Exhumation of the North American Cordillera revealed by multi-dating of Upper Jurassic–Upper Cretaceous foreland basin deposits Clayton S. Painter†, Barbara Carrapa, Peter G. DeCelles, George E. Gehrels, and Stuart N. Thomson Department of Geosciences, University of Arizona, 1040 E. 4th Street, Tucson, Arizona 85721, USA ABSTRACT New low-temperature thermochronology and geochronology data from Upper Jurassic–Upper Cretaceous strata from the North American Cordilleran foreland basin in Utah, Colorado, Wyoming, and South Dakota document rapid exhumation rates of the adjacent Cordilleran orogenic belt to the west. Both zircon (U-Th-[Sm])/He (zircon He) and apatite fission track (AFT) thermochronology were applied to proximal and distal synorogenic deposits in order to identify a thermochronometer suitable to record source exhumation during the North America Cordilleran orogeny. AFT lag times from Upper Jurassic–Upper Cretaceous deposits are 0–5 m.y. and indicate a relatively steadystate to slightly increasing exhumation rate between 118 Ma and 66 Ma. These lag-time measurements are consistent with active shortening and rapid exhumation rates of ~0.9–>1 km/m.y. of the North American Cordillera throughout the Cretaceous. Double dating of the detrital AFT samples was performed on apatites with young AFT cooling ages, in order to test whether or not the young cooling ages represent a signal related to exhumation rather than volcanic activity. Maximum depositional ages using detrital zircon U-Pb geochronology match existing ages on basin stratigraphy. This study indicates that AFT is the most effective thermochronometer to resolve source exhumation from Lower to Upper Cretaceous foreland stratigraphy in the central Cordilleran foreland, and indicates that source material was exhumed from 4 to 5 km depths but was never buried more than a few kilometers (<4 km) since Cretaceous time. Zircon He dates indicate that the orogenic hinterland could not have been exhumed from depths >8–9 km. Double dating of apatites (with † Now affiliated with ConocoPhillips; Clayton.S .Painter@conocophillips.com. AFT and U-Pb) shows that volcanic contamination is a significant issue that can, however, be addressed by double dating. INTRODUCTION Foreland basin deposits are an important archive of orogenic growth and tectonic processes (Aubouin, 1965; Dickinson, 1974; Dickinson and Suczek, 1979; Jordan, 1981; DeCelles and Giles, 1996; DeCelles, 2004; Miall, 2009). Many researchers have used coarse-grained foreland basin deposits to date thrusting events, identify unroofing sequences, and identify provenance. Examples of these techniques are clast counting of synorogenic conglomerates and sandstone petrographic analysis (Dickinson, 1985; Graham et al., 1986; Lawton, 1986; DeCelles, 1988; Steidtmann and Schmitt, 1988; Horton et al., 2004). Thermochronology applied to detrital minerals from foreland basin deposits is a powerful tool to infer the timing of sediment source cooling and exhumation (Bernet et al., 2001; Carrapa et al., 2003, 2006; Najman et al., 2005; Reiners and Brandon, 2006; Carrapa, 2010). While traditional provenance techniques provide information on the type of sediment sources through time, thermochronology provides unique information on the timing and rates of sediment source exhumation and on the thermal history of the sedimentary basin as well. In particular, detrital thermochronology can be applied to measure lag time, which is the difference between the depositional age of the detrital minerals and their cooling ages (Garver et al., 1999). Lag-time trends also provide information on the mode of orogenic growth (Bernet et al., 2001; Carrapa et al., 2003; Carrapa, 2009). Lag time of foreland basin deposits can thus successfully measure the long-term exhumation history of orogenic belts over large catchment areas (Cerveny et al., 1988; Coutand et al., 2006; Spiegel et al., 2004). In addition, many of the allochthonous thrust sheets in the North American Cordillera have since been eroded and later obscured by Basin and Range extensional tectonics, leaving only the foreland basin deposits as a record of exhumation history. Despite the great potential of such an approach in North America, to date, no detailed detrital thermochronological study had been applied in the retroarc foreland basin of the North American Cordillera. The goal of this study is to determine the timing, pattern, and rates of cooling of the North American Cordillera in order to better understand the modes of exhumation and contribute to models of fold- thrust belt and foreland basin evolution. In this study we apply zircon (U-Th-[Sm])/He (zircon He) and apatite fission track (AFT) thermochronology and zircon U-Pb geochronology to samples from Upper Jurassic–Upper Cretaceous coarse-grained foreland basin deposits in Utah, Colorado, Wyoming, and South Dakota, in order to determine provenance cooling history and maximum depositional ages (Table 1; Figs. 1, 2, and 3). Furthermore, U-Pb thermochronology can be used to assess whether the young cooling-age populations were contaminated by