See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/285114634 Devonian carbonate platform of eastern Nevada: Facies, surfaces, cycles, sequences, reefs, and cataclysmic Alamo Impact Breccia Chapter · January 2008 DOI: 10.1130/2008.fld011(10) CITATIONS READS 8 1,175 3 authors, including: John Warme Charles Sandberg Colorado School of Mines United States Geological Survey 64 PUBLICATIONS 1,308 CITATIONS 146 PUBLICATIONS 5,719 CITATIONS SEE PROFILE Some of the authors of this publication are also working on these related projects: Radiolarians View project Paleogeographic reconstructions View project All content following this page was uploaded by John Warme on 28 June 2018. The user has requested enhancement of the downloaded file. SEE PROFILE The Geological Society of America Field Guide 11 2008 Devonian carbonate platform of eastern Nevada: Facies, surfaces, cycles, sequences, reefs, and cataclysmic Alamo Impact Breccia John E. Warme* Department of Geology and Geological Engineering, Colorado School of Mines, Golden, Colorado 80401, USA Jared R. Morrow* Department of Geological Sciences, San Diego State University, San Diego, California 92182, USA Charles A. Sandberg* U.S. Geological Survey, Box 25046, MS 939, Federal Center, Denver, Colorado 80225, USA ABSTRACT Devonian limestone and dolostone formations are superbly exposed in numerous mountain ranges of southeastern Nevada. The Devonian is as thick as 1500 m there and reveals continuous exposures of a classic, long-lived, shallow-water carbonate platform. This field guide provides excursions to Devonian outcrops easily reached from the settlement of Alamo, Nevada, ~100 mi (~160 km) north of Las Vegas. Emphasis is on carbonate-platform lithostratigraphy, but includes overviews of the conodont biochronology that is crucial for regional and global correlations. Field stops include traverses in several local ranges to study these formations and some of their equivalents, in ascending order: Lower Devonian Sevy Dolostone and cherty argillaceous unit, Lower and Middle Devonian Oxyoke Canyon Sandstone, Middle Devonian Simonson Dolostone and Fox Mountain Formation, Middle and Upper Devonian Guilmette Formation, and Upper Devonian West Range Limestone. Together, these formations are mainly composed of hundreds of partial to complete shallowing-upward Milankovitch-scale cycles and are grouped into sequences bounded by regionally significant surfaces. Dolomitization in the Sevy and Simonson appears to be linked to exposure surfaces and related underlying karst intervals. The less-altered Guilmette exhibits characteristic shallowing-upward limestone-to-dolostone cycles that contain typical carbonate-platform fossil- and ichnofossil-assemblages, displays stacked biostromes and bioherms of flourishing stromatoporoids and sparse corals, and is punctuated by channeled quartzose sandstones. The Guilmette also contains a completely exposed ~50-m-thick buildup that is constructed mainly of stromatoporoids, with an exposed and karstified crest. This buildup exemplifies such Devonian structures known from surface and hydrocarbon-bearing subsurface locations worldwide. Of special interest is the stratigraphically anomalous Alamo Breccia that represents the middle member of the Guilmette. This spectacular cataclysmic megabreccia, produced by the Alamo *jwarme@mines.edu; jmorrow@sciences.sdsu.edu; sandberg@usgs.gov Warme, J.E., Morrow, J.R., and Sandberg, C.A., 2008, Devonian carbonate platform of eastern Nevada: Facies, surfaces, cycles, sequences, reefs, and cataclysmic Alamo Impact Breccia, in Duebendorfer, E.M., and Smith, E.I., eds., Field Guide to Plutons, Volcanoes, Faults, Reefs, Dinosaurs, and Possible Glaciation in Selected Areas of Arizona, California, and Nevada: Geological Society of America Field Guide 11, p. 215–247, doi: 10.1130/2008.fld011(10). For permission to copy, contact editing@geosociety.org. ©2008 The Geological Society of America. All rights reserved. 215 216 Warme et al. Impact Event, is as thick as 100 m and may be the best exposed proven bolide impact breccia on Earth. It contains widespread intervals generated by the seismic shock, ejecta curtain, tsunami surge, and runoff generated by a major marine impact. Newly interpreted crater-rim impact stratigraphy at Tempiute Mountain contains an even thicker stack of impact breccias that are interpreted as parautochthonous, injected, fallback, partial melt, resurge, and possibly post-Event crater fill. Keywords: carbonate platform, cyclostratigraphy, sequence stratigraphy, Devonian, Alamo Breccia, impact deposits. INTRODUCTION Purpose and Objectives The main purpose of this guide is to present, in outcrop examples, many of the common characteristics of shallow-water carbonate-platform stratigraphic successions. Each stop exhibits carbonate rocks that are typical of the Devonian platform facies of southeastern Nevada and, except for the platform biota that changes through time, are similar in structure to many carbonate platforms that occur elsewhere throughout Phanerozoic and even Proterozoic time. In addition, each stop presents objectives of special stratigraphic interest that sets them apart, such as distinctive cyclic stacking patterns, exposure surfaces, karst intervals, organic buildups, sandstone interbeds, and evidence for cataclysm via the Alamo Breccia. We intend that enough time be dedicated at each stop to promote observations, descriptions, discussions, interpretations, and possibly debates about the rocks. Each stop has been the subject of one or more published papers, or reported in theses, but our approach will be, as much as possible, to examine the formations as a group of unbiased observers and interpreters and interpret the rock properties and their significances. BACKGROUND INFORMATION The following brief overviews are presented for the benefit of participants unfamiliar with the field trip area and its geographic and geologic setting. Much of this information was compiled by Jared Morrow and presented in an unpublished field trip guidebook for participants of the September 2007 meeting of the Subcommission on Devonian Stratigraphy (SDS) of the International Union of Geological Sciences (IUGS). Additional data are excerpted from Morrow and Sandberg (2008). Geographic Setting The field trip area lies within a southern portion of the Great Basin (Fig. 1), which is a large part of the Basin and Range physiographic province of western North America. This vast province is characterized by hundreds of named, north-south–trending mountain ranges separated by alluvium-filled, mainly Tertiary basins. The ranges commonly exhibit tilted and well-exposed Paleozoic stratigraphic sections, as shown in Figure 2, which facilitate study and can be correlated between ranges. The Great Basin portion includes almost all of Nevada and parts of eastern California and Oregon, southern Idaho, and western Utah. As the name implies, the “Great Basin” is hydrologically defined as the region where streams drain into enclosed basins with no outlets to major rivers, such as the Columbia River system to the north and the Colorado River system to the southeast. Great Basin elevations range from ~600 m in deserts of the southern valleys to 4006 m at the summit of Boundary Peak, the highest point in Nevada. Geologic Overview The oldest rocks in the Great Basin region are Paleoproterozoic, 1.74 Ga metamorphic and intrusive igneous units exposed in southern Nevada. In the east-west corridor from western Utah to central Nevada, this crystalline basement is covered by a westward-thickening prism of Neoproterozoic to Middle Devonian, supratidal to deep-subtidal siliciclastic and carbonate sedimentary rocks that were deposited along the subsiding passive craton margin of what is now western North America (Stewart, 1980). The sedimentary prism reaches a thickness of nearly 9000 m in central Nevada, with Devonian strata making up more than 1800 m of this total (Fig. 3). Regional to global correlation of Devonian rocks, sequences, and events is facilitated by conodont biostratigraphy (Fig. 4), which provides the highest resolution biochronology for this time interval. Figure 5 shows the Middle Devonian to Lower Mississippian formations that occur in the southeastern Nevada area of this field guide. They represent sediment accumulation in the eastern and central longitudinal bands of the north-south sedimentary prism. The carbonate-dominated formations represent episodes of a long-lived, shallow-water, carbonate platform that existed until the Late Devonian to Early Mississippian Antler orogeny. Figures 6 and 7 show the relationships between eustasy and Devonian formations that accumulated along the continental margin, including those that are the subject of this Chapter. Figure 7 shows that guidebook stops in the Sevy, Simonson, Fox Mountain, and Guilmette formations (Stops 1–5) lie relatively landward on the platform, whereas the cherty argillaceous unit and Sentinel Mountain, Bay State, and Devils Gate formations (Stop 6) lie more seaward. As outlined below, however, Devonian and later tectonic disturbances, first mainly compressive and later mainly extensional, severely fragmented the platform so that paleogeographic reconstructions are difficult and still ongoing. Devonian carbonate platform of eastern Nevada 0 217 100 km Owyhee Upland Elko Reno Eureka Salt Lake City Ely S ie rr a N ev ad Alamo a Las Vegas l Co or a do R. Figure 1. Lambert projection digital elevation model shaded-relief image of central Basin and Range province, showing hydrologic boundary of the Great Basin region (dashed white line), outline of Nevada (solid white line), location of selected Nevada cities and towns, and area of field trip route shown in Figure 10 (black box). North is toward top of image. Modified from http://able1.mines.unr.edu. Dg u Dg l Dg ys f Df m Dg ab Figure 2. View, looking north, of ~700 m of Middle and Upper Devonian formations exposed on a fault block in the West Pahranagat Range. Rocks of this section are almost identical to those exposed on the traverse of Stop 1, along “Downdropped Mountain,” 1 mi (1.6 km) to the west. Devonian carbonate-platform rocks include the Givetian Fox Mountain Formation (Dfm), the Givetian yellow slope-forming member of the Guilmette Formation (Dgysf), the Givetian to Frasnian lower member of the Guilmette Formation (Dgl), the mid-Frasnian Alamo Breccia Member of the Guilmette Formation (Dgab), and the Frasnian to lower Famennian upper member of the Guilmette Formation (Dgu). The Guilmette here contains 70 documented platform carbonate cycles, which are mixed with quartzose sandstone facies in the upper member (Estes-Jackson, 1996). 218 Warme et al. Figure 3. Palinspastic map of Great Basin region with isopachs (thickness in thousands of feet) and depositional provinces of Devonian rocks. Position of Lincoln County (L.C.), Nevada, is marked. Modified from Stewart and Poole (1974). Beginning in the Middle Devonian and accelerating in the Late Devonian, the effects of eastward-verging tectonic compression crossed the region. Several orogenic episodes were driven by this compression. Most evident are the Antler orogeny (Late Devonian–Mississippian, focused along the Roberts Mountains thrust; Fig. 8), and the Sonoma orogeny (Late Permian–Early Triassic). During the Devonian to Triassic interval, western North America was fringed by a developing subduction zone system. As shown partially in Figures 6 and 7, from east to west across the Great Basin the sedimentary and tectonic provinces at this time included: (1) a shallow-marine, carbonate-dominated platform; (2) a backbulge basin (e.g., the Late Devonian–Early Mississippian Pilot basin); (3) an eastward-migrating forebulge; (4) a foreland basin, which received detrital sediments from both the east and the west; (5) an emergent allochthon; (6) a western, deep-marine basin dominated by hemipelagic sedimentation and mafic volcanism; and (7), at the longitude of present-day western Nevada and eastern California, a volcanic arc terrane. Mesozoic sedimentary rocks in the Great Basin are largely of Triassic and Early Jurassic ages, but are not exposed in this field guide area. Cretaceous sedimentary rocks are represented by continental deposits in localized tectonic basins (e.g., the Newark Canyon Formation). By the mid-Jurassic, extensive tectonic compression again spread from west to east across Nevada, culminating in the Cretaceous to early Cenozoic Sevier orogenic belt of easternmost Nevada and western Utah (Fig. 8). During the middle Cenozoic, from ~34 Ma to ~17 Ma, the region was dominated by siliceous volcanism, evidenced by widespread ash-flow tuffs and rhyolites that are preserved on most of the ranges in the field trip area. From ~17 Ma to the present, major extensional tectonism, crustal thinning, normal faulting, and mafic volcanism characterized the region, resulting in the modern basin and range topography and basaltic flows that can be young enough to follow present drainages. In the Pleistocene, from ~30,000 yr B.P. to ~10,000 yr B.P., large areas of many basins were covered by extensive pluvial lake systems, including Lake Lahontan in western Nevada and Lake Bonneville in western Utah (Stewart, 1980; Hintze, 1988). Wave-cut terraces and fine-grained lacustrine deposits are a common feature in these basins, especially north of the field trip area covered in this guide. Also during the Pleistocene, isolated alpine glaciers formed on the highest peaks of the central Great Basin. Figure 4. Devonian conodont biochronology, scaled to numerical ages of Kaufmann (2006). Correlation of zonation with German Stufen is shown for Late Devonian; Substages are those proposed by Sandberg and Ziegler (1998). Subdivisions of Early rhenana and linguiformis Zones are shown. E—Early; L—Late; semi—semichatovae Subzone interval; MISS.