and Williams (1976); and Knipe (1989).
Slip (Translation Gliding)
Slip is the main primary mechanism of deformation (Vernon 2018). It causes layers of a grain to slide past each other without fracturing and without changing the orientation of the slipped portion of the grain. Therefore, it cannot be detected in thin section, in contrast to deformation twinning in which a change of orientation is produced (fig. 17). However, the shape of the grain is changed in the slip process. Slip occurs on specific planes (commonly planes of dense atomic packing) and in specific directions in the crystal. A slip system is the combination of a slip plane and a slip direction in that plane. Slip systems have been determined for many minerals at various temperatures. Because of the crystallographic control of slip planes, ductile deformation of grain aggregates typically results in a strong crystallographic preferred orientation.
The ease with which a slip system operates depends on the strain rate and temperature (Vernon 2018). Some minerals with relatively high crystallographic symmetry, such as quartz and calcite, have several slip systems and can deform relatively easily over a range of conditions, especially at elevated temperatures of 400–600°C in the presence of water and above 700°C if dry. In contrast, many other minerals, such as mica and plagioclase, are of lower symmetry and may have only one dominant slip system, so they deform with greater difficulty. The more slip systems a mineral has, the more readily a grain of that mineral can change its shape in response to local differential stress. Minerals with at least five active independent slip systems can deform homogeneously by slip (Kelly and Groves 1970), quartz and calcite being common examples.
In grains of minerals with few slip systems, slip is commonly assisted by deformation twinning and kinking (fig. 16). In effect, a set of kink bands or of deformation twins acts as an additional independent slip system if repeated on a fine enough scale. Grains that are unfavorably oriented for slip may deform by fracturing and displacement along cleavages. Moreover, because of the common contrast between deformability of different minerals, local transient voids at grain boundaries may be relatively common, especially during deformation at lower temperatures. Those spaces may assist movement of fluid through the otherwise coherent rocks.
Slip takes place by movements of dislocations, as explained by Hobbs, Means, and Williams (1976) and Vernon (1976, 2000). Dislocations are line defects in which one row of atoms is decoupled from the rest of the lattice, effectively moving the dislocation through the solid crystal. The movement of dislocations through crystals enables solid crystalline materials to change their shapes without breaking. The stress on the mineral causes one row of atoms at a time to break. Then the next row breaks and the one behind it joins together again. So, successive rows break, one at a time, until the break (dislocation) moves right through the mineral grain, causing a displacement of one row of atoms. If many thousands of these minute displacements occur, they cause the mineral grain to change its visible shape. Each dislocation needs only a very small amount of energy, and the process does not require the mineral to change the overall arrangement of its atoms, so the mineral retains its identity during the deformation.
Kinking occurs when slip on a single slip plane is inadequate to maintain homogeneous deformation (Vernon 2018). The grain sharply bends (kinks) and the deformation localizes into kink bands, which enable shortening of the grain to continue (fig. 16). The whole grain may divide into kink bands, or the kink bands may be separate and commonly lenticular or wedge shaped. A kink band may be defined as part of a grain that undergoes rotation with respect to the unkinked part of the grain, the axis of rotation coinciding with the line of intersection of the kink band and the slip plane, perpendicular to the slip direction (Nicolas and Poirier 1976; Spry 1969).
Kink bands in a mineral grain are usually revealed by differences in absorption color, owing to their orientation differences. The widths and degrees of misorientation of the kink bands are variable, which distinguishes them from deformation twins, between which the misorientation is constant. By contrast, deformation lamellae are regularly spaced “lines” across a mineral grain, while deformation twins are also regularly spaced bands that can be lenticular (fig. 16). Broadly similar microstructures, reflecting heterogeneous deformation from one layer to another in a deforming grain but which cannot be described as kink bands according to their definition, are best referred to as deformation bands (Hobbs, Means, and Williams 1976; Spry 1969) (fig. 16).
Elongate sub-grains (extinction bands) formed by recovery in quartz are often referred to as “kink bands,” but should not be confused with kink bands formed by slip alone (Nicolas and Poirier 1976). Elongate sub-grains and true kink bands may be present in the same grain of quartz. Kinking is common in minerals with strongly anisotropic crystal structures and consequently only one slip plane, such as biotite, but also occurs in minerals with several slip systems, such as quartz (Christie, Griggs, and Carter 1964).
Deformation lamellae are narrow (0.5–10 µm), planar, crystallographically oriented zones with slightly different refractive index from that of the adjacent grain (Blenkinsop and Drury 1988; Carter 1971; Carter, Christie, and Griggs 1964; Christie, Griggs, and Carter 1964; Drury 1993; Green and Radcliffe 1972; Hobbs, Means, and Williams 1976; Turner 1948; White 1973b) (fig. 16). Deformation lamellae parallel to slip planes have been produced experimentally, but some natural deformation lamellae have complicated and variable structures and may not reflect slip alone.
Deformation lamellae generally are aligned perpendicular to extinction bands (elongate sub-grains). They are most common in quartz but have also been observed in plagioclase (Borg and Heard 1970) and calcite (Turner 1948). They tend to be formed most commonly during lower-temperature deformation. Deformation lamellae typically occur in one plane in quartz and may be slightly curved. They are generally visible due to their slightly different extinction and/or relief (refractive index) compared to the host grain and are often very closely spaced (on the order of their width) (Wojtal, Blenkinsop, and Tikoff 2022). They may be pervasive across a whole grain or localized into smaller domains. They form parallel to crystallographic planes (for example, parallel to the rhomb planes in quartz), and they may occur in more than one set in a grain.
Deformation Twinning (Twin Gliding)
Some minerals, such as calcite and plagioclase, undergo deformation twinning (mechanical twinning, secondary twinning, or twin gliding) in response to deformation (Vernon 2018) (figs. 16 and 17). The distribution of these twins within grains is typically heterogeneous. Deformation twinning operates by a limited amount of simple shear (at the microscopic scale, though it may be more complicated at the atomic scale) parallel to a glide plane (the twin plane) and in a particular direction (the glide direction), both of which depend on the crystal structure of the mineral, and which together constitute the twinning system. Thus, deformation twinning occurs in some minerals but not in others. In contrast to slip, the amount of deformation that can be achieved by twinning is limited by these requirements, especially because twins have only one sense of shear. Each atomic layer is sheared (not translated) by an amount sufficient to produce a mirror image of the original crystal (fig. 17). This restores the original structure, each half of the twin being misoriented symmetrically with respect to the other.
Twinning tends to be favored over slip at lower temperatures and faster strain rates (Vernon 2018). Deformation (secondary) twins are distinguished from growth (primary) twins on the basis of their typically lenticular shapes. Deformation twins are always multiple, never simple, and have been produced experimentally in calcite and plagioclase (fig. 16). Deformation twinning is common in plagioclase, where it occurs according to two “twin laws,” namely, albite-law twinning and periclase-law twinning, Both of these twin laws are favored by the same local stress system, and so they tend to operate simultaneously (Vernon 1965). Another example is calcite (Paterson and Turner 1970). Burkhard (1993) reviewed deformation twinning in calcite, inferring that micro-twins and straight, narrow twins (<1 µm thick) are characteristic of very low temperature deformation, whereas above about 100°C wider (>1–5 µm), fewer twins occur. Above ~200°C, curved twins, twins that are themselves twinned and completely twinned grains occur, and above ~250°C, older twins commonly show evidence of boundary migration. Deformation twinning also occurs in dolomite, and oxide minerals, such as rutile and hematite (Hennig-Michaeli 1977).
Hardening and Softening During Deformation
Broadly speaking, crystal plasticity may be divided into low-and high-temperature types (Vernon 2018). Low-temperature plasticity occurs at less than roughly half the melting temperature at laboratory strain rates and is dominated by glide of dislocations in slip planes. This leads to interference, tangling and hence immobilization of dislocations, causing the mineral to resist strain. Thus, the process is called strain hardening (strengthening). High-temperature plasticity is dominated by thermally activated recovery and recrystallization processes, which cause softening (weakening). The process involves untangling of dislocations, and consequently the mineral is able to continue to deform (creep) at relatively small differential stresses. The amount of strain accumulation depends on competition between strain hardening and recovery/dynamic recrystallization.
Plastic deformation at high temperatures (dislocation creep) is probably the main deformation process in the deeper parts of the earth’s crust (Yund and Tullis 1991). The resulting grains may show undulose (undulatory) extinction and sub-grains, sutured grain boundaries, and a pronounced shape and/or crystallographic preferred orientation. At very high temperatures, ductile grain-boundary sliding may occur. However, water-assisted cataclastic deformation may be responsible for some sub-grains and recrystallized grains in quartz that are optically identical to those commonly inferred to be due to dislocation creep (den Brok 1998).
Undulose Extinction and Sub-Grains
Undulose extinction is a smooth variation in the extinction position of a single grain when examined in cross-polarized light (Wojtal, Blenkinsop, and Tikoff 2022) (fig. 16). It is a very common feature of deformed rocks, especially in quartz and feldspars. The variation in extinction position indicates a variation in the orientation of the crystal lattice of the grain, affecting the polarizing direction of transmitted light and thus the extinction position of different parts of the grain. In moderately deformed grains, these undulose variations in the extinction position and thus lattice orientation are commonly localized into sub-grains, which are intracrystalline domains where the lattice orientation may vary by up to 10° from the rest of the grain (White 1977). This upper limit to the lattice misorientation for sub-grains distinguishes a sub-grain that forms within grains from two separate grains.
Sub-grains may have relatively planar walls in crystallographically controlled directions (fig. 16). In quartz, the basal (perpendicular to the sides of the hexagonal shape seen in large quartz crystals) and prism (parallel to the sides of the hexagonal crystal shape) planes are common sub-grain boundaries. If both directions have developed, the resulting effect is a pattern of square or rectangular domains of contrasting extinction, which is called a chessboard pattern of sub-grains (Wojtal, Blenkinsop, and Tikoff 2022). Some sub-grains have distinctly tabular shapes that define deformation bands (fig. 16). If the sub-grain boundaries are sharply defined and straight, they can be referred to as kink bands. Deformation lamellae are also tabular features but restricted to very small widths.
Diffusion creep (diffusive mass transfer) involves change of grain shape by diffusion of chemical components, either in aqueous solution (stress-induced solution transfer or dissolution-precipitation creep) or by solid-state diffusion along grain boundaries (grain-boundary diffusion or Coble creep) or through crystals (volume diffusion or Nabarro-Herring creep), which requires high temperatures (Fossen 2016; Vernon 2018; Wojtal, Blenkinsop, and Tikoff 2022) (fig. 18). In both cases vacancies in the atomic lattice of the minerals move toward high-stress sites so that the minerals accumulate strain over time. Stress-induced solution transfer (also called pressure solution) is equivalent to Coble creep in dry rocks (Wheeler 1992). Typically, material is removed from sites of high normal compressive stress and deposited at low-stress sites, with the result that a volume of rock changes its shape (Rutter 1976).
The term “pressure solution” strictly refers to the actual dissolving of minerals, and so the term “solution-transfer” has been proposed for the overall process of solution, transfer, and redeposition of chemical components (Durney 1972). A preferable term is “stress-induced solution transfer” (Passchier and Trouw 1996), which emphasizes the necessity of deformation in the process. The term “dissolution-precipitation creep” or simply “solution-precipitation creep” (den Brok and Spiers 1991) also implies a deformation-controlled process.
Stress-induced solution transfer (dissolution-precipitation creep) is especially effective at low metamorphic grades and produces microstructures such as truncated detrital grains, truncated ooliths, truncated fossils, truncated pebbles, stylolitic surfaces, tectonic overgrowths, and “beard” structures (Cox and Etheridge 1982; McClay 1977; Powell 1982 [fig. 16]). However, the process can also occur in:
(1) The deformation of high-and medium-grade metamorphic rocks, producing veins and beard structures (Wintsch and Yi 2002);
(2) During fluid-assisted “superplastic” deformation (ductile grain-boundary sliding); and
(3) Especially in ductile shear zones.
McClay (1977) estimated that stress-induced solution transfer in fine-grained quartz and calcite rocks can produce geologically reasonable strain rates at 200–300°C and that Coble creep in calcite rocks can produce geologically reasonable strain rates at around 300°C.
Microstructures generally taken to indicate diffusion creep in deformed rocks include equant grain shapes, indented grains, overgrowths, and a lack of crystallographic preferred orientation (Bons and den Brok 2000) (fig. 16). However, crystallographic preferred orientations resulting from crystallographic orientation-dependent dissolution and growth have been described for naturally deformed quartz-rich rocks (Becker 1995), and for experimentally deformed quartz rocks (den Brok 1996). Additionally, modeling by Bons and den Brok (2000) has indicated that dissolution-precipitation creep may be important in the development of crystallographic preferred orientations in rocks, and thus, the presence of a crystallographic preferred orientation alone cannot be used as evidence for dislocation creep.
Diffusion creep can grade into ductile grain-boundary sliding and frictional grain-boundary sliding (during brittle deformation) (Vernon 2018). An example is provided by deformation experiments on fine-grained (2–10 µm) albite (plagioclase) with a small amount of water (<1%) in which the deformation changed directly from cataclastic flow to grain-boundary diffusion creep with increasing temperature and decreasing strain rate, without any intermediate dislocation creep (Tullis and Yund 1987, 1991). The resulting microstructures include rectangular grain shapes, overgrowths of different composition from the original grains, and low concentrations of dislocations (Tullis and Yund 1991).
Den Brok (1998) has shown that rates of stress-induced solution transfer depend on microcracking, which may increase greatly with sudden increase in stress or fluid pressure. This can enhance grain-boundary diffusion rates and cause rock weakening. Stress-induced solution transfer tends to predominate at lower temperatures, at which diffusion occurs more readily than dislocation creep. But dislocation creep tends to swamp stress-induced solution transfer at higher temperatures (Wheeler 1992). However, because diffusion occurs along grain boundaries, stress-induced solution transfer is accentuated by finer grain sizes and so can dominate dislocation creep, even at the higher temperatures of the lower crust, at which dislocation creep would otherwise predominate. Calculations made by Wheeler (1992) also suggest that stress-induced solution transfer is more effective in polymineralic rocks than in single-mineral aggregates, owing to chemical interactions during the deformation.
Ductile Grain-Boundary Sliding
Grain-boundary or frictional sliding and fracturing during granular flow are characteristic features of brittle deformation (Fossen 2016) (fig. 15). A distinction is drawn between intergranular fracturing, intragranular fracturing, frictional sliding on fractures and grain boundaries, and grain rotation, which in combination are due to cataclastic flow (figs. 15 and 16). In contrast, granular flow, which also is characterized by grain rotation (or rolling) and frictional grain-boundary sliding, is only intergranular deformation in that there is no permanent internal deformation of the grains. It occurs at very shallow depths on porous sediments such as weakly consolidated sandstone buried at less than ~1,000 m (~3,300 ft) depth. It involves deformation in a shearing mode or in response to vertical loading (compaction). In these processes, if the stresses across grain contacts become high enough then the sedimentary rock’s grains may fracture. Those fractures are confined to individual grains and are therefore intragranular microfractures. Under low pressure conditions and with small grain contact areas microfractures may form close to the grain surfaces, commonly chipping small flakes off of the surfaces of the grains (fig. 19). This microfracturing is referred to as spalling or flaking. At higher confining pressures, corresponding to depths in excess of ~1,000 m (~3,300 ft), fractures can split the grains into more evenly sized parts, and the mechanism is known as transgranular fracturing. Once fractured, the grains reorganize themselves by frictional sliding and rotation, leading to porosity reduction.
However, grain-boundary sliding also occurs during ductile deformation (Wojtal, Blenkinsop, and Tikoff 2022). Some very fine-grained polyphase metal alloys, at certain conditions of temperature (at least half the melting temperature) and strain rate, can be deformed experimentally in tension up to strains of more than 1,000% without fracturing (Vernon 2018). This is referred to as superplastic deformation (grain size-sensitive flow). The mechanism involved is grain-boundary sliding, which involves relative grain movement without loss of cohesion and normally in the absence of fluid. Resulting potential gaps between grains are filled by diffusive mass transfer (Ashby and Verall 1973; Edington, Melton, and Cutler 1976; Nicolas and Poirier 1976; Poirier 1985; Schmid, Boland, and Paterson 1977), dislocation motion (Tullis 1983), or both these processes (Kenkmann and Dresen 2002), and so the aggregate remains coherent.
Superplasticity is a state in which solid crystalline material is deformed well beyond its usual breaking point, usually over about 600% during tensile deformation, which is usually achieved at high temperature. The mechanisms of superplasticity are still debated, but the consensus is that it relies on atomic diffusion and the sliding of grains past each other (grain-boundary sliding). Superplasticity has been proposed for quartz (Behrmann 1985; Behrmann and Mainprice 1987; Boullier and Guegen 1975), calcite (Behrmann 1983), and feldspar (Allison, Barnett, and Kerrich 1979). Some have suggested that normal crystal plasticity can change rapidly to superplasticity below a critical grain size (Behrmann 1983; Schmid, Boland, and Paterson 1977), possibly in millimeter-scale domains (Behrmann and Mainprice 1987).
The problem is to determine the extent to which superplasticity occurs in natural rock deformation (Gilotti and Hull 1990). The following microstructural features have been suggested as indicators of superplastic behavior in rocks (Boullier and Guegen 1975; Schmid 1982):
(1) Grains remaining equant, even after large accumulate strains;
(2) Very small grain size around 1–10 µm; and
(3) Moderate concentrations of dislocations without dislocation cells (that is, no sub-grains).