young, Cordilleran arc–derived apatites, and thus record cooling related to magmatic events rather than exhumation ages of the Cordilleran thrust belt. Lag-time patterns and exhumation rates calculated from this study are here compared to basin-filling and orogenic-growth models. Coarse-grained deposits have been interpreted to represent contrasting tectonic processes. For example, some researchers have asserted that proximal upward-coarsening successions represent orogenic growth, but that distal upward-coarsening successions represent periods of tectonic quiescence, flexural rebound, and the reworking of proximal deposits into the distal foreland (Beck et al., 1988; Blair and Bilodeau, 1988; Heller et al., 1988). This model has been called the two-phase stratigraphic model (Heller et al., 1988). In contrast, others have linked distal coarse-grained deposits to times of active shortening and orogenic growth, and propose that the increase in sediment supply during these periods of active orogenic GSA Bulletin; Month/Month 2014; v. 1xx; no. X/X; p. 1–26; doi: 10.1130/B30999.1; 16 figures; 6 tables; Data Repository item 2014223. For permission to copy, contact editing@geosociety.org © 2014 Geological Society of America 1 Painter et al. Sample 051101 051102 051103 051104 051105 051106 051107 051108 051201 051204 051205 051206 051207 051208 051209 051210 051211 051212 051213 051214 TABLE 1. SAMPLE LIST, LOCATION, AND ANALYSES DONE Location Latitude Stratigraphic unit Longitude Sample type Chilson Member, N43.44490° Detrital Lakota Formation W103.77887° Chilson Member, N43.44490° Detrital Lakota Formation W103.83715° N43.44717° Morrison Formation Detrital W103.83905° N43.69704° Frontier Formation Detrital W106.69336° N40.96244° Frontier Formation Detrital W109.47128° N40.95719° Dakota Sandstone Detrital W109.47023° N40.52022° Cedar Mountain Formation Detrital W109.52075° N40.54865° Morrison Formation Detrital W109.52416° N40.96344° Echo Canyon Conglomerate Conglomerate clast W111.41634° N40.76712° Kelvin Formation Detrital W111.40012° N41.58785° Lazeart Sandstone Detrital W110.63001° N41.87089° Frontier Formation Detrital W110.52497° N41.48659° Detrital Blair Formation W108.96523° Brooks Member, N41.35810° Detrital Rocks Springs Formation W108.93082° Trail Member, N41.32461° Detrital Ericson Formation W108.94299° Canyon Creek Member, N41.31646° Detrital Ericson Formation W108.92226° N41.31762° Almond Formation Detrital W108.90691° Chimney Rock Tongue Member, N41.39890° Detrital Rock Springs Formation W108.93394° N42.56673° Detrital Cloverly Formation (A interval) W106.70624° N42.52449° Morrison Formation Detrital W106.74066° Analysis type DZ U-Pb Zircon He AFT DA U-Pb x x x x x x x x x x x x x x x x x x x x x x x x x x x x (continued ) growth is greater than the accommodation space created by flexural subsidence in the proximal foredeep and leads to rapid progradation into the distal foreland basin (Burbank et al., 1988; DeCelles and Giles, 1996; Horton et al., 2004). We compare our exhumation trends and rates based on lag-time measurements to predictions made from both of these basin-filling models. Active shortening and orogenic growth should produce small lag times and rapid exhumation rates, whereas flexural rebound and reworking of stored deposits into the distal foreland should produce larger lag times. At a larger scale, lag times have been used to interpret trends in orogenic wedge behavior and to identify when orogenic wedges were in subcritical or supercritical states (Carrapa, 2009); these predictions are based on the Coulomb wedge model, which describes orogenic growth as a function of the wedge’s taper (Davis et al., 1983; Dahlen, 1984). Decreasing lag times are predicted during a subcritical wedge 2 state when the wedge is building internally, whereas increasing lag times are predicted during a supercritical wedge state, when the wedge is rapidly propagating into the foreland basin (Carrapa, 2009). We use this model to interpret our lag-time trends and identify the overall Cordilleran orogenic wedge behavior during the Cretaceous. GEOLOGIC BACKGROUND Timing of the initial development of the Cordilleran retroarc thrust belt has been the source of some debate. Some workers propose that thrusting began during the Early Cretaceous (Heller et al., 1986), whereas others state that thrusting began during the Late Jurassic (ca. 155 Ma) (DeCelles and Burden, 1992; DeCelles and Currie, 1996; Currie, 1997). Thrusting within the Cordilleran retroarc thrust belt continued until ca. 50 Ma (DeCelles, 2004) (Fig. 1). Early in the history of the adjacent foreland basin, nonmarine sedimentation dominated and included the Upper Jurassic Morrison Formation and Lower Cretaceous Cedar Mountain– Cloverly–Kootenai Formations (Suttner, 1969; Furer, 1970; Currie, 1997). Between ca. 110 Ma and ca. 71 Ma, marginal marine to fully marine deposition dominated the foreland basin while the epicontinental Western Interior Seaway extended from the Gulf of Mexico to the Arctic Ocean north of Alaska. Isopach maps show that from ca. 155 Ma to ca. 88 Ma, a flexurally influenced