—Mississippian. Scaling of Famennian biozones to numerical ages is approximate and provisional. Modified from Sandberg et al. (2002), Girard et al. (2005), Kaufmann (2006), and C.A. Sandberg (unpublished). Figure 5. Time-rock chart of Middle Devonian (Eifelian) to Lower Mississippian (Osagean) stratigraphic units exposed at Alamo Canyon (ALA), and at Bactrian Mountain (BCT and BME) and Silver Canyon, Mount Irish Range (MIR, Stop 3), east and north of Alamo, Nevada. Numerical ages are from Kaufmann (2006). Time values of Alamo Breccia Member, Leatham Member, and Mount Irish buildup are exaggerated for graphic purposes. See Sandberg et al. (1997) for Nevada Events. Modified from Sandberg et al. (1997). Devonian carbonate platform of eastern Nevada 219 220 Warme et al. Figure 6. Devonian sea-level curve, showing relative paleotectonic and geographic settings of principal stratigraphic units of the western United States. Roman numerals indicate transgressive-regressive (T-R) cycles of Johnson et al. (1985). F.I.—brachiopod- and conodont-based faunal intervals of Johnson et al. (1980); T.S.—transgressive starts in the western United States; C.Z.—conodont Zones. Kobeh, Bartine, and Coils Creek are members of McColley Canyon Formation. From Johnson and Sandberg (1989). Devonian carbonate platform of eastern Nevada SW IIf NE Continental slope Carbonate platform Leatham Mbr. Pilot Shale Barite & phosphatic black chert IIc Ib Ia TorMcMon. Ls. pre-Ia lge Woodruff tongue Lower mbr. Devils Gate Ls. Guilmette Fm. Rabbit Hill Ls. Bastille Ls. Coils Crk. Mbr. Kobeh Mbr. Fox Mountain Fm. Upper mbr. Lower mbr. uam Woodpecker Ls. bcm Sentinel Mtn. Dol. lam Oxyoke Cnyn. Ss. cxm Sadler Ranch Fm. m tfor Pla argin m Simonson Dol. Bay State Dolostone Pl m atfo ar rm gin Bartine Mbr. Windmill Ls. cau Beacon Peak Dol. Lone Mountain Dol. (pt.) m tfor Pla rgin ma Roberts Mtns. Fm. (pt.) YSF Sevy Dol. Ic Denay Limestone Id Upper mbr. Devils Gate Ls. L.-m. tongue Fenstermaker Wash Fm. FB (Locally present) Ie Lower mbr. Pilot Shale Red Hill beds Unnamed Lower & Middle Devonian units If C h e r t IIa Lower tongue Woodruff Fm. Alamo Event S l a v e n IIb U. t. Fenstermaker Wash Fm. ebu IId Upper tongue Woodruff Fm. For Woodruff Fm. IIe (U. Devonian only) Forebulge & foreland uplift McColley Canyon Fm. Pragian Emsian Eifelian Givetian Frasnian Famennian Stage Lochkovian Lower Devonian Middle Devonian Upper Devonian Series T-R Cycle Toe 221 Figure 7. Northeast-to-southwest, Devonian time-rock transect across central and eastern Nevada, showing carbonate-platform, continental slope, and toe of slope stratigraphic units and relative lateral shifts in platform margin through time. Transgressive-regressive (T-R) cycles Ia through IIf (Johnson et al., 1985, 1991; Johnson and Sandberg, 1989), main intervals of turbidity current and debris-flow deposition (arrows), proto-Antler forebulge initiation (FB), and timing of Alamo Impact Event are indicated. Silty dolostone and siltstone of the yellow slope-forming member (YSF), which forms the basal unit of the Guilmette Formation and Devils Gate Limestone, is a widespread marker lithology distributed throughout western North America (Sandberg et al., 1989, 1997, 2002). The YSF is correlated with fish-bearing Red Hill beds in north-central Nevada. Four members of Simonson Dolostone are: cxm—coarse crystalline member; lam—lower alternating member; bcm—brown cliff member; and uam—upper alternating member. Other abbreviations: cau—cherty argillaceous unit; Cnyn.—Canyon; Crk.—Creek; Dol.—Dolostone; Fm.— Formation; L.—Lower; Ls.—Limestone; m.—middle; mbr.—member; McMon.—McMonnigal; Mtns.—Mountains; pt.—part; Ss.—Sandstone; t.—tongue; U.—Upper. From Morrow and Sandberg (2008) and based on data from Johnson and Sandberg (1977), Johnson and Murphy (1984), Sandberg et al. (1989, 1997, 2002, 2003), Johnson et al. (1996), and M.A. Murphy (14 September 2007, personal commun.). 222 Warme et al. Figure 8. Index map of Great Basin region showing major thrust and strike-slip faults. Sevier thrust system, of Cretaceous to early Cenozoic age, includes individual parts consisting of Nopah, Wheeler Pass, Keystone, Gass Peak, Wah Wah, Muddy Mountains, Blue Mountain, Nebo, Charleston, Willard, and Paris faults. From Stewart (1980). Devonian carbonate platform of eastern Nevada DEVONIAN GEOLOGIC SUMMARY Rocks studied on this field trip represent part of the ~57m.y.-long Devonian geological history of the eastern and central parts of the extensive carbonate platform that extended north-tosouth through Nevada and Utah (Figs. 6, 7). The stops in this guide represent only the central latitudinal segment of a much longer Devonian platform and platform-margin complex that fringed western North America from Alaska and Arctic Canada to Mexico (Ziegler, 1989; Poole et al., 1992). Devonian platformto-basin rocks in western Utah and Nevada record the complex transition from long-term extensional to compressional tectonic modes of the Antler orogeny, which was the first in a series of late Paleozoic to Mesozoic orogenic belts that developed over the subduction zone fringing the western continental margin of North America. In the middle- to outer-platform settings, Devonian strata reach a thickness of over 1800 m (Fig. 3). During the mid-1970s to early 1990s, a series of landmark papers provided detailed stratigraphic, biostratigraphic, lithofacies, isopach, structural, and coastal onlap data on the Devonian continental margin in the western United States, including the eustatic sea-level curve of Figure 6 and multiple paleogeographic and paleotectonic time-slice maps constrained by highresolution conodont biochronology. These important papers include, among others: Poole (1974), Stewart and Poole (1974), Johnson and Sandberg (1977, 1989), Matti and McKee (1977), Murphy (1977), Poole et al. (1977, 1992), Sandberg and Poole (1977), Johnson and Pendergast (1981), Gutschick and Sandberg (1983), Kendall et al. (1983), Johnson and Murphy (1984), Murphy et al. (1984), Johnson et al. (1985, 1986, 1989, 1991), Stevens (1986), Sandberg et al. (1988, 1989), Goebel (1991), Johnson and Bird (1991), D.M. Miller et al. (1991), and E.L. Miller et al. (1992). More recent studies of the Devonian platform and platformto-basin transition in Utah and Nevada have focused on refining aspects of: (1) tectonic and structural history (e.g., Oldow et al., 1989; Giles, 1994; Giles and Dickinson, 1995; Crafford and Grauch, 2002; Grauch et al., 2003; Sandberg et al., 2003); (2) depositional models and facies geometry (e.g., Elrick, 1995, 1996; LaMaskin and Elrick, 1997; Cook and Corboy, 2004); (3) conodont-based event stratigraphy and eustasy (e.g., Johnson et al., 1996; Sandberg et al., 2002, 2003; Morrow and Sandberg, 2003, 2008); (4) stratigraphic and structural development in relation to synsedimentary exhalative gold mineralization in the Carlin gold trend, northern Nevada (e.g., Emsbo et al., 1999, 2006; Hofstra and Cline, 2000; Crafford and Grauch, 2002); and (5) relation to the early Late Devonian Alamo Impact Event, south-central Nevada (e.g., Warme and Sandberg, 1995, 1996; Sandberg et al., 1997, 2002, 2003, 2005, 2006; Warme and Kuehner, 1998; Warme, 2004; Morrow and Sandberg, 2005, 2006; Morrow et al., 2005; Pinto, 2006; Warme and Pinto, 2006; Pinto and Warme, 2008). Warme and Pinto (2006) and Pinto and Warme (2008) presented a genetic classification for different facies of the Alamo 223 Breccia, placing known positions of the Breccia into impact “Realms” with respect to the target zone. As shown in Figure 9, Stops 1–5 in this chapter fall in the Ring Realm, and Stop 6 represents the only known locality in the Rim Realm, closest to the as yet unidentified central target zone. The other realms are outside the area of this chapter, but have been described and interpreted in references cited for the Alamo Impact Event. Sedimentation Patterns In western Utah and Nevada, the position of the Devonian carbonate platform and the sedimentary facies deposited in platform-to-basin settings were influenced by both eustasy and tectonics. Since the early comprehensive work of Roberts et al. (1958), Paleozoic sedimentary strata in western Utah and east-central Nevada have been generally regarded to document, from eastto-west, shallow-to-deep marine carbonate-platform, platformmargin, slope, and basin depositional settings (Figs. 5 and 7). In general, Devonian platform deposits are dominated by supratidal, intertidal, and shallow-subtidal carbonate rocks such as biolaminated dolostone, bioturbated lime mudstone and wackestone, bioclastic wackestone and packstone, stromatoporoid-dominated lime mud-rich biostromes, and intraformational conglomerate (Elrick, 1996; Poole et al., 1992; Cook et al., 1983; Cook and Corboy, 2004). During eustatic lowstands, craton-derived quartz sand was deposited in channels and basinward-prograding clastic wedges across large areas of the platform (Fig. 5). Devonian outer-platform to platform-margin rocks consist of shallow- to deep-subtidal, bioturbated, bioclastic wackestone, packstone, and grainstone. During parts of the Early and Middle Devonian when a rimmed platform margin developed (Elrick, 1996; Cook and Corboy, 2004), deposits included coral- and crinoid-dominated biostromes, bioherms, and mudmounds. Slope and basin areas accumulated bioclastic and sandy packstones and grainstones deposited within submarine debris-flow and turbidite-fan systems, intraformational slumps with flat-clast conglomerates, and rhythmically deposited argillaceous carbonate and fine- to medium-grained siliciclastic units. The most distal deposits include rhythmically bedded radiolarian chert, very fine- to fine-grained siliciclastic units, and minor greenstones. The Early and Middle Devonian carbonate platform-to-basin transition, which can be in part characterized using classic carbonate platform models (e.g., Wilson, 1975; Read, 1982), was characterized by several morphologies including homoclinal ramps, distally steepened ramps, rimmed platform margins with intra-shelf basins, and rimmed platform-margins flanked by landward shallow-subtidal platforms and seaward slope-aprons (Cook et al., 1983; Kendall et al., 1983; Johnson and Murphy, 1984; Schalla and Benedetto, 1991; Elrick, 1996; Cook and Corboy, 2004). As discussed next, however, throughout the latter half of the Devonian, proto-Antler and Antler tectonism exerted a strong to dominant control on the position and geometry of the carbonate-platform marginto-basin settings. 224 Warme et al. 6 3 2 4 1 Figure 9. Alamo Breccia locality map showing genetic Breccia Realms, Nevada and western Utah. Lateral Breccia Zones 1, 2, and 3 of earlier publications (e.g., Warme and Sandberg, 1995, 1996; Warme and Kuehner, 1998) are now equated with the Rim, Ring, and Runup Realms (Warme and Pinto, 2006; Pinto and Warme, 2008), respectively. Black diamonds, offshore, deep-water Alamo channel localities; white circles, localities at Tempiute Mountain interpreted to be on or within the Alamo crater rim; open triangles, carbonate-platform localities with well-developed Alamo Breccia including potentially all Units A–D; black circles, carbonate-platform localities with thin Alamo Breccia; black triangle, locality with seismically disturbed zone stratigraphically equivalent to Alamo Breccia; white diamonds, distal, middle- to inner-platform Alamo channel deposits; black arrows, paleocurrent directions determined from clast imbrication; black squares, selected towns. Field trip Stops 1–6 are indicated by numbers. Modified from Pinto and Warme (2008). 