However, small grain sizes and equant grains are also compatible with dynamic recrystallization during dislocation-induced flow (Schmid 1982; White 1977) so that superplasticity generally cannot be inferred with confidence from microstructure alone. Another characteristic feature of superplasticity may be the absence of strong preferred orientation, since diffusion-accommodated grain-boundary sliding tends to weaken existing preferred orientations, in contrast to aggregates recrystallized dynamically, which typically have crystallographic preferred orientations. However, the lack of strong preferred orientation cannot be always taken to imply superplasticity, because static recrystallization may or may not reduce the strength of preferred orientations produced during dynamic recrystallization (Law 1990). Thus, more general terms such as “non-cataclastic grain size-sensitive flow” or “non-cataclastic granular flow” would better describe natural deformation.
In some rocks, non-cataclastic grain size-sensitive flow may be promoted by the formation of transient, fine-grained reaction products in metamorphic reactions, or by fluid, which assists diffusion and results in a kind of high-temperature pressure solution (Mukai et al. 2014; Tullis and Yund 1991; Tullis, Yund, and Farver 1996). This can be called fluid-assisted diffusion creep. Experiments on deforming fine-grained feldspar aggregates have shown that fluid occurring in pores at hydrostatic conditions spreads along grain boundaries during deformation, causing a change from dislocation creep to diffusion creep with consequent reduction in strength (Tullis, Yund, and Farver 1996). Because minerals continuously dissolve in and precipitate from the fluid as deformation proceeds, microstructural evidence of fluid-assisted diffusion creep may be difficult or impossible to distinguish from other forms of grain-sensitive flow. However, rectangular grain shapes and compositionally different grain overgrowths have been observed in high-temperature diffusion creep experiments on fine-grained sodic plagioclase (Tullis and Yund 1991). Fluid-assisted ductile grain-boundary sliding should be conceptually distinguished from frictional grain-boundary sliding, which involves not only intergranular fluid but also rotation of discrete fragments, rather than maintaining a coherent aggregate during deformation.
Conditions Favoring Various Deformation Mechanisms
Different deformation mechanisms dominate at different conditions of temperature, pressure, strain rate, differential stress, grain size, fluid content, and fluid composition, though several deformation mechanisms may operate simultaneously, even if one dominates (Vernon 2018) (fig. 16). For example, higher confining pressure and lower fluid pressure tend to promote dislocation creep over cataclastic behavior, and larger grain sizes tend to favor dislocation creep and deformation twinning, owing to greater ease of accommodation of strain produced by these processes at grain boundaries, compared with the situation in finer-grained aggregates.
The different deformation mechanisms that are operative in a deforming mineral under various physical conditions can be expressed by means of a deformation mechanism map of stress versus temperature contoured for a range of strain rates (Rutter 1976) (fig. 20). Deformation mechanism maps show the range for which a particular deformation mechanism dominates. They are partly based on experimental data that have been extrapolated into geologically realistic strain rates and temperatures, and partly on theoretical considerations (Fossen 2016). The example in fig. 20 is for quartz. Realistic natural strain rates are indicated in yellow. It should be noted that such maps are hampered by many uncertainties and limited data availability.
Experiments have shown that the main factors favoring ductile flow of solid dry rocks are (Vernon 2018):
(1) High confining pressure, which makes it difficult for the rock to expand and hence break during deformation;
(2) High temperature, which allows dislocations to move freely through minerals; and
(3) Slow application of the deforming force, which gives the dislocations enough time to move.
Therefore, in dry rocks, flow tends to dominate in the deeper parts of the earth’s crust, where rocks are hot and under high-confining pressures. Generally, fractures dominate at depths of less than ~15 km (~9 mi) and flow dominates at greater depths, though many exceptions occur, and the conditions vary with the minerals concerned. For example, quartz tends to be ductile at lower temperatures than feldspars.
Microstructural evidence of dynamic recrystallization is generally taken to indicate relatively high temperature, but the temperature varies greatly with the mineral. For example, though calcite typically undergoes ductile deformation and dynamic recrystallization at greenschist facies or higher temperatures (Busch and van der Pluijm 1995; Rutter 1976; Vernon 1981), these processes can also occur in calcite in temperatures as low as 150–250°C (Kennedy and White 2001).
Fluids are also important. For example, small amounts of water in the crystal structure increase the ductility of quartz. However, water films on grain boundaries may block atomic bonding between grains and so reduce the “effective pressure,” leading to fracturing and brittle deformation. Nevertheless, water may assist diffusive flow in fine-grained calcite aggregates deformed at low differential stress (Rutter 1974) and greatly assists grain-boundary migration crystallization (Mancktelow and Pennacchioni 2004).
The overall situation, summarized by Wintsch and Yi (2002), is that at geological strain rates in quartz-rich rocks, brittle deformation dominated by fracture mechanisms changes to deformation by dislocation creep at ~200°C. In plagioclase, this brittle-to-ductile transition occurs at ~450°C. If water is present, a field of stress-induced solution transfer displaces dislocation creep by 200–300°C. Wintsch and Yi (2002) inferred that, though biotite and quartz deformed by dislocation creep, most of the deformation was accommodated by deformation-enhanced dissolution of minerals at grain boundaries perpendicular to the shortening direction (evidenced by truncated zoning patterns in plagioclase and orthoclase) and precipitation in the form of beards (or fringes in fig. 16) on the ends of grains that face the extension direction. Thus, solution-precipitation creep can accompany and even dominate over dislocation creep at high temperatures in the presence of water. However, quartz microstructure and crystallographic preferred orientation are also sensitive to other variables, such as strain rate and water weakening, as pointed out by Law (2014).
Recovery and Recrystallization
During deformation, dislocations in different slip planes can interfere with each other and form “tangles,” which inhibit their movement and hence further deformation of the mineral (strain strengthening or strain hardening). Recovery and recrystallization are processes that tend to reduce the concentration and/or tangling of dislocations, and so produce volumes of material capable of continued deformation (Vernon 2018; Wojtal, Blenkinsop, and Tikoff 2022). Thus, ductile deformation is a competition between strain strengthening (hardening) and recovery processes.
Recovery includes all processes that attempt to return a crystal to the undeformed state without the formation of high-angle (high-energy) boundaries (Hobbs, Means, and Williams 1976). In other words, no new grains are formed. Recovery may be dynamic or static, depending on whether or not it occurs during or after deformation, respectively.
During recovery, dislocations are able to free themselves from tangles by dislocation “climb” (the movement of edge dislocations out of their slip planes by the addition or loss of point defects, which is a heat-activated process), and by dislocation “cross-slip” (the movement of screw dislocations from one slip plane to another) (Vernon 2018). Both these processes untangle dislocations and so reduce the amount of strain strengthening. The freed dislocations migrate to form sub-grain boundaries, which become “walls” of organized dislocations (Hobbs, Means, and Williams 1976; Spry 1969). This leaves relatively strain-free volumes (sub-grains) between the sub-grain boundaries so that further deformation can proceed.
Optically, sub-grain boundaries tend to be relatively evenly spaced and show small misorientation angles (Vernon 2018). Bending of grains, presumably involving dispersed dislocations, produces undulose (undulatory) extinction, which grades into slightly misoriented sub-grain boundaries. A maximum misorientation of 10° is often taken as a rough guide for sub-grains in quartz (White 1977). Larger misorientations produce grain boundaries. Precise distinction between sub-grain and grain boundaries on the basis of dislocation arrangements requires transmission and scanning electron microscopy (TEM and SEM).
However, slightly misaligned fragments that optically resemble sub-grains can be formed by microfracturing (Lloyd and Freeman 1994; Urai, Means, and Lister 1986). Yet normally such microfractures are formed in the presence of fluid, and thus sub-grains of this type potentially may be recognized by the presence of healed lines of fluid inclusions along the sub-grain boundaries, provided it can be ascertained that the inclusions were not formed along microfractures that developed along existing sub-grain boundaries.
The optical relief of sub-grain (low-angle) boundaries generally is not as marked as with grain (high-angle) boundaries, and together with the small misorientations, makes it clear that the sub-grains occur within grains (hence the name). Sub-grains may be equant or elongate. Elongate sub-grains form perpendicular to slip planes and appear optically as “extinction bands” at high angles to the slip planes. Sub-grains have been observed in a variety of minerals, including quartz (Hobbs, Means, and Williams 1976), calcite (Vernon 1981) and plagioclase (Fitz Gerald, Etheridge, and Vernon 1983; Vernon 1975).
Recrystallization involves the formation of strain-free volumes inside deformed grains by the creation and/or movement of grain boundaries in response to deformation (Vernon 2018; Wojtal, Blenkinsop, and Tikoff 2022). During recrystallization, strain energy is reduced by:
(1) Migration of existing high-angle (high-energy, random, irrational) grain boundaries, kink-band boundaries, or twin boundaries;
(2) Development and migration of new high-angle grain boundaries (excluding kink-band boundaries and fractures); and
(3) Development of new low-energy crystal faces, all in the same mineral.
A generally applicable definition of recrystallization is the development and/or migration of high-angle (random) grain boundaries or crystal faces in solid state in response to deformation and in the same mineral.
Recrystallization typically produces aggregates of new (recrystallized) grains that are strain free and therefore capable of continued deformation (Vernon 2018). The new grains may be:
(1) Polygonal in minerals with relatively uniform three-dimensional lattice structures, such as quartz, feldspar, and calcite (fig. 16);
(2) Crystals with low-energy faces in minerals with strongly anisotropic lattice structures, such as mica (Bell 1978; Etheridge and Hobbs 1974; Vernon 1977b); or
(3) Irregularly shaped where grain-boundary migration recrystallization is the dominant process.
However, recrystallization does not involve the production of new minerals, although small compositional changes between new and old grains commonly occur in minerals with complex compositions (for example, Etheridge and Hobbs 1974; Vernon 1975, 1977a). Stünitz (1998) has shown that differences in composition between old and recrystallized plagioclase grains can contribute to the driving force for recrystallization.
Nucleation of new grains during recrystallization generally does not involve the formation of completely new grains from new nuclei developed randomly within old grains but typically involves either sub-grain rotation or strain-induced grain-boundary migration (“bulge nucleation”). However, both processes can produce similar microstructures (Lloyd and Freeman 1994), and microfracturing can produce slightly misaligned fragments that optically resemble sub-grains (den Brok and Spiers 1991; Lloyd and Freeman 1994; Urai, Means, and Lister 1986). The following three processes are involved in recrystallization.
Sub-grain rotational recrystallization (Hobbs 1968; Poirier and Guillopé 1979) occurs when dislocations accumulate in sub-grain boundaries, causing the boundaries to progressively increase their complexity and misorientation. When a dislocation is added to a sub-grain boundary it changes the angle mismatch between the two sub-grains. By this process sub-grain boundaries become grain (high-energy, high-angle) boundaries. It involves progressive crystallographic misorientation with limited grain-boundary migration, so that orientation relationships between the old and new (recrystallized) grains may be recognized (Hobbs 1968; Vernon 1975). Sub-grains leading to recrystallization have been observed in quartz (Hobbs 1968; Tullis, Christie, and Griggs 1973), calcite (Vernon 1981), K-feldspar (Altenberger and Wilhelm 2000; Bell and Johnson 1989), and plagioclase (Bell and Johnson 1989; Dornbusch, Weber, and Skrotzki 1994; Vernon 1975). Photographic evidence under the microscope of progressive rotation of sub-grains to produce new (recrystallized) grains during deformation of transparent minerals has been presented by Means and Xia (1981) and Means (1989).
Recrystallization by strain-induced grain-boundary migration involves differential migration of parts of a high-angle boundary, such as a grain boundary, kink-band/deformation-band boundary, or a deformation-twin boundary (Vernon 2018). The migration occurs by diffusion of atoms across the boundary, which consequently moves in the opposite direction to the diffusion direction and forms a “bulge.” Strain-induced grain-boundary migration is driven by strain energy differences (differences in the dislocation concentration) on either side of the grain, kink-band, or twin boundary. The process tends to relax gradients in strain (recrystallization) and/or composition. So, as the boundary moves into a deformed grain it leaves undeformed mineral behind it. The microstructural result is a sutured (bulged) grain boundary, kink-band boundary, or deformation-twin boundary, with markedly smaller new grains along the boundary (fig. 16). The process occurs at low temperatures in quartz and calcite (Drury, Humphreys, and White 1985; Schmid, Panozzo, and Bauer 1987; Schmid, Paterson, and Boland 1980).
Sutured grain boundaries, kink-band boundaries and twin boundaries have been observed in a wide variety of minerals including quartz, plagioclase, and calcite (Vernon 1981), and K-feldspar (Altenberger and Wilhelm 2000) (fig. 16). In minerals with relatively isotropic crystal structures (quartz, feldspar, calcite), strain-induced grain-boundary migration produces equant new grains, whereas in minerals with strongly anisotropic crystal structures (sheet silicates such as micas), it produces aggregates of elongate new grains.
Poirier and Guillopé (1979) have pointed out that trace amounts of water increase the rate of grain-boundary migration, even in anhydrous minerals such as quartz (Green, Griggs, and Christie 1970). They suggested that water may enhance grain-boundary mobility by increasing the glide and/or climb mobility of grain-boundary dislocations, in the same way as it appears to induce easier glide or climb of lattice dislocations (Griggs 1974; McLaren and Retchford 1969).
Though bulges in grain boundaries commonly appear rounded (except for minerals such as sheet silicates), long-lasting strain-induced grain-boundary migration at relatively high temperature can lead to a stepped rather than smooth sutured interface (Kruhl 2001; Kruhl and Peternell 2002). The steps or sharp deflections appear to be due to crystallographic control, such as the formation of rhombohedral planes in quartz (Masberg, Hoffer, and Hoernes 1992).
Grain-boundary migration recrystallization (fast grain-boundary migration) is a more pronounced form of grain-boundary bulging that occurs during recrystallization (Vernon 2018). It has been observed in materials progressively deformed under the microscope (Means 1989; Urai 1983). The process produces bulges with long wavelengths of the order of the grain size, which migrate through the aggregate, continuously converting parts of it from one lattice orientation to another. These changing “orientation domains” move through the aggregate in a complex way, leading to irregular grain shapes, though locally interfaces may have marked steps, suggesting crystallographic control, especially if fluid occurs along the grain boundaries. Though no new grains are produced, some can be removed or dissected, and others can coalesce or amalgamate by progressive reduction of misorientation. The process affects large areas, so that original grains may be completely consumed (Urai, Means, and Lister 1986). Fast grain-boundary migration can change catastrophically to slow grain-boundary migration and vice versa, owing to sudden changes in the grain-boundary structure or the absorption of impurities (Urai 1983).
Grain-boundary migration recrystallization occurs at relatively high temperatures (amphibolite facies) in quartz and calcite (Fitz Gerald and Stünitz 1993; Schmid and Casey 1986; Schmid, Panozzo, and Bauer 1987; Schmid, Paterson, and Boland 1980). However, the process is also promoted by water on the migrating boundaries (Mancktelow and Pennacchioni 2004). This interpretation is supported by experiments in which fluid-assisted grain-boundary migration recrystallization can produce new grains with crystal faces (Urai 1983; Urai, Means, and Lister 1986). In wet samples, a continuous fluid film occurs along the migrating boundary, incorporating fluid inclusions as it moves. The boundary migration occurs by dissolution of the grain with the higher dislocation concentration, diffusion through the fluid film, and precipitation on the other grain.
In principle, recrystallization may occur either during deformation (dynamic recrystallization or syndeformational recrystallization) or after deformation (static recrystallization), which is equivalent to static grain growth (Vernon 2018). Static recrystallization has been inferred to occur if temperatures remain high enough for grain-boundary migration after strain rates decrease (in which case it could modify microstructures formed by dynamic recrystallization).
Dynamic recrystallization of low-melting-temperature minerals has been observed directly in in-situ experiments under the microscope (Vernon 2018). Such studies have enabled detailed observation of grain-boundary movements and changes in grain shapes with progressive deformation and recrystallization. For example, Urai (1983) found that:
(1) Dynamically recrystallized grains do not necessarily have undulose extinction;
(2) Recrystallization may occur by grain and twin-boundary migration (bulge nucleation) and progressive misorientation of sub-grains;
(3) Recrystallization may occur along fractures;
(4) Grain boundaries may progress and regress cyclically;
(5) One grain may be cut up into two grains by grain-boundary movement;
(6) Two grains may coalesce into one;
(7) Incomplete elimination of serrations may lead to the preservation of “leftover grains;”
(8) Bimodal grain-size distributions may form; and
(9) “Orientation families” of grains with similar orientations may develop, owing to different rates of boundary migration in different directions.
White (1977) suggested that dynamically recrystallized grains can be recognized by the presence of sub-grains, deformation bands, and deformation lamellae, in contrast to optically strain-free new grains expected from static recrystallization. Even though Urai (1983) and Urai, Means, and Lister (1986) found that dynamically recrystallized grains do not necessarily have undulose extinction, new (recrystallized) grains with undulose extinction are at least consistent with dynamic recrystallization. In fact, any evidence of deformation in new (recrystallized) grains is diagnostic of dynamic recrystallization, such as optically observable sub-grains. Similarly, orientation families, that is, groups of several apparently independent grains with identical crystallographic orientations, may also be reliable indicators of dynamic recrystallization. Furthermore, while aggregates of relatively coarse-grained, optically strain-free polygonal grains have been interpreted as indicating static recrystallization, strain-free grains may also be produced by dynamic recrystallization in experiments (Urai, Means, and Lister 1986). And one potentially useful microstructural feature is the observation that boundaries of grains developing during strain-induced grain-boundary migration (dynamic recrystallization involving bulge nucleation) grow away from their centers of curvature, whereas the reverse applies to static grain growth.