to flexurally dominated retroarc foreland basin was located east of the North America Cordilleran orogenic belt in the western U.S.A. (Jordan, 1981; Roberts and Kirschbaum, 1995; Currie, 1997; DeCelles, 2004). Although flexural subsidence continued to be influential after 88 Ma, the isopach pattern becomes diffuse, suggesting that dynamic subsidence may have influenced the foreland’s geometry (Pang and Nummedal, 1995; Roberts and Kirschbaum, 1995; Mitrovica et al., 1989; Geological Society of America Bulletin, Month/Month 2014 Exhumation of the North American Cordillera TABLE 1. SAMPLE LIST, LOCATION, AND ANALYSES DONE (continued ) Location Analysis type Latitude DZ DA Zircon He AFT Stratigraphic unit Longitude U-Pb U-Pb Sample Sample type N37.11554° 051218 Dakota Sandstone Detrital x x x W111.85088° N41.31892° 051219 Ericson Formation Detrital x W108.93170° N42.23242° 07.28.11 Adaville Formation Detrital x W110.31064° N39.96674° 060922 Price River Formation Conglomerate clast x W111.47218° N39.96532° 060923 Price River Formation Conglomerate clast x W111.47127° N40.00208° Sam 3 Price River Formation Conglomerate clast x W111.40743° N40.00193° Detrital x Sam 5 North Horn Formation W111.40824° N40.00498° Sam 7 North Horn Formation Detrital x W111.40840° N40.00193° Sam 8 North Horn Formation Conglomerate clast x W111.40945° N39.34931° Sam 11 Inkom Formation Paleozoic strata x W112.28324° N39.51203° Sam 13 Price River Formation Detrital x W111.73695° N40.16784° Sam 15 Castlegate Formation Detrital x W108.87477° N40.16843° Sam 16 Castlegate Formation Detrital x W108.87371° N40.20236° Sego Sandstone Member: Detrital x* x x x Sam 17 Mesaverde Group W108.86123° Sego Sandstone Member: N40.20167° Sam 18 Detrital x* Mesaverde Group W108.86312° N39.88097° Sam 19 Castlegate Formation Detrital x W111.21610° Sego Sandstone Member: N40.17529° NSD4 B Detrital x x Mesaverde Group W108.82601° Note: This is a comprehensive list of all samples presented in this paper and the analytical work performed on each sample (see Figs. 2 and 3 for a visual location of each sample). Sample type indicates whether the sample was a detrital sandstone foreland basin sample, or a conglomerate cobble from wedge-top deposits. DZ U-Pb—detrital zircon U-Pb; zircon He—zircon (U-Th-[Sm])/He thermochronology; AFT—apatite fission track thermochronology; DA U-Pb—detrital apatite U-Pb thermochronology. *Detrital zircon samples published by York (2010); all other analyses are new. DeCelles, 2004; Liu and Nummedal, 2004). By ca. 81 Ma, dynamic subsidence appears to have been a significant control on basin geometry (Roberts and Kirschbaum, 1995; Pang and Nummedal, 1995; Liu and Nummedal, 2004; Painter and Carrapa, 2013). Even though the cause of dynamic subsidence remains ambiguous (Pang and Nummedal, 1995), some have modeled it as a result of a cold and shallowing subducting slab (Mitrovica et al., 1989; Gurnis, 1993). Isopach thicknesses indicate that by the Maastrichtian, ca. 71– 65 Ma, Laramide-style basement-cored uplifts had begun to partition the foreland and create isolated basins (Dickinson et al., 1988; DeCelles, 2004). During uplift of basement-involved structures to the east, Cordilleran orogenic deformation continued in the west (DeCelles, 2004). During foreland basin development adjacent to the North America Cordilleran orogenic belt, coarse-grained deposits (i.e., sandstone to conglomerate) episodically prograded past the proximal foredeep and into the distal foreland, hundreds of kilometers east of the contemporary thrust front. The mechanism controlling deposition of these distal coarse-grained deposits has been debated over the years. Some have proposed that whereas upward-coarsening successions in the proximal foreland basin represent active shortening in the fold-thrust belt and are synorogenic, upward-coarsening successions in the distal foreland represent reworking of coarse material from the proximal foreland following isostatic rebound and reworking during times of tectonic quiescence (Fig. 4) (Beck et al., 1988; Blair and Bilodeau, 1988; Heller et al., 1988). Heller et al. (1988) proposed that during times of active shortening and tectonic loading, flexural subsidence rates are high, and coarsegrained deposits are trapped in the proximal foreland. After active shortening ceases, flexural rebound replaces flexural subsidence, which leads to exhumation and reworking of coarse proximal deposits out into the distal foreland basin (Fig. 4). In contrast, other researchers interpret coarse-grained deposits that prograde rapidly into foreland basins as being syntectonic (Burbank et al., 1988; DeCelles and Giles, 1996; Horton et al., 2004). This flux-driven model, described by Paola et al. (1992), predicts that orogenic growth supplies more sediment to the foreland basin than the basin can accommodate through flexural subsidence; this results in rapid widespread progradation of sediments (Burbank et al., 1988; Paola et al., 1992; DeCelles and Giles, 1996; Horton et al., 2004). Accordingly, exhumation in the fold-thrust belt should follow the same predictions, and lag times