5 Tectonic Models Neoproterozoic to early Paleozoic time was marked by a complex pattern of tectonic extension and rifting along western North America as the proto-Pacific basin opened following the breakup of Rodinia at ~850–650 Ma (Stewart, 1972; Stewart and Suczek, 1977; Poole et al., 1992). Outer-platform and platformmargin basins, which probably formed by reactivation of structures inherited from Mesoproterozoic to Neoproterozoic rifting of underlying crystalline continental basement (Stewart, 1972; Stewart and Poole, 1974), strongly influenced sedimentation patterns in Nevada during the Middle Cambrian to Middle Devonian (Johnson and Potter, 1975; Matti and McKee, 1977; Johnson and Murphy, 1984; Miller et al., 1991; Poole et al., 1992). For the Early and Middle Devonian interval especially, the distribution of facies patterns, rock isopachs, strontium and lead isotope isopleths, basement gravity signatures, and synsedimentary exhalative gold and barite deposits all suggest that the platform margin was characterized by a complex series of restricted, active, fault-bounded sub-basins, which determined the type, extent, and thickness of sedimentary units (Grauch, 1998; Emsbo et al., 1999, 2006; Hofstra and Cline, 2000; Crafford and Grauch, 2002; Grauch et al., 2003; Emsbo and Morrow, 2005; Morrow and Sandberg, 2008). By the Ordovician (Ross, 1977) or Silurian (Poole et al., 1977), a volcanic island-arc system developed over subducted oceanic crust west of the North American continent. Localized extensional or transtensional tectonics within a postulated inner-arc basin located between the volcanic arc and the continent may have further promoted the formation of fault-bounded platform-margin sub-basins prior to late Middle to early Late Devonian compression and transpression associated with the approaching Antler orogen (Poole et al., 1977; Eisbacher, 1983; Crafford and Grauch, 2002). Devonian carbonate platform of eastern Nevada Unraveling of the complicated Devonian tectonic processes and sedimentary responses in the Great Basin area has been facilitated by use of conodont biostratigraphy (e.g., Figs. 4, 6, and 7). The earliest direct stratigraphic evidence for the switch to a convergent tectonic mode is in central Nevada, where uplift and erosion was associated with development of the initial, shallow-marine to emergent, proto-Antler forebulge during the latest Givetian to early Frasnian disparilis, falsiovalis, and transitans conodont Zones (Figs. 6 and 7; Sandberg et al., 2003). Subsequent Late Devonian depositional settings and facies patterns on the outer platform and platform margin were dominated by tectonic effects of the converging Antler orogenic belt, which formed an eastward-migrating system composed, from west to east, of an allochthon, a foreland basin, a forebulge, and a backbulge (Pilot) basin that developed across the carbonate-dominated platform to the east (Poole and Sandberg, 1977; Goebel, 1991; Giles, 1994; Giles and Dickinson, 1995). By the late middle Famennian Early postera Zone (Fig. 6), the carbonate platform environment was terminated by widespread uplift driven by the continued eastward migration and expansion of the Antler orogen. Erosion off the leading forebulge formed a regional unconformity that interrupted or removed the latest Famennian depositional record of the platform (Sandberg et al., 1989, 2003; Poole and Sandberg, 1991). The magnitude of this extensive unconformity was amplified by a major eustatic sea-level fall that began during the late Famennian Middle praesulcata Zone and persisted into the Early Mississippian (Sandberg et al., 1989; 2002). At the site of the former carbonateplatform margin, the overlying Mississippian (Kinderhookian to Chesterian) foreland basin fan and overlap assemblage rocks include compositionally immature, syntectonic, siliciclastic units that were derived in large part from the Antler allochthon to the west (Johnson and Pendergast, 1981; Poole and Sandberg, 1991). Final convergence of the Antler orogen with western North America during the Early Mississippian thrust Devonian and underlying lower Paleozoic basin and slope rocks as much as 145 km eastward over coeval shelf-margin and outer-shelf rocks, forming the Roberts Mountains thrust system (Fig. 8; Stewart, 1980; Johnson and Pendergast, 1981; Poole et al., 1992). Recent models of the Roberts Mountains thrust system characterize it as a complex zone of intercalated, folded, thrust, and imbricated upper Precambrian to middle Paleozoic structural-stratigraphic units (e.g., Theodore et al., 1998; Noble and Finney, 1999; Crafford and Grauch, 2002). These relationships greatly complicate efforts to precisely reconstruct the paleogeography of the depositional systems that operated at this time. CARBONATE PLATFORM FACIES Hundreds of books, monographs, symposium volumes, and journal articles have been devoted to the sedimentology, stratal geometries, biota, petrology, diagenesis, resource potential, and other aspects of modern and ancient shallow-water carbonate platforms. The following brief overview is intended to highlight some 225 of the characteristics of carbonate platforms that are exhibited at stops described in this guide. Only a few references are cited herein, but the interested reader is encouraged to consult them and choose from the abundant cited references that they provide. Background Many early reports on carbonate rocks were exhaustive petrographic studies of the rock and fossil particles that compose limestones and dolostones of different ages, and were published in German, French, Italian, Russian, and other languages, as well as in English. Much of the non-English material was ignored or unappreciated by American geologists. By the 1970s, enough understanding was achieved to synthesize the accumulated field, subsurface, and petrographic studies into facies models that could help predict the distribution of rock types in carbonate depositional systems. Research on existing shallow-water carbonate environments, such as the Bahama Banks, the Yucatan-Belize shelf, and the Great Barrier Reef, together with regional work on classic ancient localities such as the Devonian reef complex of northwest Australia, the Permian reef complex of west Texas, and the Triassic exhumed atolls of the Italian Dolomite Alps, all helped establish the “carbonate platform” paradigm as the basic framework for the accumulation of most marine shallow-water carbonate rocks. Two classic volumes are fundamental resources for carbonate workers. Wilson (1975) comprehensively synthesized results from studies worldwide and showed how carbonate platforms functioned as similar sediment-accumulation systems through time. He demonstrated how platforms of different ages had similar three-dimensional forms but were generated by different organisms that adapted and evolved over time. In addition to corals and algae that dominate modern platform seaward margins, older margins and rims were constructed by various carbonatefixing organisms, such as bacteria, sponges, bryozoans, brachiopods, tube-building worms, and bivalve and gastropod mollusks. From the stromatolitic environments in the Proterozoic to the coral-algal (“coralgal”) reefs of today, platform carbonates accumulated laterally and stacked vertically in response to relative sea-level changes that controlled the availability of accommodation space for the in situ generation of new sediment. The compendium edited by Scholle et al. (1983) brought together the knowledge of varied carbonate depositional environments, from continental and lacustrine to pelagic deep-marine, and offered several chapters on the supratidal to subtidal environmental bands that occur across carbonate platforms. Many other volumes dedicated specifically to carbonate platforms followed (e.g., Crevello et al., 1989; Tucker et al., 1990; Simo et al., 1993). Although some carbonate-dominated shorelines lead seaward down gently inclined ramps, important facies faunas were those that built and maintained a seaward shallow-platform rim into the active wave zone. A very narrow band of reefoid facies, along wave-influenced seaward platform margins, separates the expansive and relatively quiet lagoonal environments landward of the rims from the steep, debris-covered aprons seaward of them. 226 Warme et al. Carbonate accumulations commonly become cemented directly on the seafloor, most notably strengthening the critical narrow band of reefoid and related facies along seaward margins. Bored hardgrounds, sharply eroded transgressive surfaces, short-term disconformities, and other evidence show that seafloor cementation and early burial cementation and diagenesis may completely lithify the sediments of each short-term sediment accumulation, or cycle, prior to initiation of the following one. The Carbonate Platform Signature: Cyclostratigraphy The basic building block of shallow-water carbonate, evaporite, and siliciclastic sedimentary deposits is generally agreed to be the “shallowing-upward cycle,” which has been described from worldwide examples in rocks of Proterozoic to Recent ages (e.g., Ginsburg, 1975). Carbonate platforms commonly exhibit obvious stacked meter-scale cycles whose analysis has given rise to the discipline of “cyclostratigraphy” (e.g., Elrick, 1995). A cycle is generated when flooding creates accommodation space that is invaded by carbonate-producing organisms, which establish the “carbonate-generating factory” in situ across the platform. A fully preserved idealized cycle is a vertically stacked package of genetically related beds of subtidal, intertidal, and supratidal facies, bounded by exposure surfaces that form between cycles (e.g., Hardie and Shinn, 1986; chapters in Loucks and Sarg, 1993). Of course, each cycle has an intertidal to supratidal feather edge that limits the internal sequence of facies, and every platform at any moment has a particular mosaic of shoals, channels, and clusters of carbonate-producing and sediment-trapping organisms. Thus, cycles are expected to show internal lateral variation. Nevertheless, numerous examples have been documented where an individual distinctive cycle, or bundle of cycles, was traced laterally for many kilometers without significant change in their interval character. We will see such examples in field traverses through the Guilmette Formation during this excursion. Debate about carbonate rock cycles, whether they are driven mainly by external (allocyclic) forces such as climate periodicity and global sea-level response, or internal (autocyclic) processes such as local diastrophism and expected sediment dispersal and accumulation patterns, has prompted numerous studies of modern and ancient platforms coincident with a range of theoretical models. Increased computing power has allowed development of increasingly sophisticated models. A recent example are the models of Burgess (2006), whose paper also contains a comprehensive review and reference list for the history of the extrinsic/ intrinsic debate, which has not yet been fully resolved. With the advent of “sequence stratigraphy” (e.g., Wilgus et al., 1988), researchers tested stratal patterns for hierarchical arrangements that indicated response to relative sea-level changes on various time scales, most notably within the astronomically driven Milankovitch time band in which climate change oscillated at four or more different astronomically fixed intervals, each a few tens of thousands to hundreds of thousands of years in duration (cf., papers in Arthur and Garrison, 1986). The oscillations are not syn- chronized, so that they may cancel or reinforce each other through time. However, the concept of sedimentary cycles, driven by relative sea-level changes, regardless of cause, is widely accepted. In sequence-stratigraphic terms, a simple system of oscillating sea level together with continuous subsidence could account for the generation and preservation of such cycles (Sarg, 1988). Packages of cycles were documented whose facies prograded, retrograded, and stacked, creating successions of shallow-water platform carbonates that in some cases were hundreds or even thousands of meters in thickness, shown or presumed to be preserved behind some form of subsiding platform rim. Cycles of shorter duration within the Milankovitch band, the ~20,000 yr or ~40,000 yr oscillations, may progress faster than carbonate sediment can accumulate. Some cycles exhibit evidence for transgressive drowning that deepened the platform to below wave base, or regressive shallowing that exposed the platform top to karstification and pedogenesis. Because