In both sub-grain rotation and strain-induced grain-boundary migration, the new grains are smaller than the original deformed grains, so that grain size reduction is typical of dynamic recrystallization (Vernon 2018; Wojtal, Blenkinsop, and Tikoff 2022). The new grains tend to be much smaller at lower temperatures (250–300°C for quartz and 400–450°C for feldspar) and/or fast strain rates. Indeed, at relatively low temperatures (200–300°C for quartz and 400–500°C for feldspar) and/or fast strain rates, recrystallization mainly involves grain-boundary migration, which involves bulging of grain boundaries in response to variable dislocation concentrations, forming small strain-free grains. However, grain-boundary migration recrystallization is restricted to the relatively high temperatures of amphibolite facies conditions for quartz and calcite (Fitz Gerald and Stünitz 1993; Schmid and Casey 1986; Schmid, Panozzo, and Bauer 1987; Schmid, Paterson, and Boland 1980) and granulite facies conditions for feldspar (Lafrance, John, and Scoates 1996).
Experimental studies on quartz aggregates have identified three regimes of dislocation creep, defined by different mechanisms of dynamic recrystallization (Hirth and Tullis 1992; Tullis et al. 2000). These regimes operate at different temperature-strain rate conditions and produce different microstructures, which have also been recognized in naturally deformed quartzites. However, they form at much lower temperatures, owing to presumed slower natural strain rates.
Regime 1 occurs at the lowest temperatures of deformation and is characterized by difficult dislocation climb, low grain-boundary mobility, and high dislocation-density contrasts between different grains. Dislocation glide is accommodated by recovery and strain-induced grain-boundary migration (bulging recrystallization) at slow rates, producing very small bulges. The bulging occurs mainly at triple junctions and along fractures if present. Regime 2 is characterized by recrystallization involving progressive sub-grain rotation, and occurs at intermediate temperatures. Regime 3 is characterized by grain-boundary migration recrystallization at fast rates, and occurs at high temperatures. During this recrystallization whole grains may be swept clear of dislocations, and sub-grain rotation is only important for the initial formation of new grains.
Deformation of Polymineral Aggregates
Ductile behavior of minerals and rocks is generally defined as the capacity to deform without fracturing on the grain scale (Passchier and Trouw 1996; Vernon 2018). However, ductility has also been defined as “the capacity for substantial change of shape without gross fracturing” (Paterson 1978). The latter definition refers to megascopic or macroscopic flow and is independent of the microscopic mechanisms of deformation, which can include not only crystal plasticity and diffusional flow (which maintain cohesion at the microscopic scale) but also cataclastic (microscopically brittle) mechanisms. In other words, based on that definition, a rock can be ductile on the scale of a hand specimen or outcrop but partly brittle on the microscopic scale.
A major factor governing ductility is the number of slip systems available for deformation to occur without producing holes or cracks (Murrell 1990). Five independent slip systems are necessary for plastic deformation without fracturing at grain boundaries (Groves and Kelly 1963). However, many minerals have strongly anisotropic structures (for example, micas) and so have fewer slip systems than those with more three-dimensional structures (for example, quartz). The result is that some minerals can change their shapes in response to general local stress fields more readily than others. This can lead to localization of deformation into high-strain zones or to the opening of pores or local cracks, which are important in localizing fluids.
Natural rocks typically have several minerals with different deformation properties that can vary with external conditions (for example, temperature, pressure, water activity) (Vernon 2018). This situation produces deformation contrasts between different minerals, which occur when stronger and weaker minerals coexist. For example, strong feldspar and weak quartz typically coexist, deforming at relatively low temperature (<500°C). The feldspar deforms plastically a little before it fractures (brittle deformation), whereas the quartz flows and recrystallizes in a ductile manner, commonly forming “ribbons” of fine-grained recrystallized aggregates. Those ribbons originate as kink bands or deformation bands that recrystallize with progressive deformation.
Evidence of both ductile and brittle behavior is seen in many felsic mylonites in which feldspar deforms cataclastically, whereas quartz and mica deform mainly by dislocation creep, commonly assisted by neocrystallization (Vernon, Williams, and D’Arcy 1983). On the other hand, sometimes biotite deforms by fracturing along the cleavage, forming “shreds” or cleavage platelets that become stretched out along a developing foliation (Johnson, Vernon, and Upton 2004; Vernon, Johnson, and Melis 2004), as indicated by some experimental results (Shea and Kronenberg 1993).
Though fluid-enhanced microcracking is commonly an important deformation mechanism in such rocks, both brittle and ductile processes alternate, and cohesion is maintained during deformation (Gapais 1989; Stel 1986). This has been referred to as “semi-brittle” behavior. In some rocks, hydrous minerals that grow from fluids that enter the rock during brittle deformation undergo ductile deformation (Simpson 1986), which may be followed by more fracturing and mineral growth in a cyclic process (Stel 1986).
The effect of ductility contrasts in rocks can be so great that deformation is forced to partition preferentially into zones rich in weak minerals, such as mica (Goodwin and Tikoff 2002; Shea and Kronenberg 1993) and/or fine-grained aggregates (Stünitz and Fitz Gerald 1993), promoting the formation of local zones of high strain (shear zones).
As already noted, contrasts in the deformation of quartz and feldspar are strongly temperature dependent. Similarly, strain rate is important when considering deformation contrasts between minerals. Furthermore, large grains generally deform more readily by dislocation flow than smaller grains of the same mineral, probably because intracrystalline slip can occur with less interference from adjacent grains (Rutter 1976). However, in many rocks, large grains are stronger than surrounding finer-grained aggregates of weaker minerals such as quartz and mica. This is because intergranular deformation is important in fine-grained aggregates (for example, by grain-boundary sliding, reaction-assisted diffusion), leading to increased strain rates (Etheridge and Vernon 1981; Stünitz and Fitz Gerald 1993). However, as pointed out by de Bresser, ter Heege, and Spiers (2001), dynamic recrystallization can lead to major zones of weakening and strain localization only if grain growth is inhibited.
In summary, the focus needs to be on what microstructures might apply to the Tapeats Sandstone within the Carbon Canyon fold that should be observed at the microscopic scale. Ductile deformation features especially in quartz grains that should be evident if the sandstone was lithified before the folding occurred would include undulose extinction, kink bands, deformation bands, deformation lamellae, deformation twins, pressure effects at the contacts between grain boundaries, sub-grains, sutured grain boundaries, grain boundary bulges, intragranular fractures, intergranular fractures, crystallographic preferred orientations, any rotated grains or sub-grains, any grain size reduction, and/or recrystallized grains.
A Petrographic Study
So, was the folding of the Tapeats Sandstone within the Carbon Canyon fold due to slow processes of ductile deformation over millions of years that occurred hundreds of millions of years after the sandstone lithified, or was the folding due to soft-sediment deformation soon after deposition before dewatering and lithification? It should be very evident that to resolve this debate requires a petrographic examination of sandstone samples from the fold to determine what microstructural features are present. The proposed ductile deformation should have resulted in definitive microstructural features which should be visible in the sandstone’s grains and cement under the microscope, as described in detail above. On the other hand, the absence of such microstructural features and instead the presence of preserved primary depositional features would indicate soft-sediment deformation had occurred, particularly if those preserved primary depositional features in sandstone samples from the fold are identical to those in samples from the same sandstone beds distant from the fold.
No such petrographic study has previously been undertaken. So, during an investigation of four folds in the Grand Canyon, 12 samples of the Tapeats Sandstone were collected from the Carbon Canyon fold, and four samples from outcrops along the Colorado River corridor distant from those folds (fig. 1 and table 1). The purpose was to compare under the microscope the samples from the fold (fig. 21) with the distal samples (fig. 1) to ascertain what effects the folding had on the sandstone and thus determine the conditions during, and the timing of, the folding relative to the conditions and timing of the deposition and subsequent lithification (cementation) of the sandstone. Details of the locations of those samples are provided in figs. 1 and 21, and in table 1, as well as in the appendix (in the Supplemental material). Within the Carbon Canyon fold two Tapeats Sandstone beds were chosen to be sampled laterally from the limbs through the hinges of the fold, and those sampling locations can be seen on figs. 21. All samples were sent to Calgary Rock and Materials Services, Inc. (Calgary, Canada) for thin sectioning and for x-ray diffraction (XRD) analyses and scanning electron microscope (SEM) examination.
|Location||Location Coordinates||Stratigraphic Position||Notes|
|TSS-01||River Mile 60.1||N 36° 12.784’ W 111° 48.411’||12 m below top of cliff-forming unit||Just below Sixtymile Rapid, river left, upstream end of the beach|
|TSS-02||River Mile 120.8||N 36° 14.419’ W 112° 28.825’||Halfway down the cliff-forming unit||Just beyond Blacktail Canyon, river left|
|TSS-03||River Mile 138||N 36° 23.859’ W 112° 31.896’||Close to Great Unconformity||Opposite just below Doris Rapid, river right|
|TSS-04||River Mile 138||N 36° 23.859’ W 112° 31.896’||7.5 m stratigraphically higher than TSS-03||Opposite just below Doris Rapid, river right|
|CCF-01||Carbon Canyon fold River Mile 65||N 36° 09.268’ W 111° 49.806’||10–12 m below top of cliff-forming unit||1.4 m above the hinge of the fold|
|CCF-02||Carbon Canyon fold River Mile 65||N 36° 09.268’ W111° 49.806’||10–12 m below top of cliff-forming unit||Same bed, from the hinge of the fold|
|CCF-03||Carbon Canyon fold River Mile 65||N 36° 09.263’ W 111° 49.797’||10–12 m below top of cliff-forming unit||Same bed, 2.3 m from sample CCF-02|
|CCF-04||Carbon Canyon fold River Mile 65||N 36° 09.264’ W111° 49.794’||10–12 m below top of cliff-forming unit||Same bed, 3.5 m from sample CCF-03|
|CCF-05||Carbon Canyon fold River Mile 65||N 36° 09.258’ W 111° 49.789’||10–12 m below top of cliff-forming unit||Same bed, 8 m from sample CCF-04|
|CCF-06||Carbon Canyon fold River Mile 65||N 36° 09.256’ W 111° 49.784’||10–12 m below top of cliff-forming unit||Same bed, 5 m from sample CCF-05|
|CCF-07||Carbon Canyon fold River Mile 65||N 36° 09.260’ W 111° 49.782’||10–12 m below top of cliff-forming unit||Same bed, 4 m from sample CCF-06|
|CCF-08||Carbon Canyon fold River Mile 65||N 36° 09.264’ W 111° 49.780’||10–12 m below top of cliff-forming unit||Same bed, 6 m from sample CCF-07|
|CCF-09||Carbon Canyon fold River Mile 65||N 36° 09.279’ W 111° 49.800’||14–16 m below top of cliff-forming unit||Another bed, ~4 m stratigraphically lower, 1.5 m above hinge of the fold|
|CCF-10||Carbon Canyon fold River Mile 65||N 36° 09.261’ W 111° 49.797’||14–16 m below top of cliff-forming unit||Same second bed, from the hinge of the fold|
|CCF-11||Carbon Canyon fold River Mile 65||N 36° 09.258’ W 111° 49.794’||14–16 m below top of cliff-forming unit||Same second bed, 2.3 m from sample CCF-10|
|CCF-12||Carbon Canyon fold River Mile 65||N 36° 09.258’ W 111° 49.792’||10–12 m below top of cliff-forming unit||Around the corner about 40 m from sample CCF-11|
Thin Section Examination
The thin sections for this study were all mounted on standard glass microscope slides. Rock slices were cut perpendicular to the bedding so that the laminations could be viewed in cross-section. Any disruptions of the laminations due to ductile deformation would thus be evident without diminishing the ability to observe any dislocations of grains that might or might not have occurred. However, before the slices were cut from the rock samples using a diamond saw, the rock samples were impregnated under confining pressure with epoxy resin that contained a blue dye. This ensured that grains did not get dislocated, or the rock fabrics get distorted during the sawing of the slices. However, this process left the thin sections with a blue dye staining as the surrounding background and in any holes or pores within the rock fabrics. Before cover slips were added, the thin sections were stained so as to make the K-feldspar and calcite in the rock fabrics more easily distinguished. Thus, the K-feldspar grains have a distinctive yellow color, and the calcite is pinkish in plane polarized light.
Petrographic descriptions of all samples from extensive thin section examination are provided in the appendix (in the Supplementary material), along with photomicrographs of the whole thin sections from which the descriptions were derived. The locations and stratigraphic details of all samples are provided in table 1, as well as in the appendix. All samples were collected from the major cliff-forming unit (Facies B) of the Tapeats Sandstone. The results of the XRD analyses which provided a quantitative estimate of the mineral constituents of each sandstone sample are compiled in table 2. These estimated mineral constituents could then be verified under the petrographic microscope.
|Sample||Stratigraphic Position||Quartz||K-Feldspar||Plagioclase||Calcite||Halite||Kaolinite||Total||Porosity (average)|
|TSS-01||12 m below top of cliff-forming unit||68.4%||31.6%||—||—||—||—||100.0%||~6.5%|
|TSS-02||Halfway down the cliff-forming unit||87.7%||6.4%||—||5.9%||—||—||100.0%||~6%|
|TSS-03||Close to Great Unconformity||83.3%||8.6%||—||8.1%||—||—||100.0%||~5.5%|
|TSS-04||7.5 m higher than TSS-04||98.8%||—||—||—||—||1.2%||100.0%||~0.5%|
|CCF-01||10–12 m below top of cliff-forming unit||92.7%||7.3%||—||—||—||—||100.0%||~5%|
|CCF-02||10–12 m below top of cliff-forming unit||67.6%||32.4%||—||—||—||—||100.0%||~5%|
|CCF-03||10–12 m below top of cliff-forming unit||92.0%||6.9%||—||1.1%||—||—||100.0%||~5.5%|
|CCF-04||10–12 m below top of cliff-forming unit||95.6%||4.4%||—||—||—||—||100.0%||~1.5%|
|CCF-05||10–12 m below top of cliff-forming unit||67.4%||29.5%||3.1%||—||—||—||100.0%||~5%|
|CCF-06||10–12 m below top of cliff-forming unit||88.5%||11.5%||—||—||—||—||100.0%||~2%|
|CCF-07||10–12 m below top of cliff-forming unit||90.2%||9.8%||—||—||—||—||100.0%||~3%|
|CCF-08||10–12 m below top of cliff-forming unit||100.0%||—||—||—||—||—||100.0%||~2.5%|
|CCF-09||14–16 m below top of cliff-forming unit||92.1%||7.9%||—||—||—||—||100.0%||~1.5%|
|CCF-10||14–16 m below top of cliff-forming unit||79.3%||19.2%||—||1.5%||—||—||100.0%||~5%|
|CCF-11||14–16 m below top of cliff-forming unit||90.4%||9.6%||—||—||—||—||100.0%||~4%|
|CCF-12||10–12 m below top of cliff-forming unit||89.1%||10.1%||—||—||0.8%||—||100.0%||~2%|
In the thin sections, the sandstone is generally massive and poorly to moderately well-sorted, dominated by sub-angular to sub-rounded quartz grains ranging in size from coarse silt to very coarse sand and sometimes granules (plus occasionally some small pebbles), using the standard definitions and terminologies for sorting of Folk (1966, 1980) and Pettijohn, Potter, and Siever (1973), for shape of Powers (1953) and Folk (1955), and for size of Udden (1914) and Wentworth (1922). Thin sections at normal scale of the complete set of samples are shown in fig. 22, while the photomicrographs in fig. 23 show typical textures within the complete set of 16 samples of this sandstone for this study. It should be noted that in these thin sections there is often a blue dye staining between the grains and sometimes encroaching on the grain edges or even across grain surfaces. This blue dye is associated with the epoxy that the samples were impregnated with prior to the preparation of the thin sections. Thus, some patches of blue dye mark the occasional pore spaces.
Some samples are laminated with thin (1–2 cm) coarse-grained and finer-grained laminae, even with low-angle cross-bedding in some of the laminae (for example, fig. 22a and o). There is no evidence of any significant preferred orientation of the quartz and K-feldspar grains within the laminae. But generally, the quartz grain sizes are randomly mixed and invariably occasional K-feldspar grains of various sizes are scattered through the poorly to moderately well-sorted rock fabric (fig. 23). Indeed, all samples contain numerous K-feldspar grains and at least a few thin edge-on muscovite flakes, while a few samples contain possible plagioclase grains which are evident from their multiple twinning under crossed polars. Generally, there are very few pore spaces remaining, most pores having been filled by quartz (silica) cement, often as a result of the quartz growing as overgrowths around the original detrital grains (sometimes still outlined by the original iron oxide and dust coatings), with the overgrowths meeting at triple points. Occasional former pores have been filled with later secondary iron oxides, and sometimes also with calcite or clay minerals. Minimal diagenetic alteration has occurred and is primarily alteration or dissolution of some K-feldspar grains and laths, the formation of clay minerals, and the sporadic introduction of occasional calcite. In summary, this is a submature arkosic sandstone or sub-arkose that is well-cemented, predominantly by silica (quartz) but with trivial secondary calcite and iron oxides in a few samples (Snelling 2021). This classification is based on the predominance of quartz, and the K-feldspar content which averages much less than 25% (Dott 1964; Folk 1980; McBride 1963; Pettijohn 1954, 1957; Pettijohn, Potter, and Siever 1973; Scholle 1979; Ulmer-Scholle et al. 2015).