should be short as a response to rapid erosion and little sediment storage. Relatively little thermochronological work has been done in the North American Cordillera of the western U.S.A. Various thermochronological studies have focused on Laramide mountain ranges in the Rocky Mountains (Cerveny, 1990; Cerveny and Steidtmann, 1993; Omar Geological Society of America Bulletin, Month/Month 2014 3 Painter et al. 104°W thermal gradient (e.g., Turcotte and Schubert, 2002), and rapidly deposited in the foreland basin. However, if tc > td, then tL > 0. Small lag times represent rapid exhumation, whereas large lag times represent slow exhumation (Garver et al., 1999). Constant lag times over a long period of time represent steady-state exhumation, whereas decreasing lag times represent increasing exhumation rates, and increasing lag times represent episodic or decreasing exhumation rates (Garver et al., 1999; Bernet et al., 2001; Carrapa et al., 2003) (Fig. 6). If the lag time of distal grains in coarse-grained foreland deposits approximates zero, then the deposits are assumed to be of syntectonic origin, implying no reworking from proximal foreland basin strata. However, if tL of distal coarse-grained foreland deposits is large, then reworking of deposits from proximal parts of the foreland basin during flexural rebound is plausible, as predicted by the two-phase stratigraphic model of Heller et al. (1988) (Fig. 4). This approach is valid only if the thermochronological ages are not reset or partially annealed after deposition. In the case of this study, post-depositional partial annealing is unlikely because stratigraphic thicknesses, ages, and subsidence histories in the Cordilleran foreland basin system suggest that sediment burial during the Early Cretaceous to Cenozoic never exceeded 2–3 km in eastern Utah (DeCelles and Currie, 1996). 49°N N PRB B BH WRB D-JB GRB U-PB 37° N PB SJB Sevier fold-thrust belt Cordilleran magmatic arc Laramide foreland province 0 Major thrust fault Study area 550 200 kilometers Major basins − Abbreviations outlined in caption Figure 1. Regional index map of the western U.S.A. including the Sevier fold-thrust belt, Laramide province, Cordilleran magmatic arc, and major basins (modified from DeCelles, 2004). Basins shown are the San Juan (SJB), Paradox (PB), Uinta-Piceance (U-PB), Denver-Julesburg (D-JB), Green River (GRB), Wind River Basin (WRB), Big Horn (BHB), and Powder River (PRB). et al., 1994; Crowley et al., 2002; Kelley, 2002; Peyton et al., 2012) and on the Colorado Plateau (e.g., Dumitru, et al., 1994; Flowers et al., 2007, 2008). Burtner and Nigrini (1994) and Burtner et al. (1994) used vitrinite reflectance and AFT thermochronology to study the Idaho-Wyoming part of the Sevier fold-thrust belt and concluded that anomalously high geothermal gradients during the Late Jurassic–Early Cretaceous were caused by gravity-driven fluid flow. Preliminary fission track analyses from the Upper Jurassic Morrison Formation and the Lower Cretaceous Cloverly Formation in Wyoming indicate late Neocomian–early Albian cooling ages (Heady, 1992; DeCelles and Burden, 1992; Swierc and Johnson, 1996; Chen and Lubin, 1997). In addition, the experimental work of Guenthner et al. (2013) includes some zircon He work from the foreland basin and the Sevier fold-thrust belt in Utah. However, to date, no detailed detrital thermochronological study of Cordilleran foreland basin strata is available. Zircon He and AFT thermochronometers measure the time of cooling through the 170– 190 °C and 60–120 °C temperature windows respectively, i.e., partial retention or annealing zone (PRZ, PAZ) (Gleadow and Duddy, 1981; Gleadow et al., 1983; Laslett et al., 1987; Wolf 4 et al., 1998; Reiners et al., 2004). At temperatures above the lower limit of the PRZ, the mineral system becomes open and begins to lose the radiogenic daughter product. In the case of zircon He, He diffuses out of the system. In the case of AFT, ion disruption tracks, a record of the spontaneous fission of 238U, begin to anneal (i.e., shorten). In order to determine pattern and rates of cooling and exhumation of the Cordilleran orogenic belt, we use lag-time measurements. Lag time (tL) is defined as the difference between the cooling age of a detrital mineral (tc) and the depositional age (td) of its hosting strata (Brandon and Vance, 1992; Garver et al., 1999) (Fig. 5): t L = tc − td . (1) To determine td, we use a combination of existing age controls based on published biostratigraphic and 40Ar/39Ar age controls and our new detrital U-Pb geochronologic ages (Table 2). Different lag-time patterns reveal different exhumation behavior in the source area. If tc ≈ td, then tL ≈ 0, indicating a very small lag time (Garver et al., 1999) (Fig. 5). This means that for the AFT system, the mineral was exhumed from 4 to 5 km depth, assuming a 20 °C/km geo- Existing Stratigraphic Age Control Stratigraphic age control in the retroarc foreland basin of the North America Cordillera is based on radiometric dating and biostratigraphy. Ammonite and inoceramid biostratigraphic zones and 40Ar/39Ar