the sediment cycles are commonly only a few meters thick, they may represent a compressed record of the maximum sea levels that occurred during their genesis. In such cases, sea level rose at a faster pace than sediment could accumulate, then fell to meet the surface of aggrading sediments before the maximum accommodation space was filled. Thus, the exact magnitude of maximum relative sea-level change over a platform during the life of a cycle cannot be fully known, and is a product of local subsidence, eustatic change that may have occurred, and sediment accumulation rate. Factors that further influence sediment accumulation in any cycle include the somewhat unpredictable mosaic carbonate production and accumulation across any given platform, and the results of rare events such as storms. However, together with the preserved cycle thickness, the magnitude of bathymetric change can be estimated using lithofacies and biofacies depth indicators that may be captured and compressed within a cycle. Within any vertical succession, several similar platform cycles may be bundled, separated from other bundles by a surface that represents extended exposure or an interval that indicates prolonged drowning. Such bundles have been interpreted, not without controversy, to represent shorter-term Milankovitch cycles (tens of thousands of years) captured within longer-term ones (hundreds of thousands of years). However, platform cycles commonly appear to be sorted into bundles of similar internal character. More significant regional surfaces of exposure or drowning across platforms may serve to vertically partition bundles of cycles into longer-term sequences. Thus, platform carbonate rocks commonly exhibit a hierarchy of shallowing-upward cycles, separated by a hierarchy of surfaces. The life of a platform may cease by a pronounced relative drop of sea level, exposure, and karst development, or by marine drowning, from which the shallow-water platform environment, with its cycle-generating mechanism, never recovers. Examples in the field trip area include the terminal exposure and karst formation at the top of the Simonson Dolostone, and the deepening and extinction of the shallow platform at the top of the Guilmette Formation; both examples are exhibited on the traverse of Stop 1. In Nevada, Devonian carbonate-platform cycles have been studied in detail, arranged into sequences, and analyzed for the Devonian carbonate platform of eastern Nevada transgressive-regressive sea-level history that they may reveal. North of the field trip area, bed-by-bed analyses include those of Elrick (1995, 1996) for Lower and Middle Devonian formations, and LaMaskin and Elrick (1997) for the Guilmette Formation. Within the field trip area, Estes-Jackson (1996) provided similar descriptive detail and interpretation of cycles in the Guilmette exposed in the fault block (Fig. 2) adjacent to the Hancock Summit West location of Stop 1. Chamberlain and Warme (1996) and Chamberlain (1999) developed the sequence analysis summarized in the composite stratigraphic column of Figure 11 and the accompanying Table 1. FIELD TRIP AREA Figure 10 shows the field trip area and location of stops we have chosen to include in this field guide. Numerous other localities, in ranges within and beyond the trip area, also contain excellent exposures of Devonian formations. Prior field trip guides that cover some or all of the area are those of Sandberg et al. (1997), which was extensively drawn upon for the present guide, and Gillespie and Foster (2004), which also contains seven reprinted papers on the Alamo Breccia. This guide is the first to focus mainly on the Devonian platform beds and their interpretation. Stop Locations The stop locations described herein may be visited independently, in any order. However, Stop 1, Hancock Summit West, contains a thick, continuous section of Devonian formations that are accessible, well exposed, and typical of the field trip area. Hence, Stop 1 is most useful as an initial section for comparisons with stratigraphic units at other stops and beyond. Starting Point The location of each stop is described as the direction and distance from a central point in the field trip area: a wayside rest near Crystal Springs, at the junction of Nevada State Highways 375 and 318, at the southern edge of the small settlement of Hiko (Fig. 10). Global Positioning System (GPS) coordinates at the Crystal Springs rest area are: lat 37°13′57.20″ N., long 115°24′56.75″ W., Hiko 7.5′ quadrangle. DEVONIAN FORMATIONS Devonian formations to be studied are the Lower Devonian Sevy Dolostone, Lower to Middle Devonian cherty argillaceous unit and Oxyoke Canyon Sandstone, Middle Devonian Simonson Dolostone and Fox Mountain Formation, Middle to Upper Devonian Guilmette Formation, and Upper Devonian West Range Limestone. See Figures 6 and 7 and cited papers for precise ages, lateral equivalents, and interrelationships of these formations. Figure 11 is a composite column of formations, nearly 5000 ft (~1500 m) thick, from the upper part of the Sevy 227 Dolostone to the post-platform Devonian to Mississippian Pilot Shale and Lower Mississippian Joana Limestone. The column represents an attempt to place the Devonian formations in the field trip area into a sequence-stratigraphic framework. It was constructed by Alan Chamberlain (Chamberlain and Warme, 1996; Chamberlain, 1999) on the basis of outcrops in the central Timpahute Range, close to Stop 3. The depicted sequence differs in detail from sequences exposed at other stops. For example, at Stop 3 the upper Guilmette Formation, shown in the column of Figure 11, contains a thick carbonate buildup (Dgb3), directly over the Alamo Breccia (Dgb2), and only sparse, thin quartz sandstone beds. In contrast, the upper Guilmette at Stop 1 contains thick sandstone intervals and lacks a buildup, whereas at Stop 4 it contains both small buildups and sandstones over the Breccia. The central column of Figure 11 shows basic rock types, partitioned vertically into sequences. The sequences were defined in two ways. The first method was to identify and describe individual shallowing-upward cycles in as much detail as possible from available outcrops. This process resulted in bundles of two to as many as 29 cycles of generally similar character. These cycles are listed on Table 1 and shown as excursions on the graphed line to the right of the column. The second method was to create a companion log of the outcrops using a hand-held gamma-ray scintillometer, shown as the graphed line to the left of the column. The two methods were combined to define sequences that contained cycles of similar lithologic character and gamma-ray signature, separated from other sequences by distinctive but commonly subtle surfaces that signify exposures, significant marine transgressions, or other environmental shifts. The graphed line to the right of the column was interpreted as a rough proxy for relative sea-level changes across the platform (for details see Chamberlain and Warme, 1996; Chamberlain, 1999). Characteristics of these sequences are discussed in the text for the stops. Note, however, that many of the sequence boundaries tend to match the boundaries of named formations and members, from the upper Sevy Dolostone (Dse3) at the base to the carbonate buildup over the Alamo Breccia (Dgb3) at the top. The overlying upper segment of the informal upper member of the Guilmette Formation was partitioned into five thick sequences (Fig. 11), some of which could be useful for further subdivision. This example shows an important attribute of sequence stratigraphy, whereby rock bodies are bounded by genetically significant surfaces that mark bathymetric shifts or other environmental events. Boundaries of many members, lenses, and tongues, which originally may have been loosely characterized by terms such as “transitional” or “first occurrence” of a given lithology, can be refined, redefined, or clarified if such surfaces are present and recognized. Guilmette Formation All stops described in this guide, except Stop 2, include the Guilmette Formation, which is the least dolomitized and 228 Warme et al. 115° 116° 38° 0 50 mi. 0 80 km 6 3 2 4 Crystal Springs 1 OR 37° Alamo 5 ID NEVADA UT White Pine Co. Nye Co. CA Lincoln Co. N 0 100 km Detailed map Clark Co. AZ Figure 10. Index and highway map of southeastern Nevada, showing locations of field trip Stops 1–6 (numbered stars) and Crystal Springs, the starting point for field trip road logs. Modified from: http://www.nevadadot.com/traveler/maps/StateMaps. Devonian carbonate platform of eastern Nevada most lithologically variable formation because it contains the Alamo Breccia Member. The Guilmette and its members at Stop 1 are shown in Figures 11–14. The following review is a history of studies and proposed lithostratigraphic subdivisions of this formation. Initially, Reso (1963) divided the Guilmette into informal lower and upper members. The lower member terminated at the top of a thick, stromatoporoid-rich breccia that was documented at Hancock Summit West (Stop 1), along strike in Guilmette exposures on the west side of the West Pahranagat Range, and also near Mount Irish (Stop 3). At Mount Irish, a similar breccia lies directly under a ~50-m-thick stromatoporoid-rich mound (“Reso’s Reef”). Consequently, Reso interpreted that breccia as mound talus, as did Dunn (1979), whose main objective was the study of the mound proper. Because the thick breccia at Hancock Summit West contains abundant stromatoporoids, it was probably also regarded as reef debris, although no large reef is exposed there. At both localities the thick breccia is the Alamo Breccia Member. Estes-Jackson (1996) described and interpreted a Guilmette stratigraphic section that is exposed on the fault block adjoining Stop 1, one mile east of Hancock Summit West (see Fig. 2). The section is almost identical to that traversed at Stop 1. She identified 22 shallowing-upward cycles in Reso’s lower member and 47 cycles in his upper member. She believed that the thick breccia at the top of the lower member was a normal, but perhaps deeper, platform facies and not a cataclysmic bed; however, it too is the Alamo Breccia Member. She calculated that the cycles fell within the lower part of the Milankovitch band, each of less than 100,000 years duration. Estes-Jackson (1996) documented the sandstone facies of the upper Guilmette, which is well represented at Stop 1 and in many other ranges of eastern Nevada, but is largely absent from the nearby central Timpahute Range where the stratigraphic column of Figure 11 was generated. Kuehner (1997) subdivided Reso’s (1963) lower member of the Guilmette Formation into three units, which are exposed in several ranges: a basal, yellow-weathering “slope forming interval,” a “ledge forming interval,” and the then newly designated Alamo Breccia Member. He retained Reso’s upper member for the balance of the Guilmette. Sandberg et al. (1997) partitioned Reso’s (1963) lower member of the Guilmette into three members (Fig. 14). Their “yellow slope-forming” and “carbonate platform facies” members are similar to Kuehner’s two lower “intervals.” They formalized the highest interval as the type Alamo Breccia Member of the Guilmette Formation. However, elsewhere the widespread cataclysmic Alamo Breccia rests not on the Guilmette, but on an erosive surface cut into Middle Devonian formations. At Stop 6 (Fig. 10) the Breccia takes the form of Units interpreted as fallback and resurge breccias associated with the Rim Realm (Pinto and Warme, 2008), and offshore to the west as deep-water channels of the Runout/Resurge Realm (Fig. 9) that were described at several localities by Morrow et al. (2005) and Sandberg et al. (2005, 2006). 