Cathodoluminescence (CL) Imaging
Cathodoluminescence (CL) imaging has proven useful in the study of sedimentary rocks (Boggs and Krinsley 2006; Götze and Hanchar 2018). In the Calgary Rock and Materials Services laboratory, the Luminoscope instrument used has a CL stage attached to a standard optical petrological microscope, allowing the CL images to be viewed in color through the objective lens of the microscope, and then photographed. An advantage is that viewing and photographing can be switched between normal optical and CL modes. Polished thick sections of the rock samples without any coating were mounted on the CL stage. The Luminoscope instrument runs with cold cathode electron gun at 18 kV in a vacuum of ~10-2 Torr and deflection magnets to control the electron beam that bombards the sample and produces the luminescence. Both the optical and the resultant CL images are able to be photographed using a standard camera mounted in tandem with the objective lens.
Scanning Electron Microscope (SEM) Examination
The scanning electron microscope (SEM) used in the laboratory at Calgary Rock and Materials Services, Inc. is an Amray 1820i instrument equipped with a 4pi digital control and image acquisition system and is used in its secondary mode. Energy Dispersive Spectrometry (EDS) spectra are acquired using a Gresham Titan near-windowless piezo-cooled detector.
Samples as supplied in vertical orientation were first of all fractured/broken vertically. This ensured that the horizontal bedding is not the major feature of the sample examination process. Samples were glued using five-minute adhesive to 10 mm aluminum stubs, maintaining the vertical fracture orientation. After curing, the samples were gently blown clear of debris using dry air. Following this, the samples were placed in a Polaron sputter coating unit for application of gold coating used to ensure good surface conductivity. This unit is equipped with a piezo-cooled stage to assist in preventing thermal damage to the sample. Additionally, coating was done in a burst mode—one minute on, one minute off, continued for a total coating time of five minutes for each sample.
Following coating, samples were individually and sequentially placed into the Amray 1820i for analysis. Image sequences from low magnification to high magnification were taken and reviewed for significant features. Bulk EDS is normally run on the low magnification scanned surface in order to get a composite elemental analysis. Beam accelerating voltage is normally held at 30 kV in order to provide best resolution and least beam distortion. This also assists in providing the best EDS response over the emission range of interest.
The focus of this study was to investigate the microstructures in the sediment grains and the textures within the rock samples to ascertain whether the original sedimentary rock grains and textures had been changed by the deformation in the fold, particularly the hinge zones, compared to those samples collected from the fold limbs and those distant from the fold. The detailed petrographic descriptions of all 16 samples (four regional samples distant from the fold and 12 samples from the Carbon Canyon fold) are available in the appendix in the Supplementary material.
Grains and Textures
Several observations are very evident, being uniformly and ubiquitously present in all samples, both those collected from the fold hinges and limbs, and those collected from locations distant to the fold.
The outlines of many of the original detrital quartz grains can still be seen as well as the later quartz overgrowths that cement the grains together (fig. 24). Those outlines are usually marked by the original dust and iron oxides coating them. Many of the original detrital quartz grains are sub-rounded or sub-angular. The grains vary in size and are randomly mixed resulting in a poorly to moderately well-sorted texture. While the overburden pressure has obviously compacted the originally deposited sediment grains, their close packing still left many small pore spaces between them, which would initially have been filled with connate water.
The quartz and K-feldspar grains often meet at triple points produced by the quartz (silica) cement growing as overgrowths on the original detrital grains (fig. 25). These quartz overgrowths would have resulted from dewatering of the pore spaces, the dissolved silica in the connate water precipitating to infill most of the pore spaces. Usually, the quartz overgrowths precipitated in optical continuity with the original detrital grains. Often the original detrital grain outlines have been obliterated during this silica cementation process so that the quartz grains have uniform optical appearances with few internal markings and simply interlock tightly with sub-euhedral outlines meeting at triple points. This suggests the silica for the cement was probably derived mostly from the connate water in the original pore spaces dissolving silica in situ from the edges of the detrital grains, particularly at grain-to-grain contacts. When the silica precipitated within the pore spaces it overlaid the grain surfaces and grew inwards to eventually meet at triple points, the most ergonomic configuration.
Also, of significance are the porosity estimates listed for each sandstone sample in table 2 (in the last column). In all samples there are pore spaces left in the rock fabric, yet the blue dye that accompanied the resin used under pressure to impregnate the samples before the thin sections were cut has stained between the grains and encroached on some of them, sometimes covering grains and thus distorting their colors, which can make some look like pore spaces. It should be noted that where the grains have smaller radii than the microscope slide thickness, the tight stacking of the grains may obscure some residual pores. However, the estimated porosities range from ~0.5% to ~6.5% in the distal samples (average ~4.5%) and from ~1.5% to ~5.5% in the samples from the Carbon Canyon fold (average ~3.5%). Furthermore, within the Carbon Canyon fold, samples in the hinge zones have above average porosities (~5.0%–~5.5%) compared to those along the limbs (~1.5%–~5.0%). This is somewhat surprising and counterintuitive, as one might expect the sandstone porosity to be a bit less in the hinge areas because squeezing and shaking during soft-sediment deformation can dewater the sand and thus press the sand grains tighter together. In contrast, from the conventional view that this folding was due to ductile deformation, the porosity should have been reduced in the hinge areas due to the higher compactional forces, pressure solution, and grain fracturing to fill the pore spaces there.
Only a few quartz grains in every sample contain sub-grains, regardless of whether the sample is from the limbs or hinges of the fold or from a distant location (fig. 26). In most instances the sub-grains in these quartz grains appear to have been features in the original clasts, because the outlines of these quartz grains preserve their detrital shapes. This likely indicates they were eroded and transported from metamorphic rocks. There are no uniform sizes or shapes of these sub-grains. Most are irregularly shaped, and often they are of vastly different sizes within the same quartz grain. However, in some quartz grains the sub-grains are more uniform in size and smoother in shape. Also, the sharpness of the sub-grain boundaries varies between quartz grains. Overall, though, sub-grains within the few quartz grains in which they occur are trivial features, which suggest they are not related to the deformation, especially since they occur in all samples, whether in the fold or distant from it.
The quartz grains generally do not show signs of any undulose extinction under crossed polars, nor are any deformation lamellae or deformation kink bands present (fig. 27). Almost all the quartz grains display uniform extinction under crossed polars. Where there is an appearance of slightly undulose extinction, it could be an artifact in the original quartz grains of the source rocks, probably mostly the metamorphic schists below the Great Unconformity, that was retained unchanged in those deposited clasts. On the other hand, there is no indication or even any hint of any deformation lamellae or deformation kink bands in any of the quartz grains in these samples, including the samples from the hinge zones of the fold.
Fractures within quartz grains are observed more readily in some samples than others (fig. 28). In most instances the fractures are subtle, whereas in rare quartz grains they are more pronounced (for example, fig. 28b, e, and q). Yet in those rare cases the pronounced fractures are in quartz grains primarily from samples distant to the fold, which is intuitively unexpected. This perhaps suggests that those pronounced fractures may be an artifact of the sample collection procedure and/or the preparation of the thin sections, or are most likely due to continued compactional overburden loading subsequent to deposition. On the other hand, the lack of pronounced or prominent fractures within quartz grains in samples from both the hinge and limb zones of the fold might reflect the prevalent conditions during deformation of the sandstone beds in the fold.
In some samples there are occasional broken quartz grains (fig. 29). In most instances the breakage is not pronounced, nor the displacement of the pieces. Once again, these occurrences are just as prevalent in samples distal to the fold as in samples from the fold. This may again suggest these occurrences are an artifact of the sample collection procedure and/or the preparation of the thin sections. However, in three samples, distal sample TSS-04 (fig. 29e and f), fold hinge sample CCF-10 (fig. 29q), and limb sample CCF-11 (fig. 29s) the presence of detrital muscovite flakes bent around some of the broken quartz grain fragments suggests that the latter may be a primary depositional feature due to breakage during deposition, rather than being due to the deformation of the sandstone beds in the fold.
The original detrital K-feldspar grains are still preserved in all samples (fig. 30). They are preserved as often altered fragments and sub-euhedral to sub-rounded grains and former laths of various sizes from very small to large, scattered randomly between the many quartz grains in all samples. The grains are sometimes fractured, usually along cleavage planes. However, there is no evidence of any modifications due to any metamorphism to the detrital appearance of these K-feldspar grains after their deposition, or especially due to the subsequent deformation of the sandstone beds in the fold. Indeed, the detrital K-feldspar grains appear the same and are similarly altered in both the distal samples and those from the hinges and limbs of the fold.
The original detrital muscovite flakes are likewise still preserved in all samples without any evidence of modification due to any metamorphism (fig. 31). They are observed in the thin sections as edge-on flakes, that is, cross-sections through the stacked sheets (“books”), sometimes being altered and thus the “books” have expanded in thickness (for example, fig. 31c, h, and l). Since the thin-sections were cut perpendicular to the bedding, this observation indicates that the muscovite flakes are aligned parallel and sub-parallel to the bedding. This is consistent with these muscovite flakes still being the original detrital grains, as due to their flatness, deposition by cushioning in the water column would be expected to lay them on the accumulating sediment surfaces parallel and sub-parallel to the bedding. Further evidence that these muscovite flakes are still preserved in their detrital condition is the observation that many of the edge-on flakes in the thin-sections are wedged between and often bent around the quartz and K-feldspar grains (fig. 31). And sometimes the flakes are broken and/or their ends are frayed and split apart (fig. 31a, h, o, p, x, b’). Much of the bending and breaking of flakes may, of course, have been due to compaction of the sand subsequent to deposition. Furthermore, the bending and breaking of flakes does not appear to have been caused by the deformation of the sandstone beds in the fold, because bent and broken flakes are found as often in the distal samples as in the samples from the fold. Nor are bent and broken flakes more prevalent in the hinge zones compared to in the limbs of the fold. And finally, the relatively unaltered state of many of the muscovite flakes in both distal and fold samples is consistent with them all being preserved still in their detrital condition.
If deformation in the fold had been brittle, that is, after lithification, then some localized fracturing of grains and the rock fabric might be evident at the microscopic scale in samples from the fold, especially in the hinge zones. However, there are only a very few possible localized fracture zones evident in these Tapeats Sandstone samples (fig. 32). Whereas such localized fracture zones might be expected in the hinge zones of the fold in contrast to the limb zones and distal samples, there does not appear to be any such preferential occurrence. Indeed, one distal sample not only does have a possible localized fracture zone cut across the rock fabric, but another fracture zone cuts across and is confined to a large subrounded detrital quartz grain (fig. 32a–c). Furthermore, linear zones of broken quartz grains as indicators of fracture zones are found in both limb and hinge zones of the fold. Thus, it is by no means certain that this fracturing occurred during the deformation of the sandstone beds in the fold. In the case of the quartz clast with the fracture zone across it in the distal sample, that fracture zone could have been in the original quartz grain in its source rock when it was eroded, or it could have been caused during the deposition and subsequent compaction processes. Likewise, the presence of a large intact edge-on muscovite flake associated with a possible localized fracture zone within a hinge zone sample suggests the fracturing was in that rock prior to the deformation in the fold. Of course, some fracturing could also have occurred after the folding deformation as a result of minor earth movements after lithification.
Finally, calcite veinlets or linings on and between grains, and patches associated with alteration of K-feldspar grains and former laths, and of some large altered and expanded muscovite flakes, is evident in some of the sandstone samples (fig. 33). These calcite linings and patches appear to be more prevalent in three of the four distal sandstone samples (fig. 33a–f) than in the samples from the fold (fig. 33g–n). Furthermore, among the fold samples much of the calcite is in patches associated with altered K-feldspar grains and former laths, primarily in samples from the limb zones, but prominently in one hinge zone sample. Yet the observation that an unaltered edge-on muscovite flake with a slightly bent end has some calcite patches associated with it between the surrounding sub-angular to sub-rounded quartz grains suggests the calcite is late-stage alteration not associated with, not a result of, the deformation of the sandstone beds in the fold.
Observations from the Cathodoluminescence (CL) Images
The grains and textures of three sandstone samples in prepared thick sections were imaged using the CL microscope stage—one distal sample, TSS-03 (fig. 1), and two fold samples, CCF-03 from a limb zone and TSS-10 from a fold hinge (fig. 21). The CL images obtained are compiled alongside to the right of the equivalent view in normal optical mode in figs. 34–36.
In the CL images of all three samples (figs. 34–36) the detrital quartz grains and the quartz cement are such a dark purple-black color that they are barely visible, so no further information about them can be ascertained. On the other hand, the K-feldspar grains are a strong mid-blue color with peripheral and some internal lighter blue patches, likely indicating a slightly different composition, probably due to alteration. Those patches are very evident in sample CCF-03 (fig. 35f), and also the cleavage is clearly marked (fig. 35d). Otherwise, the bright-red-colored grains are calcite, especially evident in sample TSS-03 (fig. 34b and d). It is very clear that the calcite is alteration often associated with the K-feldspar, which is evident in distal sample TSS-03 (fig. 34d), and even fold hinge sample CCF-10 (fig. 36d). So, when calcite alteration occurs, it has similarly affected the sandstone regardless of location.
The Silica Cement
The cement binding the detrital grains together is silica as quartz overgrowths (figs. 24 and 37). It is evident that in most instances this silica filled most of the initial pore spaces between the deposited sand grains during and subsequent to compaction and during dewatering, leaving very few very small pore spaces in the resultant sandstone. The cement appears to be in pristine condition, that is, still in its original condition from precipitation during lithification. A close look at the rock fabric and the silica cement under the petrographic microscope, supplemented by scanning electron microscope (SEM) imaging, thus supports the observation that lithification occurred after the deformation. However, if lithification occurred before the deformation of these sandstone beds in the fold, then the silica cement might show evidence of being fractured by the deformation but then being healed.
Petrographic Microscope Observations
The critical petrographic microscope observation is that the silica cement and the quartz overgrowths around dust and iron-oxide-outlined original detrital quartz grains are in the same condition in the samples from the fold as in the distal samples (figs. 24 and 37). Furthermore, there is no difference in the silica cement condition between the samples from the hinge and limb zones in the fold. Thus, the effects and outcome of the lithification of the deposited sand layers under the overburden pressure of the overlying strata and slightly elevated temperature are uniform throughout the resultant Tapeats Sandstone.
As reported above, the quartz grains that dominate the rock fabric are still preserved in their original detrital condition, as evident in the many sub-rounded grains that are outlined by dust and iron oxides with quartz overgrowths in optical continuity with them in many of the samples (figs. 24 and 37). And the observation that those quartz overgrowths meet at triple points, as do many of the overgrown quartz grains in which their original detrital shapes are not still outlined (fig. 25), is consistent with that configuration being the most ergonomic as precipitation of the silica occurred in the pore spaces between the compacted sand grains. Furthermore, the prevalence of overgrown quartz grains with no internal outlining of the original detrital grains would suggest that much of the silica that precipitated as quartz cement during dewatering of the sediment was derived from being dissolved in the pore waters from the edges of those original detrital quartz grains aided by pressure solution at grain-to-grain contacts as the quartz grains were compacted.
If deformation of the sandstone beds in the fold occurred after lithification, then the cement would have fractured and then healed. However, there is no evidence of that, since the condition of the silica cement is the same in the samples from the fold as in the distal samples. Any silica-carrying fluids permeating the sandstone to heal the fractured silica cement would surely have also healed the fractures within the quartz grains (fig. 28), and perhaps even some of the more prominently outlined sub-grains within the few original detrital quartz grains that have them (fig. 26). However, the fractures in some quartz grains and the fracture zone in one quartz grain in a distal sample (fig. 26a and b), as well as the prominently outlined sub-grains in the few quartz grains that have them, have not healed. And that would have required an adequate supply of silica in whatever connate water remained in the very few very small pore spaces still within the compacted and lithified sandstone. Since there are almost no fracture zones evident in the rock fabric apart from a few possible localized ones (fig. 32), there would have been no pathways for externally derived silica-carrying fluids to permeate the sandstone to deposit the silica and heal fractures within quartz grains and sub-grains. Indeed, the only evidence of post-lithification alteration deposits around quartz grains, and not within them along fractures, is calcite (fig. 33).
Whereas petrographic microscope observations produce two-dimensional images, the scanning electron microscope (SEM) produces three-dimensional images. This enabled closer examination of both the detrital quartz grains and the silica cement. Figs. 38–47 provide the SEM images at various recorded magnifications for selected samples—three distal samples, a sample from each of two hinge zones in the fold, four samples from the limbs of the fold, and one sample proximal to the fold’s limb.
It should be noted that the surfaces of the samples that were imaged were made by breaking the rocks open, so that can result in broken grains and/or cement, which should be evident in the resultant images. Nevertheless, the features evident in these SEM images were found to be the same no matter the location of the sample, whether distal to the fold or from the hinge and limb zones of the fold. That observation is critical because it reinforces the conclusion from the petrographic microscope examination that the conditions within the Tapeats Sandstone since deposition of its constituent sand grains, principally quartz grains with secondary K-feldspar grains and former laths, and muscovite flakes, have been uniform throughout the extent of the rock unit within Grand Canyon. That is, conditions in the history of the sandstone have not been different during its deformation in this fold compared to the same sandstone distant from this fold. Detailed observations of each sample justify this conclusion.