ages of bentonite beds have been used in the past (Baadsgaard et al., 1993; Obradovich, 1993; Obradovich et al., 2002; Izett et al., 1998; Gradstein and Ogg, 2004). Cobban et al. (2006) compiled these data and provided a biostratigraphic zonal data table for much of the Upper Cretaceous North America Cordilleran foreland basin. The stratigraphic age control of fluvial and alluvial-fan deposits is instead based on palynology (e.g., Jacobson and Nichols, 1982; DeCelles and Burden, 1992; Kowallis et al., 1991; Horton et al., 2004). In some cases, age control comes from proximal marine biozones that are correlated to the fluvial deposits (Martinsen et al., 1999), as well as 40Ar/39Ar and K-Ar geochronology on tuffs within the fluvial deposits. Below is a discussion on the existing age control for the Upper Jurassic–Upper Cretaceous stratigraphy in the Utah-Wyoming-South Dakota area of the foreland basin. The stratigraphic units discussed below are the horizons sampled for this study, Geological Society of America Bulletin, Month/Month 2014 Exhumation of the North American Cordillera 45° N BH B PRB 051101 051102 051103 051104 N A′ WRB 051213 051214 07.28.11 051207 051208 051209 051211 051212 051219 051206 051205 051105 051106 051201 051204 060922 060923 051108 051107 Sam 19 Sam 13 D-JB GRB U-PB 41° N Sam 16 Sam 18 NSD4 B Sam 11 PB A 051218 SJB 109°W0 250 500 Sevier fold-thrust front km Major basins − SJB (San Juan Basin), PB (Paradox Basin), U-PB (Uinta-Piceance Basins), GRB (Green River Basin), D-JB (Denver-Julesburg Basin), WRB (Wind River Basin), PRB (Powder River Basin) BHB (Big Horn Basin) Sample location with sample ID Figure 2. Index map of the study area showing Utah, Wyoming, Colorado, and western South Dakota in the western U.S.A. Map shows sample distribution. Sample information can be found in Table 1. A to A′ is the trend in which samples are plotted in Figure 3. and all samples and sample locations are found in Table 1 and Figures 2 and 3; age data are also compiled and presented in Table 2. The Upper Jurassic Morrison Formation was sampled from three geographically distinct areas in eastern Utah, central Wyoming, and western South Dakota. In eastern Utah, the Morrison Formation spans 154.8 ± 0.6 Ma to 135.2 ± 5.5 Ma (Kimmeridgian–Valanginian), based on both 40 Ar/39Ar dating and K-Ar techniques (Kowallis et al., 1991, 1998; Peterson, 1992) (Tables 1, 2; Figs. 2, 3). In central Wyoming, near Alcova Reservoir, the age of the Morrison Formation has been demonstrated to be 154.8 ± 0.6 to ca. 145 Ma (DeCelles and Burden, 1992; Currie, 1998). The older control is based on stratigraphic ties to the age reported in the lower Morrison Formation by Kowallis et al. (1991), and the younger boundary is based on palynomorphs (DeCelles and Burden, 1992) (Table 2). The far eastern extents of the Morrison Formation in eastern Colorado and Wyoming and western South Dakota and Oklahoma have been constrained with biostratigraphy. Litwin et al. (1998) reported palynomorphs in the Morrison Formation of that region that span latest Oxfordian– Tithonian time. On the basis of ostracodes and charophytes, Schudack et al. (1998) reported the same ages for the Morrison Formation as Litwin et al. (1998) (Table 2). The Kelvin Formation (equivalent of the Cloverly Formation) in northeastern Utah, near Rockport Reservoir, has been interpreted as Aptian–Albian, ca. 126–112 Ma (Crittenden, 1963; Hale and Van de Graaf, 1964; Kauffman, 1969; Ryer, 1977), based on lateral stratigraphic correlations that place the Kelvin Formation above the nearby Upper Jurassic Morrison Formation (Crittenden, 1963; Hale and Van de Graaf, 1964; Ryer, 1977). The age control on the upper boundary is from the overlying Mowry and Aspen Shales that contain the lower Cenomanian Neogastroplites cornutus (Kauffman, 1969; Ryer, 1977) (Table 2). Multiple researchers have tried to date the Cloverly Formation (a Kelvin Formation equivalent) in Wyoming with a variety of methods; Zaleha (2006) reviewed existing age controls and determined that palynology provides the most reliable results. In Wyoming, the Cloverly spans the Early Cretaceous (Valanginian) to midAlbian (DeCelles and Burden, 1992; DeCelles et al., 1993; Furer et al., 1997; O’Malley, 1994; Way, 1997; Currie, 1998; Burton et al., 2006). The A interval (Meyers et al., 1992; May et al., 1995; Zaleha, 2006) of the Cloverly Formation near Alcova Reservoir in central Wyoming is Early Cretaceous (Valanginian–Barremian) based on palynomorphs reported in DeCelles and Burden (1992) (Table 2). In western South Dakota, the Lakota Formation is the Cloverly Formation equivalent; it spans Aptian to mid-Albian time (Waagé, 1959; Post and Bell, 1961; Dahlstrom and Fox, 1995; Way et al., 1998; Zaleha, 2006; Sames et al., 2010). The lowest member of the Lakota Formation in the Black Hills is the Chilson Member, which is Aptian in age (Post and Bell, 1961; Sames et al., 2010), ca. 126–113 Ma (Table 2). The Aptian–Albian Cedar Mountain Formation in northeastern Utah has been constrained with U-Pb dating of zircons to a maximum depositional age of 117–109 Ma (Burton et al., 2006) (Table 2). In the northern Uinta Basin in Utah, palynology indicates that the Dakota Formation is upper Albian (Currie et al., 2011, 2012). The Dakota Formation in south-central Utah, west of Glen Canyon City, is ca. 95 Ma (Kirschbaum and McCabe, 1992; Uličný, 1999) (Table 2). The Frontier Formation has been documented throughout Utah and Wyoming. North of Vernal, Utah, and near Flaming Gorge Reservoir, the sandstone deposits of the Frontier Formation are Turonian in age and are within the Watinoceras devonense to Prionocyclus germari (ca. 93.2–89 Ma) biozones (Cobban and Reeside, 1952; Cobban et al., 2006). In the type locality of the Frontier Formation in western Wyoming, north of the city of Frontier, and in eastern Wyoming, just west of Kaycee, the Frontier Formation is Cenomanian to Turonian in age and spans the Conlinoceras tarrantense to Prionocyclus germari (95.73 ± 0.61–89 Ma) biozones (Cobban and Reeside, 1952; Merewether et al., 1976; Cobban, 1990; Cobban et al., 2006) (Table 2). The Echo Canyon Conglomerate is Coniacian–Santonian in age. Palynological studies have produced ages between ca. 87 and 85 Ma (Jacobson and Nichols, 1982; DeCelles, 1994) (Table 2). Geological Society of America Bulletin, Month/Month 2014 5 Painter et al. central eastern Utah Sam 8 70 060923 80 85 90 95 051218 100 Stratigraphic age (Ma) western Colorado eastern Wyoming central Wyoming western South Dakota North Horn Fm. 051211 Almond Fm. 051210 Canyon Creek Mbr. Sam 18 lower and upper Sego Sandstone 051219 Rusty Mbr. Adaville Fm. Sam 17 Mbr. 060922 051209 Trail Mbr. 07.28.11 051208 051212 051207 051205 Lazeart SS. Mbr. Brooks Mbr. Adaville Fm. Rock Springs Fm. 051201 Echo Cangon Cgl. Chimney Rock Tongue lower Rock Springs Fm. basal Blair Fm. 051105 Frontier Fm. Dakota SS 051104 051206 Frontier Fm. Sam 13 75 western Wyoming Ericson Fm. southern Utah Price River Fm. 65 051106 Dakota SS 051107 Cedar Mtn. Fm. 051204 Kelvin Fm. Frontier Fm. 105 115 130 051102 051103 Morrison Fm. 051101 120 125 lower and upper Chilson Mbr. 110 Black text = sandstone sample Gray and underlined text = conglomerate cobble sample 051213 the A interval Cloverly Fm. 051214 Morrison Fm. 135 140 145 051108 Morrison Fm. 150 155 160 Figure 3. Graphical representation of the spatial and temporal distribution of samples within this study (Table 1). See Table 2 for detailed citations and for age uncertainties associated with depositional ages presented in the literature. A to A′ in Figure 2 is the direction in which samples are plotted. Detailed information on the age control is found in the text. Black text represents sandstone samples and gray text represents conglomerate cobble samples. In western Wyoming, the Upper Cretaceous Adaville Formation is ca. 82.5 Ma at its base (the Lazeart Sandstone Member), based on Scaphites hippocrepis I, and 81.86 ± 0.36 Ma at its top, based on Scaphites hippocrepis II (Miller, 1977; Roehler, 1990; Devlin et al., 1993; Krystinik and Blakeney DeJarnett, 1995; Cobban et al., 2006). Farther east, the Blair Formation near Rock Springs, Wyoming, is coeval with the Lazeart Sandstone Member, with an age of ca. 82.5 Ma (Scaphites hippocrepis I) (Smith, 1961; Gill et al., 1970; Roehler, 1990; Krystinik and Blakeney DeJarnett, 1995; Cobban et al., 2006) (Table 2). Both the Chimney Rock Tongue Member and the Brooks Member of the Rock Springs Formation, near Rock Springs, Wyoming, are early Campanian in age. The Chimney Rock Tongue Member is ca. 81.5 Ma, constrained by Scaphites hippocrepis III, and the overlying Brooks 6 Two-phase stratigraphic model (anti-tectonic) Thrust-Derived Proximal Distal Molasse Foreland Foreland Active Thrust Belt Subsidence Erosion reworked deposits Thrust Advance Cessation of Thrusting Inactive Thrust Belt Rebound Figure 4. Two-phase stratigraphic model as proposed by Heller et al. (1988). The model asserts that upward-coarsening sequences in the proximal foredeep represent active shortening and tectonism in the thrust belt. In contrast, it asserts that upward-coarsening sequences in the distal foreland are anti-tectonic, formed during times of tectonic quiescence and flexural rebound, and are reworked from proximal coarse-grained deposits. Geological Society of America Bulletin, Month/Month 2014 Exhumation of the North American Cordillera Figure 5. Stylized fold-thrust belt, foreland basin, and geoexhumation thermal gradient. Lag time (tL) tL = tc – td equals the difference between cooling depositional age t d the cooling age (t c ) and the age t c depo sitional age (t d ) (Garver ~60 °C apatite (U-Th-[Sm])/He et al., 1999). The white dashed ~120 °C apatite fission track lines show the approximate clo~180 °C zircon (U-Th-[Sm])/He sure temperature of different thermochronologic systems. The black dashed line represents a stylized exhumation pathway, and the red dot represents an apatite-bearing sample passing through its closure temperature, being exhumed, and then being deposited in the foreland basin. Member is ca. 81 Ma, constrained by Baculites sp. (weak flank ribs) (Smith, 1961; Gill et al., 1970; Roehler, 