229 Sandberg et al. (1997) also described the lower part of Reso’s upper member, shown as the “slope facies member” on Figure 14. The four Guilmette members shown on Figure 14 total ~220 m in thickness. However, at Stop 1 the entire Guilmette totals ~660 m. Our traverse will include the upper ~440 m, which is highly heterolithic but contains classic facies that are signatures of Devonian carbonate platforms. This interval has not been described in detail on “Downdropped Mountain,” but a description in the adjacent fault block is available (Estes-Jackson (1996). Chamberlain and Warme (1996) and Chamberlain (1999) provided the composite stratigraphic column of Figure 11. The Devonian platform formations were divided into sequences, defined by bundles of similar cycles or trends in cycles. These are briefly described in Table 1. In general, the interval from the base of the Guilmette to the top of the Alamo Breccia, Reso’s lower member, is similar across several ranges in southeastern Nevada, but the remainder of the Guilmette, Reso’s upper member, exhibits more variation between ranges as well as within the member. Alamo Breccia Member of Guilmette Formation Various facies of the Alamo Breccia Member of the Guilmette Formation are traversed at Stop 1 and Stops 3–6 and are described in this guide. The Breccia has been treated in detail in other guides and papers, so it is described herein with only enough detail to satisfy our purposes of placing it in stratigraphic context, showing its characteristics, and confirming its genesis as a cataclysmic deposit created by a bolide (i.e., a large craterforming projectile such as an asteroid or comet). Figure 9 shows the general distribution of Alamo Breccia outcrops, grouped into genetic Realms. Stop 1 and Stops 3–5 lie within the Ring Realm, where the Breccia is expressed as four sequential units of distinctive facies, which are labeled as parts of the Alamo Breccia Member on Figure 14. These units were described in detail, initially by Warme and Sandberg (1995, 1996), most recently by Pinto and Warme (2008), and in several intervening reports. Two of the units occur together in the Breccia. The lowest one, termed Unit D in past reports, is a detachment monomict breccia that formed between the undamaged carbonate platform beds below and Unit C megaclasts composed of displaced but intact cyclic platform beds above. The two remaining Alamo Breccia units are polymict breccias of chaotically bedded Unit B, which may extend to the base of the Breccia, as shown in Figure 14, and sorted and graded beds of Unit A that everywhere top the Breccia. For more in-depth study and understanding of the Breccia, we suggest that this field guide be augmented by the following easily obtained references, copies of which are provided to participants of the field trip for which this guide was prepared: Warme and Sandberg (1996), Sandberg et al. (1997, 2005), Warme and Kuehner (1998), Morrow and Sandberg (2001), Morrow et al. (2001, 2005), Warme et al. (2002), Warme (2004), Warme and Pinto (2006), and Pinto and Warme (2008). 230 Warme et al. A Figure 11 (on this and following page). (A) Composite stratigraphic column of Devonian section near Silver Canyon (Stop 3), showing sequences, surface gamma-ray log, relative sea-level curve, and sequence-boundary features. (B) Legend for sequence symbols, boundary features, and lithologic symbols used in Figure 11A. From Chamberlain and Warme (1996) and Chamberlain (1999). See Table 1 for sequence thicknesses, numbers of cycles, and significant features. Devonian carbonate platform of eastern Nevada B 231 Figure 11 (continued). TABLE 1. THICKNESSES, NUMBERS OF CYCLES, AND SIGNIFICANT FEATURES OF DEVONIAN SEQUENCES NEAR SILVER CANYON (STOP 3), AS SHOWN IN THE STRATIGRAPHIC COLUMN OF FIGURE 11 Sequence abbreviation MDp2 MDp1 Dwr Dgg Dgf Dge Dgd Dgc Dgb3 Dgb2 Dgb1 Dga2 Thickness ft (m) 115 (35) 130 (39) 153 (46) 567 (172) 268 (81) 235 (71) 406 (123) 188 (57) 97 (29) 179 (54) 26 (8) 145 (44) No. of cycles 2 2 4 29 16 17 23 6 2 1 2 8 Dga1 250 (76) 12 Dgys 182 (55) 10 Dgfm Dsiualt 135 (41) 285 (86) 4 12 Dsibc Dsilalt Dsicxln 85 (26) 265 (80) 225 (68) 4 12 4 Dox2 Dox1 95 (29) 100 (30) 2 4 Dse3 240+ (73+) 12+ Significant features; weathering profile Silicified stromatolites and laminated black chert; slope Silty limestone capped with fossil bone-bearing sandstone; slope Silty, burrowed limestone; partly covered slopes Carbonate cycles capped by thick (>3 m) quartz sandstone beds Slightly deeper cycles and more limestone than in adjacent sequences Carbonate cycles capped by thin (<3 m) quartz sandstone beds Amphipora dolopackstone; dark-gray ledges and cliffs Silty limestone with abundant gastropods and burrows; slope Stromatoporoid and coral reef facies; light-gray cliffs Graded bed of carbonate breccia, open-marine fauna; brown-gray cliffs Abundant corals, stromatoporoids, and Amphipora; limestone cliffs Shallowing-upward cycles that successively deepen upward, predominately limestone, open-marine fauna; ledges and slope Shallowing-upward cycles that successively deepen upward, predominately dolostone, open-marine fauna; ledges and slope Yellow, silty dolostone, stromatolites, and cycles capped by thin beds of very fine-grained quartz sandstone, ostracodes; slope Open-shelf fauna, brachiopod Stringocephalus; resistant cliffs Shallowing-upward cycles that successively deepen upward giving an alternating dark and light band appearance, karst breccia; ledges Open-shelf fauna with corals and stromatoporoids; dark brown-gray cliff Alternating intertidal-supratidal or dark and light bands; ledges Coarsely crystalline dolostone capped by karst surface; light-gray to light graybrown cliffs Quartz sandstone with hummocky cross-bedding at base; ledge Burrowed, silty dolostone with flat-pebble conglomerate at base; light-brown slope Light-gray, fine-grained, laminated dolostone; slopes, base concealed TOTAL 4370+ (1324+) 188+ Note: Modified from Chamberlain and Warme (1996) and Chamberlain (1999). 232 Warme et al. Mj Tv End p MD Dgu b Dga Dgs p Dgc Dgl sf Dgy 375 ay hw ig lH ria Ex tra ter res t Acc es s road Dfm t ual Dsi bc Dsi Figure 12. Oblique Google Earth aerial view (eye altitude: 2.2 km) to the southeast of “Downdropped Mountain,” Stop 1 at Hancock Summit West, showing access road, traverse route, and stratigraphic units including brown cliff (Dsibc) and upper alternating (Dsiualt) members of Simonson Dolostone, Fox Mountain Formation (Dfm) undivided, and yellow sloping-forming member (Dgysf), lower member (Dgl), type Alamo Breccia Member (Dgab), and upper member (Dgu) of Guilmette Formation. Dgcp and Dgs denote carbonate platform and slope facies, respectively, of Guilmette Formation shown in the stratigraphic column (Fig. 14). Other units: MDp, Pilot Shale; Mj—Joana Limestone; Tv—Tertiary volcanic rocks. Image modified from http://earth. google.com/. Stop 1 Start traverse Figure 13. West face of Hancock Summit West (Stop 1), with stratigraphic sequence including the upper part of Simonson Dolostone (Dsi), Fox Mountain Formation (Dfm), and yellow slopeforming member (YSF), lower member (Dgl), type Alamo Breccia Member (lower Units D–C and upper Units B– A), and upper member (Dgu) of Guilmette Formation. The Alamo Breccia Member is ~55 m thick. The Stop 1 traverse ascends the ridge along the skyline from right to left (Fig. 12). Stop 1 access road is visible in foreground. Devonian carbonate platform of eastern Nevada 233 Figure 14. Stratigraphic section, facies, conodont biostratigraphy, and conodont biofacies at Hancock Summit West (Stop 1; Figs. 12 and 13) of upper member of Fox Mountain Formation and lower part of Guilmette Formation, showing type section of Alamo Breccia Member. Shows position of 24 conodont samples used to constrain biostratigraphic age. Conodont biofacies abbreviations: Icr.—icriodid; Pol.-icr.—polygnathidicriodid; No c.—no conodonts. From Sandberg et al. (1997). 234 Warme et al. FIELD TRIP STOPS Stop 1. Hancock Summit West: Middle and Upper Devonian Formations, and Type Section of the Alamo Breccia Location Stop 1 is at the informally named “Downdropped Mountain” or “Down Dropped Block” (Fig. 12), which is a prominent ridge south of, and parallel to, Highway 375, from 12–14 mi (19–22 km) west of the starting point at the Crystal Springs rest area. The entrance to Stop 1 is a gravel road at the west end of a guardrail along the south side of Highway 375, 2.2 mi (3.5 km) by road west of Hancock Summit. The gravel road descends into an arroyo and highway maintenance gravel pit that bounds the northwest side of the mountain. The road continues southwest down the arroyo. The Stop 1 traverse begins at the lowest beds exposed along the bank, 0.5 mi (0.8 km) from Highway 375 (Fig. 12). Coordinates at the Stop 1 parking area and base of traverse: lat 37°24′36.04″N., long 115°24′05.42″W., Crescent Reservoir 7.5′ quadrangle. Rock Units Exposed Simonson Dolostone (brown cliff member, upper alternating member, informal “upper coarse crystalline member”), Fox Mountain Formation, Guilmette Formation, and possibly West Range Limestone (Figs. 5 and 11). The Sevy Dolostone, cherty argillaceous unit, Oxyoke Canyon Sandstone, and lower members of the Simonson Dolostone (Fig. 11) are not exposed along the traverse of Stop 1; see Stop 2. The Simonson was divided into four informal members by Osmond (1954; Figures 5, 11): coarse member, now termed the coarse crystalline member (Johnson et al., 1989), which appears to be transitional from the Oxyoke Canyon Sandstone below and becomes more coarsely crystalline upward; lower alternating member, which contains alternating light and dark bands of beds and grades upward into the brown cliff member, which in turn grades into the upper alternating member. The upper member also commonly becomes coarsely crystalline upward, exhibiting an interval that is informally referred to as the “upper coarse crystalline member.” The Simonson Dolostone exhibits upward-shallowing cycles that are partially exposed in each member. The more dolomitic Simonson cycles are generally thinner and represent shallower conditions than those that are so well preserved in the overlying Guilmette Formation, and thus were probably situated more landward. However, structureless intervals at the base of many cycles probably represent lower intertidal to subtidal bioturbated limestone that was later dolomitized along with the entire formation. The underlying Sevy Dolostone, exposed in ranges nearby, may represent even shallower conditions, probably accumulated more dolomite-prone beds, and is even more strongly altered by regional dolomitization. The Fox Mountain interval was regarded as the upper unit of the Simonson Dolostone in Nevada or the lower member of the Guilmette Formation in Utah until it was recognized as a regionally widespread unit and given formation status by Sandberg et al. (1997), who divided it into lower and upper members. Part of the upper member at this locality is shown in the outcrop photograph of Figure 13 and the stratigraphic column of Figure 14. The history of studies and partitioning of the Guilmette Formation has already been recounted under “Devonian Formations.” The lower part of the Guilmette on the Stop 1 traverse was divided by Sandberg et al. (1997) into the four intervals shown on Figure 14: the “yellow slope-forming” and “carbonate-platform facies,” the type Alamo Breccia Member, and the “slope facies.” The “slope facies” is only the lower part of the upper Guilmette, which continues upward for an additional ~440 m and contains thick quartz sandstone intervals as well as beds that evidence both deep and shallow carbonate-platform environments. Objectives • Introduce several of the Devonian formations exposed in the field guide area. • Describe shallowing-upward cycles and their character in different formations. • Document fossils and ichnofossils of platform facies. • Discover significant surfaces; compare with established formation and member limits. • Note trend upward from dolostone of Simonson to mainly limestone of Fox Mountain and limestone/dolostone cycles in the Guilmette and discuss probable controls. • Discuss sedimentary structures and provenance of quartzose sandstone in upper member of Guilmette. • Discover varied character of Devonian exposure surfaces. • Introduce Alamo Breccia and its bolide impact signatures. Traverse The Stop 1 traverse begins in the brown cliff member of the Simonson Dolostone, at the base of the stratigraphic section exposed along the arroyo, and continues eastward up through the stratigraphic section for ~1 mi (~1.6 km) along a ridge that forms the drainage divide along the crest of “Downdropped Mountain” (Fig. 12). The traverse ends at the east end of “Downdropped Mountain,” at the base of the dip slope that marks the top of the exposed platform facies of the Guilmette Formation, or possibly within, or at the top of, a thin interval of West Range Limestone. East of “Downdropped Mountain” is a strike valley of Pilot Shale, accessible by a rough dirt road that enters from the north, and a ridge of Joana Limestone that is cut off at the south end by a major fault. Beyond the fault is the stratigraphic section studied by Estes-Jackson (1996), shown in Figure 2, and a twin of the section traversed at Stop 1. Observations Simonson Dolostone Brown Cliff Member: Rich brown color; conversion to dolomite of varying crystal sizes; relatively open platform evidenced Devonian carbonate platform of eastern Nevada by several forms of abundant stromatoporoids, some corals, and other invertebrates; cycle boundaries