Samples TSS-01, 02, and 03 are sandstone samples distal to the fold (fig. 1). The progressive magnification of images (a)–(e) in fig. 38 reveal the tight but open porosity in the broken surface of clean quartz-cement-covered detrital quartz grains in sample TSS-01. Many clean faces of quartz cement crystals are visible, best seen in higher magnification in (d) and (e). Note that there has been no disturbance or displacement relative to one another of these pristine quartz cement crystals. It is very clear that once the quartz cement crystals had grown, they locked in the detrital quartz grains as the rock lithified and no breakage of the cement and displacement of the cement crystals occurred subsequently. Also visible in images (c)–(e) is the partial dissolution of detrital K-feldspar grains and former laths, evidenced by the open parallel lamellar structure remaining that reflects the original cleavage. And in image (e) it can be seen that “wavy” illite-smectite (mixed-layer clay) and “hairy” illite have grown on the apex of the partially dissolved K-feldspar grain, the product of the dissolution of the K-feldspar. In fig. 38f can be seen a fracture or crack across and through the quartz cement covering detrital quartz grains. It propagates across into the adjoining cement-covered grain and on its crest can be seen illite-smectite grown into and over the crack, indicating the illite-smectite growth occurred after the fracturing. Since this sample was situated many miles away from any folds, this fracturing was not caused by deformation, but probably by the compactional loading on the sandstone by deposition of the overlying sedimentary layers. In fig. 38g the beveled edge of the clean face of the quartz cement crystal would have been originally in contact with another quartz-cement-covered quartz detrital grain but the two cement crystal faces were broken apart during sample preparation for the SEM imaging. Yet across the lower face of that beveled-edged quartz cement crystal can be seen the remains of dissolution of an adjacent K-feldspar grain. And finally, in fig. 38h two cracks or fractures are visible with tiny displacements due to the compactional loading. The narrower of the two fractures displays minimal displacement and as the upper right-hand corner of the image shows has been significantly healed, likely by silica derived from the local dissolution of adjacent K-feldspar seen across the bottom of the image. Furthermore, in several places along the length of the wider fracture can be seen some bridging “hairy” illite that has grown subsequent to the fracturing.
Sample TSS-02 consists of coarser quartz grains, as can be seen in the progressively magnified images (a)–(d) in fig. 39. This sample is poorly sorted because it also consists of a mixture of quartz grain sizes and some lamination appears evident in image (a). At the higher magnifications in images (b)–(d) some clean faces of quartz cement crystals covering detrital quartz grains and the dissolution of some scattered K-feldspar grains can be clearly seen. A crack can also be seen between two such quartz cement crystals and extends further back between the clean faces of several more quartz cement crystals. Image (d) shows concentric growth zones within one of those quartz cement crystals as well as places where the crack has been overgrown with probable illite-smectite and silica, the ingredients provided by the local dissolution of the adjacent K-feldspar grains. The crack between the originally meshed faces of these adjoining quartz cement crystals was opened post-cementation by the compactional loading. The highly magnified images (e) and (f) in fig. 39 show the crystallites as typical features produced by dissolution of K-feldspar, grown as both straight and curved “hairy” illite. In image (g) are some clean faces of quartz cement crystals (that cover detrital quartz grains), as seen in the upper left corner, and one of which has a euhedral termination (left-hand bottom corner). Across the middle of the image can be seen clumps of “hairy” illite that grew from dissolution of K-feldspar grains, visible to the far left. To the far right in the image is an open linear pore, likely opened by compactional loading as the clean edge of a quartz cement grain borders the left side of the pore. Bordering the pore’s right side is illite-smectite covering the face of the adjoining quartz cement grain. Image (h) is the highly magnified center of image (g) and shows the very fine crack between adjoining quartz cement grains which has been bridged by the subsequent growth of a clay mineral, likely mixed layered illite-smectite.
Images (a) and (b) in fig. 40 show the quartz cement covering the detrital quartz grains in sample TSS-03 with evidence of occasional coatings on them from the dissolution of scattered adjacent K-feldspar grains. In the more magnified images (c) and (d) can be seen the conchoidal fracturing of some of the quartz cement caused during sample preparation. A crack separating several quartz cement grains can also be seen running across these images that bifurcates laterally (center left). There is no displacement along this crack, which was likely widened from the original grain boundaries by the continuing effects of compactional loading subsequent to lithification, but there may be some dissolution of quartz, which could have been aided by the presence of calcite in this sample. Otherwise, illite-smectite has grown on some of the faces of the quartz cement grains. In figs. 40e and f can again be seen the clean faces of quartz cement crystals overgrowing detrital quartz grains, with good matching of the clean faces between crystals. Also, illite-smectite can be seen around the crystal edges having grown along the contacts between the quartz cement crystals. Fig. 40g is the highly magnified portion of the brighter area to the left of the top middle of image (e) and shows the illite and illite-smectite that has grown on the surface of a quartz cement crystal that covers a detrital quartz grain, these clay minerals having grown after the cementation during lithification and demonstrating no subsequent disturbance to them.
Sample CCF-01 is from a fold limb zone in the Carbon Canyon fold (fig. 21). In the progressively higher magnification images (a) through (c) of fig. 41 can be seen the macro-texture of the broken-open surface of this sample, which reveals the quartz cement that covers the detrital quartz grains. Clean faces of the quartz cement crystals can be seen, especially in image (c) where right in the middle can be seen an excellent euhedral quartz crystal termination. The detrital quartz grains appear to be well cemented together by the overgrown quartz cement that infilled most of the original pore spaces left between them after their deposition. There do not appear to be any fractures with dislocations or fracture fillings, those tiny fractures likely present only having occurred due to continued compaction after lithification. Even though this sample comes from within the fold near a hinge zone, there is no evidence or features that the folding deformation occurred after lithification and/or during the continuing compactional loading. Porosity in this rock’s fabric is limited to the tiny narrowed passages (“pore throats”) and the tiny residual pore spaces between the quartz cement crystals grown over the detrital quartz grains. It is the normal porosity left by grain-to-grain contact and the overgrown quartz cement. If the folding deformation had occurred after lithification, then there should be significant dislocations evident, yet there are none. Otherwise, the porosity has been partially infilled primarily by undisturbed “wavy” mixed-layered clay illite-smectite. In fig. 41d significant dissolution of K-feldspar grains can be seen, with overgrown illite-smectite visible to the right. Image (e) shows a zone of complete quartz cementation over several adjoining detrital quartz grains, but across the center is a pore space produced by an intact open joint along the crystal-to-crystal contact boundaries with bordering clean quartz cement crystal faces, the quartz cement crystal to the right being euhedral. No dislocation has occurred, nor has any wavy illite-smectite grown within the joint. Image (f) is a magnified view of the texture produced by the dissolution of K-feldspar in image (d). Images (g) and (h) show the tight contacts between quartz cement crystals with many clean crystal faces and no evidence of any dislocations subsequent to the cementation (lithification). Scattered across image (g) and to the right of center in image (h) are patches of illite-smectite that has grown in pores and along pore “throats.”
Sample CCF-02 is from the hinge zone within the Carbon Canyon fold close laterally to sample CCF-01 (fig. 21). The progressively magnified images (a) through (c) in fig. 42 show the quartz cement crystals covering the detrital quartz grains are better sorted and finer-grained than in the adjoining sample CCF-01. Yet there is no difference in the packing of the quartz cement crystals and the detrital grains they have overgrown in this hinge zone sample CCF-02 compared to the adjoining limb zone sample CCF-01 (fig. 41). Image (d) of fig. 42, which is the central portion of image (c) magnified, shows there has been some dissolution of quartz at quartz cement crystal contacts and that has locally grown again (precipitated) at the same crystal orientation and in optical continuity. Fig. 42e and f show that the cementing together of the quartz cement crystals grown over the detrital quartz grains has not been fractured or displaced by the deformation in the fold’s hinge zone so the cementing (lithification) had to occur after the deformation. The faces of the quartz cement crystals are clean, and the open porosity is typical of normal diagenesis, all of which is clearly evident in the middle of image (f). To the right in image (f) there has been some dissolution of quartz cement crystals, with similar dissolution perhaps evident on the edges of most other quartz cement crystals. Likewise, images (g) and (h) show the quartz cement crystals grown over the detrital quartz grains have clean faces and are locked in (cemented) together with no fracturing or dislocations between or within crystals. In the bottom right corner of image (h), which is the magnified portion just below and left of center of image (g), can be seen dissolution of the quartz cement with illite and illite-smectite in its place, similar to scattered locations within image (g).
Samples CFF-04 and 08 are progressively more distant from the CCF-02 hinge zone laterally along the fold’s limb (fig. 21). Images (a) through (d) of sample CCF-04 in fig. 43 are progressively magnified and show the general texture of this sandstone sample which is poorly sorted with grains of various sizes. The quartz cement crystals grown over the detrital quartz grains are juxtaposed tightly together with no open fracturing or dislocations. In images (c) and (d), the brighter areas are dissolution of scattered K-feldspar grains, which would have been the local source of ingredients for silica and illite formation. Additionally, the quartz cement crystals covering the detrital quartz grains display clean faces with no fracturing or dislocations and some with euhedral terminations, all of which is compatible with the lithified rock not having suffered from any stress or strain. Fig. 43e shows two quartz crystals cemented together displaying the typical conchoidal fracturing produced during breaking the rock apart in sample preparation, while image (f) is a magnified view of that conchoidal fracturing. In images (g) and (h) the quartz cement can be seen between and covering the detrital quartz grains, with the upper half of (g) being almost continuous quartz cement. The joint boundaries between quartz cement crystals can be seen in (g) and are magnified in (h), yet the quartz cement crystals are tightly interlocking. There is also a protrusion where there is no extension of the rock fabric and where there would be expected to be fracturing, but there is not. Otherwise, there are small patches of quartz dissolution and some tiny illite and illite-smectite growth.
Sample CCF-08 in fig. 44a consists of larger detrital quartz grains well cemented by quartz overgrowths that display clean faces. Images (b) through (e) in fig. 44 are progressive magnifications of image (a) so that more details of the quartz cement crystals can be seen. A significant fracture can be seen across images (c) through (e) that in part follows the boundaries between several quartz cement crystals but then traverses a euhedral quartz cement crystal in (e). There is no significant dislocation along the fracture and across that euhedral quartz cement crystal indicating it was caused by the continued compactional overloading after cementation (lithification) rather than post-lithification deformation. The fracture appears to have been partially cemented. The striated and banded features in the euhedral quartz cement crystal are indicative of concurrent growth of two phases of quartz cement between two clean faces of that euhedral crystal. Overall, the quartz cement crystals have been well knit together, as images (c) through (e) show, with no dislocations due to deformation, so lithification must have occurred after cementation (lithification). Fig. 44f shows dissolution of an area of the quartz cement having created a pore, while image (g) shows dissolution of a probable K-feldspar grain with some illite growth and some illite-smectite in the upper left. Finally, in images (g) and (h) are excellent euhedral growth terminations and clean faces of adjacent quartz cement crystals that are well knit together, locked in with no fracturing or dislocations, consistent with the cementation (lithification) being after the deformation which produced the fold.
Sample CCF-10 is from another hinge zone within the Carbon Canyon fold (fig. 21). Fig. 45a–e progressively magnify the general texture and content of the sandstone, which consists of finer grained detrital quartz grains overgrown by quartz cement crystals. Even though during sample preparation the quartz cement was broken, leaving a rough surface, there are still some clean faces on some of the quartz cement crystals. There are also scattered patches of likely dissolution of K-feldspar grains with the in situ growth of “hairy” illite and “wavy” illite-smectite, best seen in images (c) through (e). In fig. 45f it can be seen from the extensiveness of the quartz cement, that the cement crystals grown over the detrital quartz grains are not only well cemented and thus were locked into place during lithification, but there has been no subsequent dislocation or disruption of the cement, so the deformation that produced the fold had to occur prior to the cementation (lithification). Small patches of dissolution can also be seen, probably of the quartz cement, with the growth in situ of the clay minerals, illite and illite-smectite. Image (g) is a magnification of the middle left portion of image (f) and again shows the clean faces of the quartz cement crystals, some of which have euhedral terminations, that have overgrown the detrital quartz grains. And finally, image (h) is a magnification of the lower left corner of image (g) and shows more clearly the illite and illite-smectite in a cavity produced by dissolution of some quartz cement.
Sample CFF-11 is from the fold limb close to the CCF-10 hinge zone (fig. 21). In fig. 46a–c the freshly fractured face of the rock produced by the sample preparation displays the general texture, which shows the relationship between the quartz cement that overgrew the detrital quartz grains and the occasional K-feldspar resulting in moderate to well cementation of the sand. Most of the cement is quartz crystals grown over the detrital quartz grains with some late illite coatings. None of the quartz overgrowths are fractured or displaced from the host detrital grains, so that implies any movement or slippage of the detrital grains occurred prior to the quartz cementation lithifying the rock and locking in its texture. Fig. 46d–e shows a possible minor fracture or joint. The surfaces on either side were not bonded or cemented and are not clean but seem to have a corrosion or suturing overprint. This would imply movement of grains had ceased and compactional loading became dominant, creating the pitted and possibly sutured joint surfaces. The upper surface displays numerous micro-quartz crystals with characteristic pointed terminations, while the large crystal on the lower surface is a quartz crystal and not chert. Some minor dissolution of the detrital quartz grains or even quartz cement surfaces elsewhere may have been the source of this local quartz cement. Note that the quartz overgrowths are undisturbed. Any displacement between all these quartz crystals would have resulted in fracturing of this cemented joint. As with the other samples, this is indicative of the lithification (cementation) occurring after fold deformation and not before, as the cement shows no evidence of being disturbed once the detrital grains were locked in place with the cement. Fig. 46f–g shows the close association of the diagenetic quartz cement and the “hairy” clay mineral illite. It is possible that lamellar illite was deposited first on the substrate quartz detrital grains, and then quartz overgrowths occurred followed by hairy illite growing either syn-or post-quartz, implying at least two possible illite growth events. Fig. 46h–j shows the dissolution of a K-feldspar grain, which was a possible source of diagenetic quartz and the illite. The lath-like structures in fig. 46j are typical of feldspar dissolution preferentially along cleavage planes.
Sample CCF-12 was collected a short distance (about 100 m) laterally from the fold, well beyond the limb zone of sample CCF-08 (table 1). Images (a) through (f) in fig. 47 are the progressive magnification of the broken surface produced during sample preparation. The texture is medium-grained and identical to all other samples in that the quartz cement crystals have grown over the detrital quartz grains to lock them well-cemented in place, yet often exhibiting clean faces. There is also no evidence of any dislocations due to any disturbance after lithification (cementation), although there are fine cracks around a few boundaries between some quartz cement crystals. In images (e) and (f) one such crack also traverses across the corner and two faces of a clean-faced quartz cement crystal. Where that crack traverses the side face it is cemented and not displaced, even where it merges into the crystal boundary again. There is no evidence of grain rotation, and thus this is a normal fracture due to continued compactional loading subsequent to cementation (lithification). In image (f) a small blocky piece of quartz cement can be seen (to the left of the middle) attached to the clean face of the quartz cement crystal and underneath and to the left of it is a horizontal line across that clean face. That is a dust rim that would be in thin section outlining the edge of the original detrital quartz grain, and that small blocky piece is a fragment of quartz cement over the top of it. Otherwise, the crack below and beneath that quartz cement crystal is wide enough to have been an open fluid pathway. Then in the bottom left on image (f) some illite-smectite has grown on the quartz cement. Fig. 47g is an isolated image that again shows the conchoidal fracturing of the quartz cement that occurred during sample preparation, but it also shows the clean faces of the quartz cement grains. Images (h) through (j) are a progressively magnified sequence that again shows the clean faces of quartz cement crystals, one with a euhedral termination and also with growth banding. There is also dissolution of one face of a K-feldspar grain and perhaps of some quartz, the dissolution products being the ingredients for the growth of “hairy” illite and “wavy” illite-smectite plus possibly some quartz. The “hairy” illite bridges some of the pores produced in the dissolution cavity.
It is clearly crucial to first determine the likely temperature and pressure conditions the Tapeats Sandstone was subjected to at the depth to which it was buried after its deposition, and before it was then uplifted with the Kaibab Plateau and folded during the Laramide orogeny. Those determined temperature and pressure conditions will automatically rule out any expectation of certain macroscopic and microscopic features in the Tapeats Sandstone within the Carbon Canyon fold due to the deformation. Indeed, the observation of the remaining macroscopic and microscopic features will confirm the deduced temperature and pressure conditions and enable a conclusive case to be made for ductile or brittle deformation, or for soft-sediment deformation, to have been involved in the folding mechanism, and it will also determine the timing of lithification with respect to the folding.