1990; Krystinik and Blakeney DeJarnett, 1995; Cobban et al., 2006) (Table 2). The Sego Sandstone Member of Mesaverde Group in the Book Cliffs area, Utah, overlies Baculites perplexus and has Baculites scotti in its upper part (ca. 78 Ma to 75.56 ± 0.11 Ma) (Gill and Hail, 1975; Cobban et al., 2006). In northwest Colorado, the age of the Sego Sandstone Member is less well understood than it is in the Book Cliffs area, Utah. Baculites perplexus has been identified below the Sego Sandstone Member in northwest Colorado, but no ammonite zone has been identified in the upper portions of the Sego Sandstone Member in northwest Colorado (Cullins, 1971; Molenaar and Wilson, 1993; Painter et al., 2013). However, in a detrital zircon U-Pb study, a single young zircon grain was dated at 76.6 ± 1.5 Ma (York, 2010), suggesting a similar age to the Sego Sandstone Member in the Book Cliffs area in Utah (Table 2). The Upper Campanian Ericson Formation, near Rock Springs, Wyoming, sampled in this study (Table 1; Figs. 2, 3), spans the biozones Baculites mclearni to Baculites reesidei (ca. 80 to 72.94 ± 0.45 Ma) (Gill et al., 1970; Martinsen et al., 1999; Cobban et al., 2006). However, the Ericson Formation consists of fluvial to estuarine deposits, and these biostratigraphic horizons are correlated along strike from nearby marine stratigraphy (Gill et al., 1970; Martinsen et al., 1999; Leary, 2011). The Trail Member of the Ericson Formation, its stratigraphically lowest member, spans the Baculites asperiformis to Baculites sp. (smooth) biozones (ca. 79 Ma). The overlying Rusty Member of the Ericson Formation has been correlated to the Baculites sp. (smooth) to Baculites perplexus biozones (ca. 78 Ma). The uppermost member of the Ericson Formation is the Canyon Creek Member, which has been correlated to the Didymoceras cheyennese to Baculites reesidei zones (74.67 ± 0.15 to 72.94 ± 0.45 Ma) (Gill et al., 1970; Martinsen et al., 1999; Cobban et al., 2006) (Table 2). In north-central Utah, Upper Cretaceous to Paleocene conglomerate deposits have been dated using palynology (Horton et al., 2004); the Castlegate–Price River Formation in the Charleston-Nebo salient in north-central Utah is mid- to upper Campanian (ca. 80–71 Ma) (Fouch et al., 1983; Horton et al., 2004). The overlying North Horn Formation is Maastrichtian–early Paleocene (ca. 70–61 Ma) (Horton et al., 2004) (Table 2). The upper Campanian to lower Maastrichtian Almond Formation, near Rock Springs, Wyoming, is correlated to Baculites jenseni to Baculites baculus biozones (ca. 72–71 Ma) (Gill et al., 1970; Martinsen et al., 1999; Cobban et al., 2006) (Table 2). METHODS Thirty-seven samples of conglomerate cobbles and sandstones were collected from proximal and distal Cordilleran foreland basin deposits (Table 1). Detrital zircon U-Pb geochronology was applied to all sandstone samples (Table 1). Zircon He thermochronology was applied to one conglomerate cobble sample, seven foreland basin sandstones, and one paleozoic sandstone exposed in the thrust belt (Table 1), and AFT thermochronology was applied to four conglomerate cobbles and seven sandstone samples (Table 1). All thirty-seven samples presented in this paper were collected from surface outcrops, and both the base and top of the selected stratigraphic units were sampled. Because of generally poor apatite yield in clasts and sandstones derived from Cordilleran quartzites, ~50 pounds (20 kg) were collected for each sandstone sample. All samples were processed to separate both zircons and apatites. Zircon and apatite crystals were extracted by standard mineral separation methods of crushing followed by separation by Wilfley table, Frantz magnetic separator, and heavy liquids. Every sample collected for this study produced zircons; however, only eleven samples produced apatites of suitable quality and quantity for AFT thermochronology. The paucity of apatite could be a result of low apatite content in the miogeoclinal Paleozoic source rocks, or it could indicate that apatite did not survive transport from the sourcing orogenic belt to the foreland basin because of mechanical and/or chemical weathering. U-Pb analysis on detrital zircon and detrital apatite, zircon He analysis, and AFT methods are explained below. More detailed information about laboratory procedures and analytical equipment can be found in the GSA Data Repository1 (Expanded Methods). Detrital Zircon and Apatite U-Pb Geochronology Zircon and apatite U-Pb ages were determined by laser ablation–multicollector–inductively coupled plasma mass spectrometry (LA-MC-ICPMS) at the Arizona LaserChron Center (Gehrels et al., 2006, 2008; Thomson et al., 2012). Twenty-two new detrital zircon samples were analyzed, producing 1874 new U-Pb ages. The analytical data are reported in the Data Repository (Table DR1). Uncertainties shown in these tables are at the one-sigma level and include only measurement errors. Analyses that are >20% discordant (by comparison of 206Pb/238U and 206Pb/207Pb ages) or >5% reverse discordant are not considered further (Gehrels, 2011). The closure temperature for U-Pb in apatite