vague; transition upward to upper alternating member. Upper Alternating Member: Trend upward to light-gray color; cycles marked by structureless (bioturbated) lower intervals and algal-laminated upper intervals; fossils less abundant, mainly bulbous stromatoporoids; trend upward to coarser grained dolostone; pockets of yellow-weathering, coarse-grained dolomite crystals interpreted as karst fillings; abrupt shift across bedding upward to finer grained dolostone and absence of yellow crystals, indicating exposure surface and underlying episode of diagenetic recrystallization and solution; altered intervals with zebra rock and coarse crystallization associated with Devonian exposure surfaces and also with much later (Cenozoic) fault zones. Fox Mountain Formation The Fox Mountain was divided into lower and upper members by Sandberg et al. (1997). The contact between those members represents a regional shift from the underlying shallow-platform dolostone formations to open-marine platform limestones, and signals the termination of the long-lived very shallow platform that had existed from the beginning of Devonian deposition. The karst zone under the base of the lower member separates underlying Simonson dolostones from Fox Mountain beds interpreted as peritidal, restricted-marine, and evaporite-solution-breccia limestones. A second karst at the top of lower member separates these beds from open-marine crinoidal wackestones and encrinites of the upper member, which contains nautiloids, brachiopods (including Stringocephalus), and corals. The upper member represents initiation, in the Middle varcus conodont Zone, of the Taghanic onlap, a marine transgression recognized throughout North America and in parts of Europe (e.g., Johnson et al., 1985; Johnson and Sandberg, 1989). See Figure 14 for thicknesses and details of the upper member. Guilmette Formation Yellow Slope-forming Member: The yellow-weathering interval of fine-grained, dark-gray, silty dolostone beds forms the topographic saddle shown in Figure 13 and is underlain by several meters of stromatolitic dolostone that regionally represent the basal beds of the interval (Fig. 14). Note the columnar and branching stromatolites and yellow-weathering, silty dolostone and dolomitic siltstone beds that are replaced upward by darkgray limestones of the overlying member. Carbonate Platform Facies (Member): This member exhibits excellent examples of shallowing-upward cycles. They show basal transgressive erosion surfaces and sediment lags overlain by a lower interval of dark-gray bioturbated limestone that usually contains bulbous and other forms of stromatoporoids, and may contain other invertebrate fossils and oncolites. The upper part of cycles that are completely preserved becomes increasingly lighter gray, dolomitic, and algal laminated. Alamo Breccia Member: As shown on Figure 14, the base of this Member is marked by the subtle Unit D monomict 235 detachment breccia, overlain by Unit C megaclasts composed mainly of previously deposited platform cycles similar to those in the underlying member. Unit B is a chaotic heterolithic breccia with impact lapillistone clasts, overlain by Unit A graded beds with shocked and hematite-studded quartz grains (Warme and Sandberg, 1995, 1996; Morrow et al., 2005) and both local and exotic deformed clasts. The traverse along the drainage divide intercepts the Breccia where Unit B reaches the base of the Breccia and separates two Unit C clasts that are hundreds of meters in length. Unit B contains clasts, tens of meters in length, floating in a chaotic matrix. The stacked graded beds of Unit A are well exposed on the sloping ledge at the top of the Breccia. Slope Facies (Member): The member over the Alamo Breccia is varied. Beds are commonly mottled, fossiliferous limestones of deeper-water aspect (Warme and Sandberg, 1995, 1996; Sandberg et al., 1997), and exhibit one or more hardgrounds. The interval is partly covered, and ends at the thick quartz sandstone beds that continue upward into the lower part of the upper Guilmette (Fig. 12). Upper Guilmette (Member): The lowest interval of Reso’s upper Guilmette is the 35-m-thick “slope facies” member described above, which is overlain by quartzose sandstones that are broadly channeled, cross bedded, and exhibit biogenic sedimentary structures. The middle part contains biostromes and small bioherms of stromatoporoids, and beds rich in corals, gastropods, and bivalves including megalodonts. Limestones of the upper part are thin bedded and quartzose. They contain abundant biogenic sedimentary structures and at the top may include a thin interval of West Range Limestone. Stop 2. Sixmile Flat: Upper Sevy Dolostone, Cherty Argillaceous Unit(?), Oxyoke Canyon Sandstone, and Coarse Crystalline Member and Lower Alternating Members of Simonson Dolostone Location Stop 2 is situated north of Sixmile Flat, a broad valley east of the Hiko Hills (Figs. 9 and 10). From the Crystal Springs rest area starting point, travel 0.8 mi (1.3 km) east to Highway 93, then east on Highway 93 for 10 mi (16 km), past the south end of the Hiko Hills, entering Sixmile Flat and continuing to a dirt road on the left (north) that is the entrance to a cattle pen. Travel 0.4 mi (0.6 km) WNW to the pen, then north along a straight sectionline fence and gravel road for 5.8 mi (9.3 km) to a fence gate and cattle trail on the left (west) (Fig. 15). Stop 2 traverse begins 0.3 mi (0.5 km) west of the gate and can be approached part way by vehicles with high ground clearance. Coordinates at Stop 2 parking area at fenceline: lat 37°40′28.61″N., long 115°04′59.22″W., Hiko NE 7.5′ quadrangle. Rock Units Exposed Sevy Dolostone, cherty argillaceous unit(?), Oxyoke Canyon Sandstone, and coarse crystalline and lower alternating members of the Simonson Dolostone. The traverse can be con- 236 Warme et al. tinued upslope and into the brown cliff member, but is truncated northward by Cenozoic layered volcanic rocks (Fig. 15). Objectives • Overview of exposed formations. • Transition from Sevy Dolostone to local expression of cherty argillaceous unit (Dox1? of Fig. 11) and Oxyoke Canyon Sandstone (Dox2 of Fig. 11). • Deeper facies of Oxyoke Canyon Sandstone (Dox2 of Fig. 11): hummocky cross bedding and trace fossils. • Transition to cyclic bedding and gradual coarsening to top of coarse crystalline member. • Karst signatures at top of coarse crystalline member and finer-crystalline dolostone at base of lower alternating member. Traverse From dirt road proceed west on cattle trail to highest point of first shallow saddle, then walk south to the upper part of the Sevy Dolostone and start of northward traverse. Observations Cryptic evidence for platform cycles in heavily dolomitized Sevy Dolostone; disseminated fine-grained quartz in upper Sevy (Dox1?) sequence of Figure 11; varied quartz concentrations in upper Oxyoke Canyon (Dox2) sequence of Figure 11; identification of ichnotaxa in Oxyoke Canyon; confirmation of hummocky cross-stratification (HCS); nature of cycles, increasing coarse crystallinity, and increasing karst features in coarse crystalline member (Dsicxln of Fig. 11); abrupt fining of crystallinity at base of lower alternating member (Dsilalt of Fig. 11). Stop 3. Silver Canyon: Alamo Breccia and “Reso’s Reef” Location From Crystal Springs rest area starting point, travel north 2.5 mi (4.0 km) on Highway 318, into the settlement of Hiko, to entrance of gravel road on left (west; unmarked Logan Canyon Road). Travel northwest for 7 mi (11 km) to “Y” junction; turn right (unmarked Silver Canyon Road). Note excellent views of the white carbonate buildup at top of hill, front right; Alamo Breccia is steep cliff below the buildup. Continue north 1.3 mi (2.1 km) to two small, leveled parking and turnaround areas on right. Coordinates at Stop 3 parking area and base of traverse: lat 37°37′14.10″N., long 115°21′37.74″W., Mount Irish SE 7.5′ quadrangle. Rock Units Exposed Formations exposed north and east of the road are Devonian. To west of the road, in valley, are dark orange-brown-weathering acidic volcanic flows, some marked with American Native petroglyphs. Devonian formations in various fault blocks to east of road can be identified as Sevy Dolostone below the distinctive twin intervals of dark-brown-weathering Oxyoke Canyon Sandstone, and coarse crystalline member of Simonson Dolostone above them. Thick brown beds well above the Oxyoke Canyon are in the brown cliff member. Due east, a low ridge in the foreground has almost continuous exposures of upper Simonson Dolostone and Fox Mountain Formation, which are exposed below the distinctive yellow slope-forming member of the Guilmette. The member weathers to a light-yellow band across the near mountain face, and is labeled on Figure 16. The yellow band is overlain by an interval similar to the “carbonate platform facies” of Stop 1 (Fig. 14), labeled as lower Guilmette (Dgl) on Figure 16. This interval is overlain by the cliff-forming Alamo Breccia Member, which extends to the skyline on Figure 16. See description of lower three members of the Guilmette under Stop 1 (Fig. 14). The white carbonate buildup above the Breccia is not visible from the parking location. Objectives • Study graded beds of Unit A, upper interval of Alamo Breccia, containing large clasts of platform carbonates and clasts of impact lapillistone. • Note facies directly over Alamo Breccia that shift west to east, from dark, bedded, off-buildup intervals to massive white carbonate buildup. • Note interfingering buildup and off-buildup tongues. • Document evolution of buildup from base to top. • Discuss whether the buildup is mudmound, microbial mound, reef, or other alternatives. • Study karst developed across highest pinnacles of buildup. • Document cyclic shallow-water platform beds over buildup. Traverse Stop 3 traverse is ~1.75 mi (~2.8 km) each way. It begins at the right side of parking areas, northward up a gentle ridge (Fig. 16) that arcs eastward, crests, then drops down to a bench that separates the graded bed Unit A at the top of the Alamo Breccia from the base of the overlying buildup and off-buildup facies. As indicated on Figure 16, the traverse continues eastward around reentrants along the top of the Alamo cliff, to the center of the buildup facies over the Breccia. The last reentrant terminates in a steep wall at the base of the buildup, and exposes the early phases of its development. Return westward to notches where the buildup can be traversed upward to the crest. The traverse ends in dark carbonate beds over the structure. Return by same route, or take shortcut westward to intercept the ridge that leads to the parking area. Observations Beds at the beginning of the traverse dip westward into the Silver Canyon fault zone and are in the upper Guilmette over the Alamo Breccia. They contain low-spired gastropods and large solitary rugose corals. Alamo Breccia The Breccia is exposed along the south-facing slope of the traverse ridge, and the traverse follows the graded Unit A. Devonian carbonate platform of eastern Nevada Figure 15. Oblique Google Earth aerial view (eye altitude: 1.8 km) to the west of Stop 2 at Sixmile Flat, showing access road and trail, traverse route, and stratigraphic units including Sevy Dolostone (Dse), lower and upper members of Oxyoke Canyon Sandstone (Dox1? and Dox2, respectively), and coarse crystalline (Dsicxln), lower alternating (Dsilalt), and brown cliff (Dsibc) members of Simonson Dolostone. Image modified from http://earth.google.com/. End Dsibc Start traverse Dsilalt Dsicxln Dox1? Dox2 Dse 237 cess trail Ac 93 Fenceline Access road Stop 2 Dgu Dg-buildup Mt. Irish Dgab Dgl Traverse Dgysf Dfm Dox Dse Dsi Figure 16. Outcrop photograph of southfacing Devonian units east of Silver Canyon (Stop 3), including Simonson Dolostone (Dsi), Fox Mountain Formation (Dfm), and Guilmette Formation (Dgysf, yellow slope-forming member; Dgl, lower member; Dgab, Alamo Breccia Member; and Dgu, upper member, with “Reso’s Reef” organic buildup directly overlying Alamo Breccia). Faulted blocks of Sevy Dolostone (Dse) capped by dark-orange weathered cliffs of Oxyoke Canyon Sandstone (Dox) are visible in foreground. Stop 3 traverse route is shown by dashed white line. The traverse ascends ridgeline from the parking area, out of view to left (west), then follows the top of Alamo Breccia cliff and base of the buildup to the center of the buildup, then ascends the buildup onto the platform cyclic beds over it. 238 Warme et al. Scattered clasts of lapillistone may be encountered along the Unit A traverse to the top of the hill. Below the crest, the west-facing Breccia cliff exhibits a large-scale folded