Temperature and Pressure Conditions at the Burial Depth
There are several methods for estimating the temperatures and pressures to which the Tapeats Sandstone was subjected. However, first it is easy to calculate the depth of burial because the thickness of the overlying strata has been measured. According to Blakey and Middleton (2012) the Paleozoic stratigraphic section in Grand Canyon comprises >1,000 m of strata, but their scaled stratigraphic column suggests a more detailed estimate of ~1,350 m (~4,430 ft). Then based on the diagrammatic cross-section in Morales (2003) the Grand Staircase of Mesozoic and Cenozoic strata total a thickness of ~1,220 m (~4,000 ft), although Karlstrom, Timmons, and Crossey (2012) suggest a thickness of ~2,000 m (~6,560 ft). Thus, the total conservatively estimated thickness of Phanerozoic strata in the Grand Canyon-Grand Staircase region would be ~3,350 m (~10,990 ft). However, that is a lower estimate than that of Dumitru, Duddy, and Green (1994), who estimated that the Cambrian strata of the Tonto Group, which includes the Tapeats Sandstone, would have been, prior to the erosion of the Mesozoic section from off the top of the Grand Canyon’s Paleozoic sequence, at a depth of burial of between 4.5 km (~14,750 ft) and 6 km (~19,500 ft), although that estimate was based on apatite fission-track data. In any case, it is highly doubtful the entire thickness of the Grand Staircase was covering the Grand Canyon region, as it likely thinned dramatically, like the Grand Canyon Paleozoic sequence does to the north and northeast. Therefore, we can conclude that the Tapeats Sandstone was possibly buried under ~3,300–4,500 m (~10,825–14,750 ft) of overlying strata which had progressively accumulated during the Phanerozoic.
Since the Tapeats Sandstone sits unconformably on the Precambrian basement granites and schists in the Upper Granite Gorge of Grand Canyon, then those granites and schists would have been buried under a similar thickness of Phanerozoic strata deposited directly on the granites and schists after erosion of the Great Unconformity. It is significant, therefore, that the biotite flakes within the Vishnu and Rama Schists of the Granite Gorge Metamorphic Suite contain very abundant 238U and 210Po radiohalos, while biotite flakes in several of the granite plutons of the Upper Granite Gorge contain somewhat fewer numbers of 238U and 210Po radiohalos (Snelling 2005a) (fig. 48). These radiohalos would have been readily annealed if the temperature at their burial depth under the overlying Phanerozoic strata had reached 150°C (Laney and Laughlin 1981). Thus, we can conclude that the burial temperature beneath the Phanerozoic strata did not reach 150°C, as the Tapeats Sandstone was not likely buried as deep as some claim.
A similar paleotemperature indicator is the presence of fission tracks in numerous minerals in the Tapeats Sandstone. Snelling (2005b) reported fission tracks in zircon grains from a tuff bed within the Tapeats Sandstone in the western Grand Canyon (fig. 49), while in this study fission tracks were found in quartz grains in a sample from the Carbon Canyon fold (fig. 50). Fission tracks in both zircon and quartz have been experimentally determined to be annealed at elevated temperatures above 300°C (Sandhu et al. 1990). Naeser et al. (1989, 2001) and Dumitru, Duddy, and Green (1994) found that the apatite fission-tracks in the Proterozoic rocks below the partial annealing zone (below the base of the Redwall Limestone) yielded ages of 61–66 Ma and the shortened fission-track lengths suggested that those rocks at the bottom of Grand Canyon cooled to temperatures of 60–65°C during uplift and erosion associated with the Laramide deformation after the Proterozoic basement rocks had been at a burial temperature of ≥110°C during the late Cretaceous prior to the Laramide event. In contrast, Naeser et al. (1989) found that the fission-track ages of ~1,000 Ma obtained from zircons from Proterozoic basement rocks now exposed at river level indicated that those rocks had been at temperatures of ≤200°C for the last 1,000 million years.
Subsequently, Kelley, Chapin, and Karlstrom (2001) used apatite fission-track ages and track length data collected at river level in eastern Grand Canyon to calculate that the Proterozoic basement rocks had cooled during the Laramide deformation to 55–65°C. They also found, as did Naeser et al. (1989), that the apatite fission-track ages obtained from the Proterozoic rocks along the Colorado River generally increased toward the west, perhaps reflecting the differences in the uplift elevations. Kelley and Karlstrom (2012) reported additional new apatite fission-track ages in eastern Grand Canyon and Marble Canyon. They also found that the apatite fission-track ages are progressively younger toward the east and northeast. For example, in the Supai Group the apatite fission-track ages decreased from 127 ± 13 Ma near Grand Canyon village to 33 ± 6 Ma at river mile 12. Additionally, the apparent apatite fission-track cooling ages on the upthrown blocks on the major monoclines in the eastern Grand Canyon were higher at 80–90 Ma than the 55–65 Ma on the downwarped side of the East Kaibab Monocline. This suggested to them that the Supai Group in the downwarped side of the East Kaibab Monocline to the northeast in Marble Canyon had cooled through 110°C much later than in the East Kaibab uplift and was indicative of the erosional retreat of the Grand Staircase escarpment that exposes ~2 km (~6,560 ft) of Mesozoic strata which may have been stripped away from the Grand Canyon region.
Flowers et al. (2007) and Flowers, Wernicke, and Farley (2008) used apatite (U-Th)/He thermochronology data to constrain the cooling history of eastern Grand Canyon to <70°C. Eight samples from the Upper Granite Gorge yielded apatite (U-Th)/He dates of 23 ± 3 Ma to 55 ± 7 Ma, but their modeling suggested complete resetting had occurred during peak temperatures near the end of Cretaceous sedimentation, followed by cooling during the Laramide deformation event. In contrast, samples from Permian and Triassic sedimentary units in eastern Grand Canyon yielded a broad span of apatite (U-Th)/He dates of 5–104 Ma, but they similarly explained the thermal history of those ages based on a large range of accumulated radiation damage due to the wide range of uranium contents of the detrital apatite grains.
Flowers and Farley (2012) added apatite 4He/3He thermochronology data to the discussion of the cooling history of Grand Canyon’s basement rocks. They found that the 4He/3He spectra of single apatite grains from basement rocks in eastern Grand Canyon with differing (U-Th)/He dates, radiation damage and U-Th zonation yield a self-consistent cooling history that substantially validated the He diffusion kinetic model they applied. In their modeling assuming a 20–25°C/km geothermal gradient thermal histories were fitted through 110° to 120°C peak temperatures at 80 to 85 Ma, as suggested by complete annealing of apatite fission-tracks at this time (Dumitru, Duddy, and Green 1994), and cooling to the 20° to 25°C surface temperature by present-day. Statistically acceptable paths imposed tight constraints on the ~90° to 30°C thermal history experienced by eastern Grand Canyon, which are consistent with, but more restrictive than, the history inferred from the apatite (U-Th)/He dates alone (Flowers et al. 2009) and apatite fission-track data from the same area.
Finally, Peak et al. (2021) and Thurston et al. (2022) used zircon (U-Th)/He thermochronology data obtained from the Precambrian crystalline basement rocks in eastern Grand Canyon to constrain the thermal history of the unroofing of the Great Unconformity. They found that their data and models were also highly sensitive to late-stage reheating due to burial beneath ~3–4 km (~9,840–13,120 ft) of Phanerozoic strata prior to ca. 60 Ma. Their models that best matched observed date-equivalent uranium trends showed maximum burial temperatures of 140–160°C, which are in agreement with the available apatite (U-Th)/He and apatite fission-track data.
In contrast, as the basis for a totally different method to determine burial temperatures, experimental studies of the conversion of smectite to illite have demonstrated its potential use as a geothermometer (Essene and Peacor 1995; Huang, Longo, and Pevear 1993), which has been confirmed by field studies (Hillier et al. 1995; Pollastro 1993; Pytte and Reynolds 1989; Renac and Meunier 1995; Smart and Clayton 1985; Velde and Espitalié 1989; Velde and Lanson 1993). Similarly, many studies have demonstrated the value of using illite crystallinity as an indicator to distinguish between diagenesis, very low-grade metamorphism and low-grade metamorphism (Barrenechea, Rodas, and Mas 1995; Blenkinsop 1988; Frey and Robinson 1999; Kisch 1983, 1987; Kubler 1964, 1967, 1968; Kubler and Goy-Eggenberger 2001).
However, the smectite/illite ratio relationship to temperature appears to be neither simple nor unequivocal, because of various factors such as the ion content and concentrations in interstitial waters and the geothermal gradient, not just at the present time but also during the history of the sediment pile. Nevertheless, Hower (1981) found clear relationships between depth, temperature, and the percent illite in illite interstratified with smectite in the sediments intersected by oil wells in the Gulf of Mexico coast region (fig. 51) (Pollastro 1993), one of which is directly comparable to the sedimentary strata sequence in the Grand Canyon-Colorado Plateau region. There Dumitru, Duddy, and Green (1994) estimated that the Cambrian strata of the Tonto Group, which includes the Tapeats Sandstone, would have been, prior to the erosion of the Mesozoic section from off the top of the Grand Canyon sequence, at a depth of burial of between 4.5 km (~14,500 ft) and 6 km (~19,500 ft), with their apatite fission-track data suggesting temperatures of between 110° and 130°C, as also determined by the subsequent studies discussed above. In fig. 51 the percent illite in the illite interstratified with smectite in two samples from thin tuff beds within the Muav Formation and Tapeats Sandstone (Tonto Group) in Grand Canyon, as reported by Snelling (2005b, 265, table 3), were plotted on the curve from oil well (B), and projected onto the depth and temperature axes. This suggests that with that same geothermal gradient, these tuff beds would have been, prior to the erosion of the Mesozoic strata above, at depths of 4,800–5,600 m (~15,700–18,400 ft) and subjected to temperatures of between 110° and 130°C, consistent with the estimates by Dumitru, Duddy, and Green (1994) and the subsequent studies discussed above.
Dumitru, Duddy, and Green (1994) based their estimation on a pre-Cretaceous geothermal gradient of 20–30°C/km, and the geothermal gradient in the Miocene oil well (B) (fig. 51) is of the order of 20°C/km. Such a geothermal gradient is not unreasonable in the timeframe of the Genesis Flood event, given the catastrophic deposition of the thick Paleozoic and Mesozoic strata sequence (Austin 1994) and the elevated temperatures of the waters depositing those sediments (Austin et al. 1994). Thus, the estimates of depth and temperature based on the percent illite in the illite interstratified with smectite for these two tuff samples, though very approximate due to the likely large errors in the XRD determinations, are not unreasonable. Therefore, because of the consistency of these estimates with the apatite fission-track data of Naeser et al. (1989), Dumitru, Duddy, and Green (1994) and the subsequent studies discussed above, it seems reasonable to conclude that these two tuff units have since their burial only been subjected to maximum temperatures of 110–130°C, well below the 200 ± 40°C temperature for total annealing of fission tracks in zircon (Harrison et al. 1979; Hurford 1985; Zeitler 1985) and the 150°C temperature for the total annealing of radiohalos (Laney and Laughlin 1981).
The significance of the Kubler Index values calculated from the XRD clay mineral analyses of the two samples from the two tuff units (Snelling 2005b, 265, table 3) are harder to interpret from the available literature, which primarily focuses on low-grade metamorphism of sedimentary strata sequences. Estimating the temperatures to which these two tuff units were subjected based on these approximate Kubler Index values depends on the value of the Kubler Index used to define the boundary between diagenesis and the lowest grade metamorphism, which is otherwise defined by mineralogical changes in the clay minerals (Kisch 1987; Kubler 1967). As indicated by Blenkinsop (1988), early studies using the Kubler Index for illite crystallinity all adopted different values of the index to define this crucial boundary, so standardization was warranted. Using the standardized definition of Kisch (1991) and Brime (1999) with a Kubler Index of 0.42 for the boundary between diagenesis and the lowest grade metamorphism, as successfully applied by Brime, Talent, and Mawson (2003), the estimated Kubler Index values for the Muav and Tapeats tuffs (Snelling 2005b, 265, table 3) indicate that they are on the lower temperature side of this boundary, so they only suffered diagenesis. Temperature estimates for that boundary place it at 150 ± 50°C (Bucher and Frey 2002; Frey and Kisch 1987; Robinson and Merriman 1999). Thus, the Kubler Index values for these two tuff units are consistent with the estimate of 110–130°C for the temperatures to which these tuff units have been subjected from both the apatite fission-track data of Naeser et al. (1989), Dumitru, Duddy, and Green (1994) and the subsequent studies discussed above, and their smectite/illite ratios.
In conclusion, therefore, the consensus from all these estimation methods is that the Tapeats Sandstone prior to the Laramide deformation responsible for the Carbon Canyon fold would have been subjected to a burial temperature of 110–130°C. Then during the Kaibab uplift erosion caused the temperatures within the Tapeats Sandstone to decrease to <70°C. However, estimates of the burial depth vary, but based on measured strata thickness it was concluded above that the Tapeats Sandstone was possibly buried under ~3,300–4,500 m (~10,825–14,750 ft) of overlying strata which had progressively accumulated during the Phanerozoic. However, this is probably an overestimate of the thickness as the Phanerozoic strata which likely thinned to the south, and these strata (such as the Tapeats Sandstone and the Redwall Limestone) even vary in thickness within the walls of Grand Canyon. Thus, using a general overburden pressure gradient (Khan and Islam 2008), at those depths the overburden (confining) pressure on the Tapeats Sandstone would have been ~0.3–0.4 kbar (~4,300–5,900 psi). According to Bucher and Frey (2002, 5, fig. 1.1) these pressure-temperature conditions are well within the pressure-temperature field of sedimentary diagenesis. Thus, it is consistent that the mineralogy and textures (macroscopic or microscopic) of the Tapeats Sandstone do not indicate any signs of any metamorphic changes to the detrital grains (Snelling 2021), as confirmed by the petrographic and SEM observations reported in this study.
The Macroscopic Features
The next question to answer is whether the macroscopic features in the outcropping Tapeats Sandstone within the Carbon Canyon fold are consistent with ductile or brittle deformation of the sandstone beds long after their lithification, or with soft-sediment deformation of the sandstone beds soon after their deposition and before lithification. As already noted, though, the Tapeats Sandstone was most likely not buried deep enough to experience ductile deformation as it is well above the brittle-ductile transition zone. On the other hand, under some near surface conditions, rock layers may remain coherent because the grains and/or beds within them can facilitate folding due to brittle deformation. Thus, most near surface rock layers undergo brittle fracturing and faulting, leaving the rock’s grains fractured. Some coherent beds may slide past one another as the rock layers are folded via the process known as bedding plane or flexural slip, which should leave tell-tale features in the outcrop.
From field observations of the outcrop of the Tapeats Sandstone beds in the Carbon Canyon fold it is quite clear that bedding plane or flexural slip must have occurred to accommodate their folding. However, the hinge zones are open without shattering of the rock fabric, and generally there has been no thickening of the beds in most of the hinge zones (fig. 52). The fold would be best classified according to Ramsay (1967) as a Class 1B parallel-concentric fold (fig. 13), and corresponds to a Donath and Parker (1964) flexural-slip fold (fig. 12). The hinge distances are also open and there is no mechanical crowding or thinning of the sandstone beds in either the hinge zones or the limbs, contrary to the claims of Huntoon (2003) and Hill and Moshier (2009). Indeed, the thicknesses of the individual sandstone beds are very consistent along their lengths when traced from one limb through the hinge zone and out onto the opposite limb (fig. 21), contrary to the claims by Hill and Moshier (2009) and Tapp and Wolgemuth (2016) that the bedding thickness changes along the fold. Certainly, the sandstone beds have been dragged up to the Butte Fault as they were upturned through the ~90° fold, and at the Butte Fault they are chopped off and end (fig. 8). Furthermore, there is one very minor change in the direction of the fold hinges between only two sets of sandstone beds, while within those sets of sandstone beds the direction of the fold hinges remain the same (fig. 8). This is not quite the same as the claim of Tapp and Wolgemuth (2016) (fig. 10) in which they, with their annotated red arrows, have exaggerated the change of direction. And contrary to Tapp and Wolgemuth (2016), there is only the one hinge zone between those two sets of sandstone beds that has been thickened, and it is unclear whether it has been filled with weathered material or weaker deformed rock.
There are no clusters of fractures in the hinge zones, as would be expected if lithified rock had suffered from brittle deformation. And rather than simple fractures, one would expect to see faults that transgressed multiple beds. Instead, Fossen (2016, 157) has an illustration of fractures or joints that would have opened in a cluster around the stretched edge of the hinge zone of a folded bed as a result of strain during folding, yet such clusters are absent from the sandstone beds in the hinge zones of the Carbon Canyon fold. However, there are fractures, as on the annotated overlay provided by Tapp and Wolgemuth (2016). Yet, they are regularly spaced and most of them are confined to individual sandstone beds (fig. 10). They also penetrate totally across, but are confined to, individual sandstone beds, including in the hinge zones. This is not what would be expected if these were fractures due to ductile deformation. Instead, fractures in the hinge zones should be only open where the sandstone beds were stretched on the outer curve of the folded beds and compressed tightly shut on the inside curve.
Furthermore, rather than being due to ductile deformation as Tapp and Wolgemuth (2016) imply, these could be joints produced by contraction of the rock fabric during dewatering and lithification, and then especially during onloading of the confining overburden pressure as the overlying strata were eroded away during erosion of Grand Canyon and its side canyons, including Carbon Canyon. Joints are fractures or cracks with minute openings, with little to no displacement along their sharp walls (Fossen 2016; Schultz 2019). Indeed, one of the principal causes of the development of joints is the release of the vertical stress and thus the horizontal stress as well (to a lesser extent) during exhumation of the overburden (Fossen 2016), and in this case, the erosion of Carbon Canyon through the fold. And for the most part, joints come in populations defined by local stress fields, including diagonal sets, and are often regularly spaced according to the strength of the rock fabric (Fossen 2016; Groshong 1988; Schultz 2019), as can be seen in the annotated overlay provided by Tapp and Wolgemuth (2016) (fig. 10). Furthermore, joint spacing also depends on layer thickness, such that field observations and experimental work has demonstrated the very simple relationship that the joint spacing is more or less equal to the layer thickness, independent of scale (Fossen 2016; Narr and Suppe 1991; Silliphant, Engelder, and Gross 2002). This relationship is also somewhat evident in the Tapeats Sandstone beds bent in the Carbon Canyon fold (figs. 8 and 10).