clast, tens of meters long. The south-facing Breccia cliff exhibits Unit A graded beds with sparse lapillistone clasts, and is interrupted by several bedparallel or tilted clasts, 10 m or more in length. One ~30-m-long tilted clast protrudes from the graded bed at the top of Unit A. Eastward, toward the carbonate mound, beds over the top of the Breccia become light gray to white, fossiliferous, and packed with stromatoporoids of both hemispherical and elongate forms; some elongate tabular forms are 1 m or more in maximum length. The sheer cliff at the end of the traverse exhibits the graded beds in Unit A at the top of the Breccia, is near the center of the buildup, and displays abundant stromatoporoids and an erect branching coral ~70 cm high, preserved in life position. Carbonate Buildups We use the non-genetic term “buildup” for carbonate accumulations with positive relief, because they exhibit a spectrum of compositions and frameworks and have been differently classified and variously named in numerous schemes. They include “reefs” that some workers restrict to shallow and wave-resistant bio-accumulations, and deep-water structures that are commonly termed “mudmounds.” A review of reef versus mudmound concepts is beyond the scope of this field guide. Discussion papers continue to appear. The volume edited by Monty et al. (1995) brings forth the controversies, and includes the contribution by Pratt (1995) who outlined the wide variability of “mudmounds” in time and space. They occur as early as Proterozoic and in every Phanerozoic period, contain variable proportions of mud-sized particles and potential frameworks, and encompass a variety of recognizable invertebrates that change over geologic time and that may play active or passive roles in mound formation. Most structures contain fine-grained cement that, without detailed petrographic study, is commonly difficult to differentiate from originally fine-grained clastic calcareous particles. Reso’s Reef The buildup at Stop 3 three has been termed a mudmound (e.g., Sandberg et al., 1997), but Dunn (1979) documented potential framework of several species of stromatoporoids and corals in the core of the structure, and used the term of bioherm. She listed invertebrates that include gastropods, brachiopods, and crinoid columnals within and adjacent to the buildup, which appears to contain a more abundant fauna than has been observed beyond its margins. One nautiloid has been found. These components are difficult to observe in the central core facies because of pervasive recrystallization. “Reso’s reef” could benefit from further investigation. An upward traverse through the buildup offers the chance to discuss its genesis: reef versus mudmound or other options. The upper ~10 m of the buildup shows increasing vugs and seams that are stained yellow, red, and orange, indicating that the top was exposed in Devonian time. A karst cave, 1 m in diameter, near the top exhibits a floor of bedded sediment that dips at about the same angle as the regional dip, providing a geopetal indicator and evidence that the solution occurred before regional tilting and not after current exposure. Beds over the buildup are cyclic and contain abundant Amphipora, indicating continued platform conditions. The stratigraphic column of Figure 11 was measured nearby. The sequence lacks thick sandstone beds, in contrast to the abundant sandstones in the upper Guilmette at Stops 1 and 4. Stop 4. Hiko Hills: Alamo Breccia and Evacuation Structure Location Stop 4 is located at the south end of the Hiko Hills. It is accessed by traveling east 0.8 mi (1.3 km) from the Crystal Springs rest area starting point to the end of Highway 318, turning north, then east on Highway 93 for 1 mi (1.6 km), and then north (left) onto a dirt road. The road skirts the west side of a gravel pit, becomes rough, and heads east-northeastward to the mouth of a small canyon at the base of the range. The canyon leads upward to outcrops of the Alamo Breccia intercalated with the Guilmette Formation. Coordinates at the Stop 4 parking area and base of traverse: lat 37°32′51.27″N., long 115°12′08.38″W., Hiko 7.5′ quadrangle. Rock Units Exposed Guilmette Formation: Alamo Breccia Member; cyclic platform carbonates in lower Guilmette Formation below the Breccia; cyclic carbonates, carbonate buildups, and broadly channeled sandstones above the Breccia. Objectives • Characterize internal fabric and components of Alamo Breccia. • Note character and distribution of lapillistone within Breccia. • Observe post–Alamo Event recolonization of carbonate platform: fossils, trace fossils, carbonate buildups. • View evacuation of matrix under finger of Unit C megaclast. Traverse From the mouth of the canyon, proceed up the main gully. The closest Breccia section is on a down-faulted block, detached from the mountain front. It contains excellent exposures of the clasts and matrix of Unit B in the middle part and stacked graded beds of Unit A in the upper part. The Guilmette above the Breccia exhibits platform cycles, which are heavily dolomitized and altered near the fault, which terminates the lower traverse. Upward, across the fault, is a more complete second exposure of the Breccia. The base of the Breccia is exposed across the fault. The Breccia may be traversed vertically to overlying beds, or laterally northward for several hundred meters along the west face of the Hiko Hills to observe variations within the Breccia and the overlying and underlying beds. Devonian carbonate platform of eastern Nevada Observations A climb through the lower Breccia outcrop reveals the chaotic character of Unit B: heterolithic clasts and variable matrix. The interval of Unit A contains three or more graded beds that become finer grained and thinner upward, and shows load, flame, and dewatering structures at bed boundaries. The top of the Breccia merges with a silty interval that contains faint crossbedding and abundant ichnofossils resembling Teichichnus. This section was discussed by Sandberg et al. (1997). Recovery of the platform biota after the Alamo Event is under study (Tapanila and Anderson, 2007). Across the fault, the upper traverse begins with a thick section of chaotic Unit B matrix and heterolithic clasts. As shown in Figure 17, Unit B terminates upward at a surviving finger of cyclic beds that project eastward from the top of the 80-mthick Unit C clast visible to the west. Pinto and Warme (2008) described the unusual relationships between the very thick Unit C clast, nearly in its original position, and the laterally adjoining matrix of the Alamo Breccia. The finger of platform beds extends from the upper part of the thick Unit C clast, over ~60 m of Unit B breccia. During the Alamo Event, this finger initially remained intact, then fractured and parted in two places, allowing well-sorted clasts from the already accumulated overlying Unit A to cascade down the new slots. The structure is interpreted to have formed when some of the Unit B breccia was evacuated from under the finger. This process is proposed to be part of the ring-forming adjustments of the transient crater in later phases of the Alamo Event (Pinto and Warme, 2008). Stop 5 provides a second example of this process. Northward, the thick Unit C interval of intact cyclic beds can be traversed ~0.25 mi (~400 m) to a vertical fault, beyond which most of the Unit C clast was destroyed and replaced by the chaotic Unit B, which displays a variety of spectacular clasts tens of meters long. The upper 10 m of the Breccia contains a train of numerous lapillistone clasts that appear to be remnants of the same lapillistone bed. Above the Alamo Breccia are discontinuous light-gray-weathering carbonate buildups with abundant stromatoporoids and fewer colonial corals, and stacks of broadly channelized quartzose sandstones, interbedded with cyclic carbonates. Details of the Breccia in this area were documented by Kuehner (1997). 239 canyons between the ridges (Fig. 18), where the Alamo Breccia is displayed, are ~0.6 mi (~1 km) from the highway, and can be reached on foot. Coordinates at the Stop 5 parking area at Highway 93 and base of traverse (approximate): lat 37°04′35.01″N., long 114°59′25.24″W., Pahranagat Wash 7.5′ quadrangle. Rock Units Exposed The lower Guilmette Formation dips more steeply than the structural dip along the western face of the southern end of the Delamar Mountains, so that the Alamo Breccia caps several isolated east-west–trending ridges that slope westward, the underlying carbonate-platform facies member is exposed in the intervening small valleys, and the yellow slope-forming member (terminology of Sandberg et al., 1997) forms an irregular strike valley east of the ridges. Northward, Middle Devonian beds under the yellow slope-forming member crop out along a series of very irregular ridges and valleys. Objectives • Note relatively thin interval of lower Guilmette members. • Observe the scale and distribution of giant tabular clasts that compose ~80% of the Alamo Breccia. Discuss origin and significance for genesis of Alamo Breccia. • Note unusually well-sorted matrix between clasts, and lithologic similarity with Unit A at top of Breccia. • Inspect small stromatoporoid patch reef within Unit C detached clast. • Note subtle expression of Unit D monomict detachment breccia. • Time permitting, traverse eastward, down section, to the yellow slope-forming member, and continue northeast into the underlying Middle Devonian formation with abundant bioherms and biostromes of pentamerid brachiopods, stromatoporoids, and corals. Traverse From Highway 93, approach the front of the Delamar Mountains (Fig. 18) and traverse one or more of the isolated ridges of Alamo Breccia and one or more intervening valleys. Time permitting, walk northward in the yellow-weathering strike valley east of the ridges, then northeastward topographically up and stratigraphically down into the exposed Middle Devonian fossilrich dolostone beds. Stop 5. Southern Delamar Mountains: Stacked Tabular Clasts in Alamo Breccia Observations Location Stop 5 is located near the southern end of the Delamar Mountains, where they verge closest to Highway 93 (Fig. 18). From the starting point at the Crystal Springs rest area, travel east 0.8 mi (1.3 km) to the end of Highway 375, then south on Highway 93 for 35 mi (56 km), passing through the settlements of Ash Springs and Alamo. The Alamo Breccia is the irregular interval that caps several ridges that dip westward toward the highway. Entrances to The lower Guilmette under the Alamo Breccia is similar, but overall thinner, to that at Stops 1, 3, 4, and other locations in the field trip area to the north. However, the fossil-rich Middle Devonian interval, under the yellow slope-forming member, may be either the brown cliff member of the Simonson Dolostone or the upper member of the Fox Mountain Formation. This stratigraphy suggests that the upper alternating member of the Simonson and the lower member of the Fox Mountain were 240 Warme et al. Figure 17. Photograph and diagram of Alamo Breccia evacuation structure at the south end of the Hiko Hills (Stop 4). Breccia interval is 100 m thick. (A) View to northeast showing characteristic shallow-water carbonate-platform cyclic bedding of the Guilmette Formation above and below Breccia. (B) Left: unusually thick (~80 m) preserved Unit C megaclast with thin (~10 m) Unit A graded beds over top. Center and right: cyclic carbonates equivalent to the megaclast disintegrated down to the level of detachment (Unit D), except for an upper finger of beds (F) that extended over newly formed Unit B chaotic breccia. The finger broke into pieces as some of the underlying Unit B was evacuated. Lapillistone clasts (L) as much as 50 m under the finger represent early-precipitated beds that were broken and mixed with Unit B. One or more later lapillistone beds precipitated from the impact plume, became partially lithified, and were preserved as a discontinuous trail of broken and smeared lapillistone within a graded bed of Unit A (black circles), which formed across the whole area in a late phase of the Alamo Event after the finger collapsed. Post-Event deposits in this area include buildups, up to ~40 m high, containing stromatoporoids and corals (R). From Pinto and Warme (2008). Devonian carbonate platform of eastern Nevada 241 Alamo Breccia outcrops Tv Gr e at Ba sin Hw y Figure 18. Oblique Google Earth aerial view (eye altitude: 1.2 km) to the southeast of Stop 5 at the southern Delamar Mountains, showing isolated Alamo Breccia outcrops (labeled) capping eastwest–trending ridges. Stacked tabular clasts within the Breccia are visible. Highway 93 is labeled. Tv indicates Tertiary volcanic rocks. Image modified from http://earth.google.com/. 93 either not deposited or were eroded prior to deposition of the yellow slope-forming member. The Alamo Breccia at Stop 5 is atypical and difficult to interpret as part of the Alamo Breccia scenario. The long, tabular, stacked clasts and sparse, presorted interclast matrix (Fig. 19) have not been observed at other Alamo Breccia localities. Stop 5 is ~85 km from the present position of Tempiute Mountain (unrestored), Stop 6, where the beds are interpreted as a fragment of the Alamo crater rim. At Stop 5, the Breccia is ~60 m thick and contains stacked irregular clasts that are a hundred meters or more in length. The mega-fabric of the clasts suggests that they moved eastward, not northwestward in the direction of Tempiute Mountain (Figs. 9 and 20) or westward toward the paleo-platform margin. The orientation of large-scale clasts in the Alamo Breccia at other localities, much closer to Tempiute Mountain, indicates movement approximately westward, as if they were sliding toward the crater or the seaward platform margin (Kuehner, 1997; Warme and Kuehner, 1998). In addition, the total thickness of the Alamo Breccia here is ~60 m (Fig. 19), whereas it is thinner at some localities closer to the present position of Tempiute Mountain or to the trend of the platform margin. Pinto and Warme (2008) proposed that the clasts at Stop 5 were detached, moved eastward, and stacked over one another during the ring-forming processes associated with adjustment of the transient crater. In this scenario, listric-fault-bounded, arcuate segments of the platform dipped outward, fault footwalls became rings, and near surface intervals of beds detached and slid away, perhaps collecting near the footwall of the next ring fault outward. Figure 9 shows that both Stops 4 and 5 are located near the outer edge of the Ring Realm of the Alamo Breccia, suggesting that significant faulting formed one or more outer crater rings and an adjacent moat that collected Alamo Breccia. Stop 6. Tempiute Mountain: Crater-Rim Impact Stratigraphy Location From the Crystal Springs rest area travel ~33 mi (53 km) on Highway 375 westward, past Stop 1, then northwest to the Coyote Summit road marker. Continue northwest on Highway 375 for 3.0 mi (4.8 km) and turn east on a dirt road that leads to Tempiute Mountain (Fig. 20). Travel eastward for 1.4 mi (2.2 km) to fork; turn left (northeast) and continue 1.7 mi (2.7 km) to canyon mouth, where road is washed out. Continue on foot eastward up canyon through old mining works to cliff of Alamo Breccia, Stop 6A (Fig. 20). Coordinates at the Stop 6 parking area and base of traverse: lat 37°36′58.44″N., long 115°38′51.84″W., Tempiute Mountain South 7.5′ quadrangle. Rock Units Exposed The west face of Tempiute Mountain clearly exposes Paleozoic formations from the Ordovician Eureka Quartzite to the 242 Warme et al. Figure 19. View to south-southwest of Alamo Breccia outcrop that caps the dip slope at the southern end of the Delamar Mountains (Stop 5). Image is tilted to restore horizontal, which is indicated by trend of ridge of the Sheep Range in distance at right in (A) and slanted line in (B). (A) Photo of northern slope of one of several east-west–trending ridges that display Alamo Breccia with unusual tabular megaclasts and very little matrix. Note 60-m scale of total Breccia. (B) Units of the Breccia include the detachment surface (D), jumbled megaclasts that continue to the top of the Breccia in most places (C), limited internal chaotic Breccia (B), and topmost graded beds that are now in the process of eroding away (A). R represents stromatoporoid buildups within displaced clasts. From Pinto and Warme (2008). Mj M Dp Grants Peak 6A Ddg b Da Traverse 6B Stop 6 Dsm Dox Dse Sl Oes Oe W ild ca tC Access road Figure 20. Oblique Google Earth aerial view (eye altitude: 2.1 km) to the southeast of Stop 6 at Tempiute Mountain, showing access road, traverse route, Stop 6A and 6B locations, and stratigraphic units including Eureka Quartzite (Oe), Ely Springs Dolostone (Oes), Laketown Dolostone (Sl), Sevy Dolostone (Dse), Oxyoke Canyon Sandstone (Dox), Sentinel Mountain Dolostone (Dsm), Alamo Breccia (Dab), Devils Gate Limestone (Ddg), Pilot Shale (MDp), and Joana Limestone (Mj). The detailed, complex, crater-rim stratigraphy of the Alamo Breccia and adjacent units is depicted in the columnar section of Figure 21. Grants Peak (7199 ft, 2182 m) and Wildcat Canyon are also indicated. Image modified from http:// earth.google.com/. n. ny Devonian carbonate platform of eastern Nevada Mississippian Joana Limestone (Fig. 20). Devonian formations include the Sevy Dolostone, cherty argillaceous unit, Oxyoke Canyon Sandstone, Sentinel Mountain Dolostone (and Bay State Dolostone, if it was locally preserved), Alamo Breccia, Devils Gate Limestone, and Devonian to Mississippian Pilot Shale. The Sentinel Mountain and Bay State Dolostones are deeper platform equivalents of the Simonson Dolostone. All of the Guilmette Formation, or its equivalent that was deposited in this section, and probably all of the Fox Mountain Formation, were cut out and replaced by newly defined Units 3–5 of the Alamo Breccia, as shown in Figure 21 and so far discovered only at Tempiute Mountain. Objectives • Review characteristics of impact beds, interpreted as preserved inner rim of Alamo crater, as depicted in the stratigraphic column of Figure 21. • Stop 6A: Note features of Unit 3, interpreted as large-scale fallback breccia clasts and matrix, and base of resurge beds, Unit 5. • Stop 6B: Discriminate between characteristics of parautochthonous impact breccias (Unit 1), developed nearly in situ in Lower to Middle Devonian Oxyoke Canyon Sandstone and Middle Devonian Sentinel Mountain Dolostone (and Bay State dolostone?) and contrasting exotic clasts characteristic of Units 3–5. • Note features of injected sedimentary sills and dikes, Unit 2, into Unit 1. • Discuss interpretations for shatter-cone-like structures in Unit 1 dolostones. • Note features of Unit 3, interpreted as intensely deformed fallback breccia; Unit 4, interpreted as smeared or flattened fallback breccia; and Unit 5, interpreted as resurge of impact debris into crater, against inner crater rim, or across newly formed slope. • Discuss depositional environment of post-impact deepwater limestones labeled Devils Gate (Fig. 21). Traverse Steeply dipping Paleozoic formations are exposed along the washed-out track in the axis of the canyon, and are labeled on Figure 20. Most noticeable is the Ordovician Eureka Quartzite near the canyon mouth, and the Devonian Oxyoke Canyon Sandstone midway to the cliff of Alamo Breccia that terminates the eastward segment of the road, which is Stop 6A (Fig. 20). Stop 6B requires a significant commitment of time. Return west ~330 ft (~100 m) to intersection of steep road that leads northward, up past mine workings and an abandoned shaft, to drainage divide and a view northward of the stratigraphic section on Tempiute Mountain, northwestward across Sand Spring Valley, and west to the settlement of Rachel on Highway 375. This point is the beginning of the traverse for Stop 6B, which runs along the ridge that leads eastward to the range crest (Fig. 20). Return via the same route. 243 Observations Stop 6A Exposures along the north side of the easternmost ~165 ft (~50 m) of road show 20 or more lithologies of smashed and interpenetrated Unit 3 megaclasts, some as much as several meters across, that are interpreted as a heterolithic fallback Alamo Breccia (Pinto and Warme, 2008). Near the cliff face at the end of the road is a sandstone clast identified as the only megascopic fragment of probable Ordovician Eureka Quartzite found thus far, providing evidence for crater excavation to depths of 1.5–2.0 km. Other clasts appear milky white and marbled, and are candidates for partial melting of target rock during the cratering process (Pinto, 2006). The fallback breccia matrix is best exposed in sparse outcrops on the steep slope that leads to the next ridge north. The matrix contains a variety of clasts, shocked quartz grains, and impact lapilli mixed with the heterolithic clasts (Pinto and Warme, 2008), Stop 6B From the Stop B starting point (Fig. 20) the road becomes level and continues a short distance northward, then eastward into the next east-west drainage, and provides excellent views of the next ridge to the north and its south-facing foreground slope. This excursion of the traverse is shown on Figure 20. Visible from west to east, in ascending order, are: the irregularly silicified upper Sevy Dolostone; the well-bedded cherty argillaceous unit that is not well represented in localities to the east but is a deeper-water facies that may correlate to Dox1 of Figure 11; indurated and cross-bedded Oxyoke Canyon Sandstone, equivalent to Dox2 of Figure 11; and Sentinel Mountain Dolostone and possibly Bay State Dolostone, equivalent to the Simonson Dolostone of shallower facies on the platform. Weathered brownish-orange patches in the Sentinel Mountain are injected and sediment-filled sills and dikes of Unit 2, which can be inspected in outcrops near the canyon axis at the end of the road (Fig. 20). The east end of the ridge contains the Alamo Breccia, Devils Gate Limestone, Pilot Shale, and Joana Limestone, which cannot be discriminated from this viewpoint, but can be traversed along the ridge of Stop 6B (Fig. 20). Return to Stop 6B starting point. Beginning at the Stop 6B starting point (Fig. 20), the traverse eastward along the ridge axis exhibits almost continuous exposures that represent impact stratigraphy, as interpreted by Pinto (2006) and Pinto and Warme (2008). The traverse crosses breccias of parautochthonous deformed bedrock overlain by exotic fallback and resurge clasts, all interpreted to be preserved on the inner rim of the transient Alamo crater (Fig. 21). Along the ridge, the cross-bedded, silica-cemented, upper part of the Oxyoke Canyon Sandstone (S1A), together with the very dark-gray to black beds of the Sentinel Mountain Dolostone (S1B), are designated as the parautochthonous Unit 1 impact breccias on the stratigraphic column of Figure 21. This 300-m-thick interval is thoroughly fractured, faulted, and injected with the sediment-filled 244 Warme et al. Figure 21. Columnar section of Devonian rocks at Tempiute Mountain (Stop 6), showing the thickness and character of Alamo impactogenic Units 1–5, the underlying upper part of the Sevy Dolostone (Dse) and cherty argillaceous unit, the overlying deep-water Devils Gate Limestone (Ddg), and the Pilot Shale (MDp). Parautochthonous impact breccias of Unit 1 are composed of the Oxyoke Canyon Sandstone (S1A) and Sentinel Mountain Dolostone (S1B). Unit 2 is injected polymict breccia that tends to be thickest where it swells, pinches and separates S1A and S1B. S1B contains shatter-cone–like structures, interpreted as impact-induced. Units 3 and 4 are composed of allogenic limestone clasts with varied matrices that bear shocked quartz, lapilli, and other particles interpreted as shock and melt indicators. Unit 5 is two thick resurge breccias. From Pinto and Warme (2008). Devonian carbonate platform of eastern Nevada dike-and-sill system of Unit 2 and interpreted as nearly in situ altered bedrock. Note the abundant shatter-cone–like structures and related features in the black dolostones. The dolostone breccias of Unit 1 are overlain by the mainly limestone breccia Units 3 and 4. Unit 3 is a well-exposed, roughly graded, fallback breccia with clasts as much 10 m in exposed length. The better sorted smaller clasts of Unit 4, averaging ~5 cm in length, are interpreted as a separate fallback event of heterolithic clasts that were partially melted, weakened, and smeared. In contrast, Unit 5 is composed of two 30-m-thick graded beds of generally angular, clean-washed, heterolithic clasts that are interpreted as resurge flows deposited against the inner wall of the crater rim or across a new slope that formed by collapse of the platform margin during later stages of the Alamo Event. The upper graded bed fines imperceptibly into the post-Breccia deep-water limestones labeled Devils Gate on Figure 21. Of interest in the Devils Gate is the lack of benthic invertebrates and ichnotaxa, presence of small pelagic or nektonic species, and several debrites, as much as ~4 m thick, of locally derived slumps and ripup clasts with varying proportions of quartz grains derived from elsewhere. Hypotheses for the depositional environment of the Devils Gate at this locality include post-Event crater fill and slope veneer. 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