There are other relevant field observations. If bedding plane or flexural slip has occurred, then the bedding planes should have acted like fault plane surfaces and thus slickensides might be found on them. In fact, potential slickensides were found on only one of the many exposed bedding plane surfaces examined (fig. 53). Thus, it is likely that slickensides on bedding plane surfaces in the Carbon Canyon fold are not prolific, yet this one occurrence is still significant. Equally significant is the occurrence of some faulting within some of the Tapeats Sandstone beds within the Carbon Canyon fold. Fig. 54 shows an apparent small fault with a very small offset within a single sandstone bed in one hinge zone that was sampled low in the outcropping fold in the canyon wall (near sample CCF-10 in fig. 21b). This same small fault was also reported by Tapp and Wolgemuth (2016) who claimed it was evidence for brittle deformation. Yet, this small fault appears to coincide with a cross-bedding parting surface, as it does parallel the cross-bedding, and it is confined to just part of the thickness of this one sandstone bed. This thus suggests that movement was only within part of the bed and facilitated by the cross-bedding plane surface, which means it was not related to brittle deformation fracturing.
And finally, within the long horizontal limb of the fold there is a drag fold within a finer-grained siltstone bed or lens that pinches out between the regular sandstone beds, the tight fold and the adjoining sandstone bed being also faulted (fig. 55). It would appear that at the time of the drag folding the siltstone bed or lens was less competent, due to being finer-grained and likely having some clay minerals within it, than the more competent adjoining quartz-rich sandstone bed. This drag folding and faulting may have occurred at the same time as the overall Carbon Canyon fold and may also be a product of the bedding plane or flexural slippage during the claimed ductile and/or brittle deformation.
But do these field observations preclude the Carbon Canyon fold being due to soft-sediment deformation before lithification of the Tapeats Sandstone, rather than due to ductile and/or brittle deformation after its lithification? The short answer is no, as demonstrated by experiments replicating soft-sediment deformation. Nabavi and Fossen (2021) have reviewed the history of such experiments, primarily undertaken in squeeze boxes with layers of dampened sand and/or clay, glass sides to the box and a crank handle for moving one end inwards towards the other fixed end so that the compressional folding of the dampened sediment layers can be simulated. Some excellent relevant examples are the simulation experiments of Rettger (1935), Handin et al. (1976), Friedman et al. (1976), Weinberg (1979), and Friedman, Hugman, and Handin (1980). These and other experiments involved confining pressures, and yet the dampened sand and/or clay layers when compressionally folded would appear to have faithfully simulated soft-sediment deformation to produce folds similar and identical to those observed and classified as folding due to soft-sediment deformation in exposed outcrops of now lithified sedimentary layers elsewhere (for example, Waldron and Gagnon 2011 and Alsop et al. 2019). Even the dragging vertically upwards of the Tapeats Sandstone beds by displacement on the Butte Fault and the beds ultimately being terminated and truncated by that fault have been simulated in these soft-sediment deformation experiments.
Waldron and Gagnon (2011) defined soft-sediment deformation, following Maltman (1984), as any deformation, other than vertical compaction, of a sediment or sedimentary rock that is achieved by rearrangement of the original sedimentary particles, without internal deformation of those particles or of any interstitial cement. They added that such soft-sediment deformation occurs primarily by the mechanism of grain-boundary sliding. In contrast, Borg et al. (1960) conducted a quantitative study of experimental deformation of sand grains washed from the St. Peter Sandstone of Illinois by applying a uniform confining pressure to simulate overburden pressure and differential load to simulate tectonic pressures. They found that purely cataclastic brittle deformation occurred resulting in fracturing of the sand grains as the most conspicuous feature. The fracture pattern was random under uniform deformation pressure, whereas the fracture-orientation patterns reflected the symmetry of the deformation under differential loading conditions. And most importantly, the apparent elongation and optic-axis orientations in the deformed samples were much the same as those in the undeformed sands. There was also no evidence that the experimental deformation had produced any deformation lamellae or that the overall occurrence of grains with undulose extinction had been changed. They found uniform loading did not reorient the fabric of the sands, whereas the differential loading (simulating tectonic deformation) resulted in preferred orientation of fractures, the optic axis, and apparent grain elongations, all of which reflected the orientations of the principal applied stresses.
In conclusion, all the features observed in the outcropping Tapeats Sandstone beds deformed in the Carbon Canyon fold, and described above, apart from the likely slickensides on that one bedding plane surface, are identical to those recognized and classified as due to soft-sediment deformation, both in the simulation experiments and in outcrops in other geological settings. The faulting and fracturing within the sandstone beds and the drag folding of the siltstone bed or lens between the sandstone beds have all been replicated in soft-sediment deformation experiments and observed in other outcrops elsewhere. Thus, these observed features do not necessarily support the claims of Huntoon (2003), Hill and Moshier (2009), and Tapp and Wolgemuth (2016) that the Carbon Canyon fold was produced by ductile deformation during the Laramide event ~450 million years after deposition, lithification, and progressive deep burial of these Tapeats Sandstone beds. Rather, the field evidence is still compatible with the Carbon Canyon fold having been produced by soft-sediment deformation of these Tapeats Sandstone beds soon after deposition and deep burial, and all before final lithification. However, since grain-boundary sliding is regarded as the essential process in soft-sediment deformation and the results of that process and features such as undulose extinction and deformation lamellae in quartz grains regarded as due to ductile deformation are only observed under the microscope, the microscopic evidence is thus crucial to definitively determining the timing of, and the conditions under which, the Tapeats Sandstone beds were deformed to produce the Carbon Canyon fold.
The Microscopic Evidence
As reported above, the critical petrographic microscope observations are that the silica cement and the quartz overgrowths around dust and iron-oxides outlined original detrital quartz grains are in the same condition (the quartz overgrowths being in optical continuity with the detrital quartz grains) in the samples from the fold as in the distal samples (figs. 24 and 37). Furthermore, there is no difference in the silica cement condition between the samples from the hinge and limb zones in the fold. The original rock fabric is still evident, with the detrital quartz grains still sub-rounded or sub-angular, varying in size and randomly mixed, resulting in a poorly to moderately well-sorted texture. And there is no significant difference in the porosity of the sandstone between distal and fold limb samples with fold hinge zone samples. These petrographic microscope observations are also emphatically substantiated by the SEM observations. Thus, the effects and outcome of the lithification of the deposited sand layers under the overlying overburden pressure and slightly elevated temperature are uniform throughout the resultant Tapeats Sandstone. In other words, the folding must have occurred before lithification of the sandstone beds and thus the Carbon Canyon fold must have been produced by soft-sediment deformation.
There are no deformation lamellae or deformation kink bands in the quartz grains as examined under the petrological microscope (figs. 24–27). Those would have been evidence for ductile deformation as demonstrated in experiments (Borg et al. 1960; Carter, Christie, and Griggs 1964; Christie, Griggs, and Carter 1964; Groshong 1988; Vernon 2018), so their complete absence is significant in ruling out ductile deformation having occurred. However, even though the quartz grains display uniform extinction and generally show no signs of undulose extinction under crossed polars, there are a few quartz grains where there is an appearance of slightly undulose extinction. These observations are also contrary to the outcomes of experiments on ductile deformation of quartz grains and microscope observations of quartz grains in ductile deformed rocks (Carter, Christie, and Griggs 1964; Groshong 1988; Vernon 2018; Wojtal, Blenkinsop, and Tikoff 2022). Those few quartz grains in the Tapeats Sandstone samples in this study, from the Carbon Canyon fold and distal from it, with observed slightly undulose extinction (fig. 27) can be easily explained. Either they could be an artifact of the original detrital quartz grains retaining unchanged the slight undulose extinction they had in their source rocks, or more likely, they acquired the slight undulose extinction during compaction. Borg and Maxwell (1956) and Borg et al. (1960) found that quartz grains in deformed sands and the undeformed St. Peter Sandstone, respectively, that had only experienced previous compaction exhibited a preponderance of grains with no undulatory extinction and only a few displaying various intensities of undulose extinction. On the other hand, Maxwell (1960) who did compaction experiments on sand and sandstone samples did not report any resulting undulose extinction. However, grain-to-grain compaction is known to cause undulose extinction due to grain rotation and contact point pressures during compaction (Adams, McKenzie, and Guildford 1984; Scholle 1979; Ulmer-Scholle et al. 2015), these processes being reported in experiments by Chester et al. (2004, 2007), Chuhan et al. (2002), de Boer, Nactegaal, and Duyvis (1977), Elias and Hajash (1992), Maxwell (1960), Miyakawa and Kawabe (2014), and Wolf and Chilingarian (1975), and are noted by Ulmer-Scholle et al. (2015). The pressure solution of a few quartz grains from compaction is also evident in the SEM images in this study (figs. 38–47).
Fractures within quartz grains are usually subtle and only more pronounced in rare grains (fig. 28). In most cases, the pronounced fractures are in quartz grains primarily in samples distant to the fold. In some samples there are occasional broken quartz grains, though the breakage is not pronounced nor is the displacement of the pieces (fig. 29). And again, these occurrences are just as prevalent in samples distal to the fold as in samples from the fold. The SEM images (figs. 38–47), as described above, indicate that this fracturing of quartz grains is due to the compaction produced by the overburden pressures of the overlying strata. This is further confirmed by the detrital muscovite flakes in many of the samples in this study that are observed to have been bent around the detrital quartz (and K-feldspar) grains including those that have been fractured and broken, while a few muscovite flakes are also broken (fig. 31a, h, o, p, q, x, b’). Once again, the bent and broken muscovite flakes are present as often in the distal samples as in the samples from the Carbon Canyon fold, and they are just as prevalent in the hinge zones compared to in the limbs of the fold. Those detrital muscovite flakes would have been initially deposited flat between the quartz and K-feldspar grains parallel and sub-parallel to the bedding because of their sheet structure, but were then bent subsequently during compaction, which at the same time fractured some quartz grains and broke both a few quartz grains and even some of the muscovite flakes.
Sediment compaction producing fracturing of quartz grains has been thoroughly demonstrated in many experiments (Borg et al. 1960; Borg and Maxwell 1956; Carter, Christie, and Griggs 1964; Christie, Griggs, and Carter 1964; Chester et al. 2004, 2007; Chuhan et al. 2002; Elias and Hajash 1992; Gallagher et al. 1974; Groshong 1988; Karner et al. 2003; Maxwell 1960). In fact, the experiments demonstrate that a large overburden load that produced high confining pressures should, over a sustained period of hundreds of millions of years, have produced a lot of obvious fracturing and breakage of quartz grains, vastly more than the few subtle fractures and rare broken quartz grains observed in the Tapeats Sandstone samples in this study, regardless of whether they are samples from the fold or distal to the fold. This latter observation is clearly at odds with that experimental outcome. It is thus possible to conclude that the overburden load overlying the Tapeats Sandstone was not sustained for hundreds of millions of years because the overlying strata sequence was deposited rapidly in so short a time that the overburden pressures could not be sustained long enough to compact the quartz grains so that they fractured and/or were broken. Furthermore, the overlying strata sequence may never have been that thick.
However, it could be that the reason there are so few quartz grains with just subtle fractures and rare quartz grains with fractures or are broken is because of recrystallization and recovery. In those processes, any crystal lattice dislocations produced by ductile deformation are freed and migrate to form sub-grain boundaries (Hobbs, Means, and Williams 1976; Spry 1969). Thus, another claimed evidence for ductile deformation is the development of sub-grains within quartz grains (Groshong 1988; Vernon 2018; Wojtal, Blenkinsop, and Tikoff 2022). Yet such sub-grains are supposed to be relatively evenly spaced and show small optically misorientation angles, and such dispersion of dislocations in bending the grains should produce undulose extinction grading into the slightly misoriented sub-grain boundaries. However, as already noted, there are only a few quartz grains where there is an appearance of slightly undulose extinction (fig. 27). Also, only a few quartz grains in every sample in this study contain sub-grains, regardless of the location of the sample in the fold or distal to the fold (fig. 26). Yet there are no uniform shapes or sizes of those sub-grains, most being irregularly shaped and often vastly different in sizes within the same quartz grains. They are not significantly misoriented optically and the sharpness of the sub-grain boundaries varies between quartz grains. In most instances the sub-grains appear to have been features in the original quartz clasts because the dust and iron-oxides outlines of the quartz grains containing the sub-grains preserve their original detrital shapes (figs. 24 and 26), which suggests those quartz grains were eroded and transported from metamorphic source rocks. Overall, sub-grains within the few quartz grains in which they occur are trivial features, which suggests they are not related to the deformation of the sandstone beds, especially as they occur in all samples, whether in the Carbon Canyon fold or distant from it.
The SEM images overwhelmingly confirm that there has been no stress on the fabric of the sandstone after its compaction and lithification, apart from perhaps some slight further compaction due to the confining pressure of the overlying strata sequence. That has resulted in trivial fracturing with no displacements in a few samples, as seen in some SEM images (figs. 38–47) and in some petrographic photomicrographs (figs. 26 and 32). Nevertheless, the original detrital quartz and K-feldspar grains and muscovite flakes would have been initially compacted by the overburden pressure during the progressive deposition of the overlying strata, which would have reduced the sizes of the initial pore spaces as well as bending some muscovite flakes around the quartz and K-feldspar grains, fracturing some grains and flakes, and breaking some flakes. During subsequent dewatering and lithification, the silica in the pore water crystallized as quartz overgrowths to infill many residual pore spaces and cement the detrital grains together, the overgrowths often meeting at triple points (fig. 25). Once cemented, the rock fabric has not been subsequently disturbed, as the SEM images (figs. 38–47) emphatically show. This again implies that the deformation responsible for the Carbon Canyon fold must have occurred soon after deposition before cementation and lithification of the sandstone beds, so deformation had to be soft-sediment deformation rather than ductile deformation hundreds of millions of years after lithification. The SEM images (figs. 38–47) clearly show the localized growth of illite and illite-smectite that occurred during diagenesis due to alteration breakdown of K-feldspar grains.
It has already been determined above that the pressure-temperature conditions of ~0.3–0.4 kbar (~4,300–5,900 psi) and 110–130°C to which these Tapeats Sandstone beds were subjected were only in the diagenesis P-T field, well below even low-grade regional metamorphism and the necessary conditions for most ductile deformation, as discussed above. However, even during soft-sediment deformation it is postulated that both grain-boundary sliding and rotation of the detrital grains occurs (fig. 15a), yet there is no obvious definitive evidence of that process having occurred that is visible under either the petrographic or the scanning electron microscopes. Nevertheless, there is no preferred crystallographic orientation of the quartz grains since their extinction occurs at different angles (fig. 27), which would be expected from the random settling of quartz grains during their deposition. Furthermore, there doesn’t appear to be any overall direction of elongation of the quartz grains parallel to the bedding (fig. 23), which might be expected as evidence of grain-boundary sliding and rotation of the grains during compaction and subsequent soft-sediment deformation before cementation and lithification. Only locally in one or two samples under magnification might there appear to be some elongation of quartz grains parallel to the bedding (fig. 25k and n), but at the macroscopic scale there is none (fig. 22). Of course, the muscovite flakes are generally parallel and sub-parallel to the bedding, but that is a depositional feature due to the flatness of the flakes having caused such settling during deposition.
Thus, there is no definitive microscopic evidence of ductile deformation of the Tapeats Sandstone beds within the Carbon Canyon fold, either under the petrological microscope or the scanning electron microscope. However, the conventional published accounts of the Laramide orogeny and monocline folding (DeCelles, Lawton, and Mitra 1995; DeCelles and Coogan 2006; Huntoon 1993, 2003; Ismat and Mitra 2005; Karlstrom and Timmins 2012; Matthews 1978; Reches 1978a; Sanz et al. 2008; Tindall and Davis 1999) insist that the folding was due to ductile deformation, yet all the features they describe as the macroscopic evidence for ductile deformation to fold the strata have all been replicated in simulation experiments involving the compressional folding of dampened soft sediment layers (Friedman et al. 1976; Friedman, Hugman, and Handin 1980; Handin et al. 1976; Nabavi and Fossen 2021; Rettger 1935; Weinberg 1979). So, instead, all these simulation experiments have demonstrated are the macroscopic features produced by soft-sediment deformation, the very same features observed in the Tapeats Sandstone beds within the Carbon Canyon fold. Thus, it is to be expected that the microscopic evidence is consistent with the folding being due to soft-sediment deformation having occurred soon after deposition of the sandstone beds and before subsequent cementation and lithification.
The Dating of Tapeats Sandstone Deposition and the Laramide Orogeny
So how can these macroscopic and microscopic observations be reconciled with the conventional published accounts of the Laramide orogeny and monocline folding (DeCelles and Coogan 2006; DeCelles, Lawton, and Mitra 1995; Huntoon 1993, 2003; Ismat and Mitra 2005; Karlstrom and Timmins 2012; Matthews 1978; Reches 1978a; Sanz et al. 2008; Tindall and Davis 1999)? Put simply, it is not a matter of the tectonic processes involved with the subduction and underplating of the Farallon plate being responsible for the uplift of the Colorado Plateau, which are not in dispute (Austin et al. 1994; Dickinson and Snyder 1978; Huntoon 2003; Karlstrom and Timmins 2012), but rather the huge disagreement with respect to the timing. Since the macroscopic and microscopic evidence indicates that the monoclinal folding during plateau uplift was accompanied by soft-sediment deformation of the Tapeats Sandstone beds in the Carbon Canyon fold within the East Kaibab Monocline and not by the ductile deformation claimed by Huntoon (2003), Hill and Moshier (2009), and Tapp and Wolgemuth (2016), this implies that the uplift and folding must have occurred very soon after deposition of the whole regional strata sequence before cementation and lithification of those strata. Yet the conventional view is that there were ~450 million years between deposition of the Tapeats Sandstone at 507–508 Ma (Karlstrom et al. 2018, 2020) and the Laramide orogeny at ~35–70 Ma (Huntoon 2003; Karlstrom and Timmins 2012).
Thus, this huge discrepancy between the claimed vast ages for the deposition of the Tapeats Sandstone and the subsequent Laramide folding, and the macroscopic and microscopic evidence of rapid deposition of the whole strata sequence followed by soft-sediment deformation during the folding event all prior to cementation and lithification of the sandstone beds, needs to be reconciled. Snelling (2021) has already resolved this issue with respect to the dating of the Tapeats Sandstone at 507–508 Ma. The same resolution applies to the dating of the Laramide orogeny. Vardiman, Snelling, and Chaffin (2005) reported the technical details of six lines of evidence, including experimental confirmation, that during a past global catastrophe nuclear decay rates were likely grossly accelerated by potentially six orders of magnitude, such that ~600 or more million years’ worth of nuclear decay as measured today occurred within about a year, which they identified as the year-long biblical Flood cataclysm recorded in Genesis 6–9. On that basis, the deposition of the Tapeats Sandstone dates to only the first few weeks of the Flood year, only ~4,350 years ago. Critics have pointed to the enormous quantities of heat that apparently would be released by such accelerated nuclear decay (Wiens 2016), yet Vardiman, Snelling, and Chaffin (2005) had already anticipated this criticism and provided plausible possible explanations, including the experimental fact that the radiohalos (which only form below 150˚C) would have been annealed if such an enormous heat release had occurred (Laney and Laughlin 1981; Snelling 2005a).
However, Snelling (2021) went further to demonstrate the problems with the U-Pb radioisotope dating of the sandstone and of that dating method itself. Specifically, Karlstrom et al. (2018) obtained U-Pb ages for detrital zircons within the Tapeats Sandstone as “young” as only 407.2 million years old, and then did not explain how the supposedly 507–508 million years old Tapeats Sandstone can have included within it so many detrital zircons with U-Pb ages less than its supposed depositional age. Nor did they explain from where these “younger” detrital zircons within the Tapeats Sandstone originated. Indeed, how could even the 507–508 Ma detrital zircons be incorporated in the Tapeats Sandstone if the underlying rocks that were eroded to provide the sand grains, including the zircon grains, are older than 507–508 Ma? This question alone raises serious doubts as to the applicability and reliability of this technique for supposedly quantifying the apparent depositional ages of sedimentary rock units. Yet not only is their methodology questionable, so must be the U-Pb dating method they used if it produced such illogical ages. Snelling (2000, 2009) has already provided details of numerous problems with the U-Pb dating method that are well-documented in the scientific literature. Furthermore, Snelling (2017a) reviewed all the determinations of the U-Pb decay rates (half-lives) and demonstrated that these crucial parameters are not yet precisely known, while Snelling (2017b, 2018, 2019) highlighted in detail the problems of common Pb, U, and Pb mobility, and mass fractionation respectively that plague all efforts to obtain accurate U-Pb age determinations.
Thus, once the subjectively interpreted U-Pb dates for the deposition of the Tapeats Sandstone are demonstrated to be invalid, there is no valid scientific objection to assigning the deposition of the Tapeats Sandstone to the first few weeks of the Flood year, only ~4,350 years ago. Similarly, the dating of the Laramide orogeny and the accompanying monocline folding at ~35–70 Ma relies on the same and various other related radioisotope dating methods that are plagued by identical problems (Snelling 2000, 2009). However, debate continues as to when the Laramide orogeny and monocline folding is envisaged to have occurred. Whitmore and Garner (2008) maintain it would have been at the end of the Flood year and continued into the early post-Flood years as the catastrophic plate tectonics of the Flood year reached isostatic equilibrium, causing mountains to rise all over the globe rapidly. Others, like Clarey (2020), disagree, and place the Laramide within the year of the Flood. But regardless, the Laramide orogeny occurred relatively recently, about 4350 years ago.
The Timing of the Folding—Flood Deposition and Tectonics
Austin (1994) provided a detailed comprehensive description and account of the geological development of Grand Canyon strata in the context of the global Genesis Flood cataclysm and the canyon’s erosion in the Flood’s aftermath. In particular, he described the Tapeats Sandstone as being deposited by the Flood waters advancing eastwards onto the western edge of the North American portion of the pre-Flood supercontinent after the initiation of the Flood event with the breaking up of the fountains of the great deep (Genesis 7:11) and the triggering of catastrophic plate tectonics (Austin et al. 1994; Baumgardner 2003). However, before the Tapeats Sandstone was deposited there had to be a prolonged period (days or more) in which there was a significant amount of continental-scale erosion to bevel the Precambrian (pre-Flood) land surface to produce the Great Unconformity. In the Grand Canyon region this involved intensive catastrophic erosion to remove several thousand meters of Grand Canyon Supergroup strata (which appear to only have survived in several down-faulted blocks) and then to bevel the underlying metamorphic schists and granite plutons. Then after this period of destructive erosion, and subsequent to the localized deposition of the Sixtymile Formation, the Tapeats Sandstone represents the first widespread (continental-scale) deposit of the Tonto Group. Snelling (2021) provides more details of, and evidence for, the rapid deposition of the Tapeats Sandstone in the first few weeks of the global Flood cataclysm.
Austin (1994) also diagrammatically envisaged a fining upwards model for the time transgressive rapid deposition of the Tonto Group strata as the powerful westward back underflow of the advancing Flood waters at a water flow speed of >2 m/sec intensely scoured and catastrophically eroded all pre-Flood rocks to produce the Great Unconformity before sequentially depositing their load of sediments as horizontally segregated facies in the vertically stacked Tonto Group strata during the first weeks of the Flood year. Then followed the progressive rapid deposition of the overlying sedimentary strata sequence in the subsequent months as the Flood waters rose violently to sweep and deposit sediments rapidly in these layers, many of which can also be traced across the North American continent (Clarey 2020; Sloss 1963).
Baumgardner (2013, 2018a, b) has made considerable progress with numerical simulations of the catastrophic erosion of bedrock via cavitation to produce these sediments that were rapidly deposited on the continental plates as shallow waters moved rapidly around the surface of the rotating globe. His modeling posits that the dominant means for sediment transport during the Flood was by rapidly flowing turbulent water, and that water motion was driven by large-amplitude tsunamis that were generated along subduction zone segments as the subducting plate and overriding plate, in a cyclic manner, locked and then suddenly released and slipped rapidly past one another. His calculations show that with plausible parameter choices average erosion and sedimentation rates on the order of 9 m/day (0.38 m/hr) occurred with tsunami-driven pulses of turbulent water that transported the generated sediments vast distances across the continental plate surfaces, sufficient to deposit the Tapeats Sandstone within 3–10 days and most of the Paleozoic-Mesozoic strata during the initial 150-day rising and prevailing waters phase of the Flood (Genesis 7:18–24), thus accounting for some 70% of the Phanerozoic sediment layers that blanket the earth’s continental surfaces today.
In the catastrophic plate tectonics model for the cataclysmic Flood event (Austin et al. 1994; Baumgardner 2003), the plates moved the same as in conventional plate tectonics, but at rapid rates. In the case of the Farallon plate, as its subduction under the western edge of the North American flattened, it thickened the continental crust of western North America. Consequently, rapid isostatic equilibration began, resulting in the Laramide orogeny and the rise of the Colorado Plateau and the monocline folding in the Grand Canyon region and elsewhere in the Colorado Plateau.
The Tapeats Sandstone beds were deposited rapidly in the first few weeks of the year of the biblical global Flood cataclysm only ~4,350 years ago (Snelling 2021). In the subsequent months the overlying sedimentary strata were progressively deposited rapidly, their accumulating overburden pressures of ~0.3–0.4 kbar (~4,300–5,900 psi) compacting and dewatering the Tapeats Sandstone beds at a possible maximum burial depth of ~3,300–4,500 m (~10,825–14,750 ft) where the temperatures rose to ~110–130°C. Then late in the Flood year, or as that Flood year ended, the Laramide uplift of the Colorado Plateau occurred, helping to drain off the Flood waters from the North American continent, eroding away almost all the Mesozoic strata off the plateau in the Grand Canyon region. Thus, in the Grand Canyon region the Laramide uplift caused bending of the whole Paleozoic strata sequence in the East Kaibab Monocline as the reactivated Precambrian Butte Fault moved the underlying Precambrian basement, producing the Carbon Canyon fold in the Tapeats Sandstone. The Tapeats Sandstone beds had for much of the Flood year remained relatively damp and soft, even as they were increasingly compacted by the rapidly accumulating overlying strata. But because the compaction was so rapid, very few microscopic effects of it are observed in the sandstone. Then when the Laramide folding occurred the Tapeats Sandstone beds were bent in the Carbon Canyon fold by soft-sediment deformation, consistent with both the observed macroscopic and microscopic features in the sandstone. Only subsequently did the sand in the Tapeats Sandstone beds fully dry and become cemented and lithified, again consistent with both the observed macroscopic and microscopic features in the sandstone, those processes being accelerated in the following years by the carving of Grand Canyon and its side canyons (Austin 1994; Austin, Holroyd, and McQueen 2020) that exposed the Tapeats Sandstone and the Carbon Canyon fold. Finally, ongoing micro-earthquakes still occurring in the Grand Canyon region (Karlstrom and Timmons 2012) indicate that imperceptible earth movements are still happening today that might induce trivial fracturing in some affected rock layers
Summary and Conclusions
The Cambrian Tapeats Sandstone beds are bent in the Carbon Canyon fold where they have been dragged up against the Butte Fault along the East Kaibab Monocline exposed in Carbon Canyon, a side canyon in the eastern Grand Canyon. This occurred during the Laramide orogeny at ~35–70 Ma when the Colorado Plateau including in the Grand Canyon region was uplifted. However, the Tapeats Sandstone had been deposited at 507–508 Ma, so after ~450 million years it should have been fully cemented and lithified. Thus, when its sandstone beds were bent in the Carbon Canyon fold, they should have suffered ductile deformation via bedding plane or flexural slip and grain-boundary sliding. And in the hinge zones particularly the lithified sandstone should have fractured. However, even during a superficial inspection of this fold it is evident that there is no significant fracturing of the sandstone in the hinge zones, and even fewer fractures than along the limbs of the fold. Thus, the sandstone beds look as though they were bent smoothly, perhaps while they were still unlithified and soft. Yet such a conclusion is preposterous if there were ~450 million years between deposition and lithification of the Tapeats Sandstone and its subsequent deformation to form the Carbon Canyon fold.
To date there had not been a detailed investigation of the Carbon Canyon fold to examine the bent sandstone beds, especially their microscopic features, to determine if their folding was due to ductile deformation (as conventionally claimed) or due to soft-sediment deformation. Thus 12 samples of the Tapeats Sandstone were collected from the Carbon Canyon fold, from hinge zones and from various distances along the limb zones, as well as four samples from approximately the same stratigraphic position in the Tapeats Sandstone at various distances of miles from the fold. This strategy was adopted so that the samples from the fold could be compared with the distal samples acting as a “control” to ascertain any differences between the folded and unfolded (“background”) sandstone beds.
An initial study detailed all previous investigations of the Tapeats Sandstone. From petrographic examination of 26 Tapeats Sandstone samples it was concluded that the poorly to moderately well-sorted, sub-angular to sub-rounded quartz and K-feldspar grains, and muscovite flakes comprising the sandstone were still in their detrital condition with no indications of the silica cement having been disturbed since lithification of the sandstone or of any metamorphic changes to these constituent minerals or the rock fabric. These observations, as well as the sedimentary structures such as cross-beds and the body fossils and fossil traces preserved in the sandstone, were deemed consistent with rapid deposition of the Tapeats Sandstone.
For this study the macroscopic and microscopic features that should or could be present if the Tapeats Sandstone beds in the Carbon Canyon fold had been bent via ductile deformation were set out. For example, at the macroscopic scale bedding plane or flexural slip should have produced slickensides on bedding plane surfaces and there should be thickening of hinge zones in the fold and thinning of limb zones, as well as more fracturing in the hinge zones compared to the limbs. Field observations had been obtained to test these expectations. At the microscopic scale there should minimally be evidence of grain-boundary sliding, rotation of grains, and fracturing of grains, and within many quartz grains there should be sub-grains, undulose extinction, deformation lamellae, and even deformation kink bands. Both petrographic observations were made and scanning electron microscope (SEM) images obtained, as well as some cathodoluminescence (CL) images and even fission tracks observed, to ascertain whether these microscopic features are present in the sandstone, especially also comparing the samples from the hinge and limb zones in the fold with the distal samples.
The field observations of the sandstone beds in the fold were mostly inconsistent with ductile deformation. While bedding plane or flexural slip must have occurred, slickensides were only found on one bedding plane surface, there was only trivial thickening of one bed in one hinge zone, and fracturing was more prevalent in the limbs than in the hinge zones. Yet all these and other features have been replicated using damp soft sediment layers in experiments simulating compressional folding, which equates to soft-sediment deformation. On the other hand, none of the microscopic features expected from ductile deformation were present in any of the samples, and the samples from the hinge and limb zones of the fold were essentially identical to the distal samples. There are no deformation lamellae or deformation kink bands in the quartz grains which rarely displayed even trivial undulose extinction, and there is no obvious evidence of any rotation of grains or grain-boundary sliding. The few quartz grains containing sub-grains are instead likely derived from the metamorphic source rocks rather than being a product of ductile deformation, and the few subtle fractures in rare quartz grains are consistent with trivial fracturing due to compaction of the sand grains under the confining overburden pressures. Furthermore, the SEM images clearly demonstrate that the silica (quartz) cement binding the sand grains has not been disrupted since lithification, with many quartz cement crystals still being pristine with terminal faces intact. Thus, both the macroscopic and microscopic evidence are conclusively consistent only with soft-sediment deformation before cementation and lithification.
Therefore, since the bending of the Tapeats Sandstone beds in the Carbon Canyon fold must be due to soft-sediment deformation, the ~450 million years between deposition of the sandstone and the Laramide uplift responsible for the folding must be in error and are thus eliminated. Instead, the Tapeats Sandstone had to be folded while still relatively damp and soft soon after deposition and before cementation and lithification. The problems with the radioisotope dating methods and the U-Pb dates obtained for the Tapeats Sandstone rule out the vast claimed ages. This scenario can all be easily reconciled with rapid deposition of the Tapeats Sandstone during the first few days to weeks of the biblical global Flood cataclysm only ~4,350 years ago and rapid deposition of ~3,300–4,500 m (~10,825–14,750 ft) of overlying sedimentary layers during the catastrophic plate tectonics of the Flood year. Then near or at the end of Flood year the Farallon plate underplated the western North American plate, causing isostatic reequilibration which resulted in the Laramide uplift of the Colorado Plateau and the monocline folding in the Grand Canyon region now exposed in the Carbon Canyon fold. Because the Tapeats Sandstone beds were still relatively damp and soft after less than a year of rapid burial, they easily responded to the soft-sediment deformation to form the smooth bending (without brittle fracturing) in the Carbon Canyon fold before the beds dried, and were cemented and lithified to sandstone. Altogether, more than 500 million years of claimed geologic history are thus eliminated.
All samples were collected under the authority of National Park Service Scientific Research and Sampling Permit #GRCA-2017-SCI-0052 dated June 23, 2017, issued by the Grand Canyon National Park’s Research Office. The Alliance Defending Freedom (ADF) team led by then Senior Counsel Gary McCaleb is especially thanked for their legal work that led to a successful lawsuit against viewpoint discrimination in the permit application and granting process. Tom Vail, founder of Canyon Ministries who encouraged this research from its start, is also thanked for organizing with Terry Vallely, and assisted by their wives Paula and Kathy, respectively, the August 6–12, 2017, research raft trip down the Colorado River through Grand Canyon to collect the samples, facilitated by Grand Canyon National Park Special Use Permit #GRCA-3701 issued June 26, 2017. Special thanks go to Tom Vail and Dr. John H. Whitmore, Senior Professor of Geology at Cedarville University, Ohio for their invaluable field assistance, without which the samples would not have been collected, especially after I was injured early in the trip. Ray Strom of Calgary Rock and Materials Services, Inc. is thanked for the thin sections he prepared, and for the XRD and SEM analyses, as well as for the use of his research microscope for photography. Cedarville University is also thanked for use of their geologic research microscope and Dr. John H. Whitmore for his advice, support, and encouragement. The helpful comments and edits from three kind reviewers were much appreciated. This research was fully funded by many generous donors to Answers in Genesis and has had the full support of the Answers in Genesis leadership team under Ken Ham. Our production assistant Laurel Hemmings is also thanked for her work in preparing this paper for publication. Nevertheless, I take full responsibility for the content of this paper.
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Appendix—Location and Petrographic Descriptions of Tapeats Sandstone Samples