is 450–550 °C (Cherniak et al., 1991), classifying it as a medium-temperature thermochronometer. In quickly cooled volcanic rocks (e.g., ash-fall material), this temperature is attained at nearly the same time as the crystallization age and therefore yields an age near the crystallization age. Dates from metamorphic and plutonic rocks can also record metamorphic events and late-stage cooling of magmatic intrusions. In 1 GSA Data Repository item 2014223, which contains expanded methods, raw detrital zircon U-Pb data (Table DR1), raw apatite U-Pb data (Table DR 2), and concordia plots (Figure DR1), is available at http://www.geosociety.org/pubs/ft2014.htm or by request to editing@geosociety.org. Geological Society of America Bulletin, Month/Month 2014 7 8 Geological Society of America Bulletin, Month/Month 2014 Frontier Formation Echo Canyon Conglomerate Adaville Formation Rock Springs Formation Sego Sandstone Member: Mesaverde Group Ericson Formation Price River Conglomerate ca. 82.5 ca. 82.5 Western Wyoming South-central Wyoming Lazeart Sandstone Member Blair Formation 95.73 ± 0.61–89 95.73 ± 0.61–89 Western Wyoming Eastern Wyoming ca. 93.2–89 81.86 ± 0.36 Western Wyoming Upper Adaville ca. 87–85 ca. 81.5 South-central Wyoming Chimney Rock Tongue Member Eastern Utah ca. 81 South-central Wyoming Brooks Member North-central Utah ca. 78–76 ca. 79 South-central Wyoming Trail Member Northwest Colorado ca. 78 74.67 ± 0.15– 72.94 ± 0.45 South-central Wyoming South-central Wyoming ca. 80–71 ca. 70–61 ca. 72–71 Age (Ma) Rusty Member Canyon Creek Member North-central Utah North-central Utah North Horn Formation Location South-central Wyoming Almond Formation Formation/Member Equivalent stratigraphy Cenomanian–Turonian Cenomanian–Turonian Turonian Coniacian–Santonian Early Campanian Early Campanian Early Campanian Early Campanian Early Campanian Campanian Campanian Campanian Late Campanian Mid–late Campanian Maastrichtian– early Paleocene Late Campanian– Maastrichtian Geologic age Ammonites, Ar/Ar Ammonites, Ar/Ar Ammonites Palynomorphs Ammonites Ammonites Ammonites, Ar/Ar Ammonites Ammonites Stratigraphic correlations, ammonites, DZ U-Pb Stratigraphic correlations, ammonites Stratigraphic correlations, ammonites Stratigraphic correlations, ammonites, Ar/Ar Palynomorphs Palynomorphs Ammonites Data type TABLE 2. LATE JURASSIC TO LATE CRETACEOUS STRATIGRAPHIC AGES 25, 26, 27 25, 26, 27 25 28, 29 31, 33, 34, 35 30, 31, 32, 33 30, 31, 32, 33 30, 31, 32, 33 30, 31, 32, 33 36, 37, 38, 39 35, 40 35, 40 35, 40 41 41 35, 40 Source None None None 76.6 ± 1.5 None None 90.5 ± 2.0 N/A 84.3 ± 4.8 85.3 ± 1.3 b None None 72.1 ± 1.5 a N/A N/A None None None 91.5 ± 2.5 N/A 85.6 ± 4.1 87.2 ± 4.8 None None None None None None N/A N/A N/A None None None 94.0 ± 0.8 N/A 96.0 ± 0.8 96.9 ± 0.7 None None None None None None 72.9 ± 4.8 a N/A N/A None DZ young ages MDA (Ma) Youngest Average of Youngest grain young grains population (conitnued) 051104 051206 051105 051201 051207 051205 07.28.11 051212 051208 Sam 17 051209 051219 051210 060922, 060923 Sam 8 051211 Sample(s) Painter et al. ca. 126–112 Eastern Utah ca. 126–113 154.8 ± 0.6– 135.2 ± 5.5 154.8 ± 0.6– ca. 145 Central Wyoming Western South Dakota Eastern Utah Central Wyoming Chilson Mbr. of the Lakota Fm. ca. 139–126 117–109 Ma ca. 102 Eastern Utah Eastern Utah ca. 95 A interval Kelvin Fm. Location South-central Utah Age (Ma) 15 Ar/Ar, palynomorphs 3, 4 None None 154.2 ± 3.8 157.0 ± 3.2 None 136.3 ± 8.8 147.6 ± 5.9 155.3 ± 4.1 Kimmeridgian–Tithonian 4, 5, 6 Ar/Ar, K-Ar Kimmeridgian–Berriasian 051214 051108 051101, 051102 None None 16, 17, 18, 19, 20, 21 Palynomorphs Aptian 051213 None None 3, 11, 12, 13, 14, 15, 20 Valanginian–Barremian Palynomorphs 051204 118.0 ± 4.5 121.3 ± 3.2 117.2 ± 3.2 7, 8, 9, 10 051107 106.3 ± 2.8 107.3 ± 3.6 109.2 ± 2.5 051106 U-Pb on zircons None None None 22, 42, 43 Stratigraphic correlations, ammonites 051218 Sample(s) None 23, 24 None 94.5 ± 2.9 Source Data type Stratigraphic correlations, ammonites Stratigraphic correlations, ammonites Aptian–Albian Aptian–Albian Albian Cenomanian Geologic age DZ young ages MDA (Ma) Youngest Average of Youngest grain young grains population Geological Society of America Bulletin, Month/Month 2014 ca. 158–ca. 145 Depositional age st ea dy -st at e e co xhu ns m ta nt atio n la r g tim ate incre asing e exhu matio co n rat ns e ta nt la g tim e rate exhumation decreasing Western South Dakota Late Oxfordian– Palynomorphs, ostracodes, Tithonian (predominantly 1, 2 157.8 ± 6.6 160.2 ± 4.2 161.8 ± 3.3 051103 charophytes Kimmeridgian) Note: Stratigraphic ages of Late Jurassic–Paleocene sandstones to conglomerates that span Utah, Colorado, Wyoming, and South Dakota. Existing ages were gathered from literature, and the sources are given below. Absolute ages of certain biozones are all from Cobban et al. (2006), which is a compilation of previous biostratigraphic and Ar/Ar work. New constraints from detrital zircon (DZ) U-Pb dating, presented in this study, are shown also (asome DZ U-Pb grains from Leary [2011]; bDZ age from York [2010]). In the DZ age columns, “None” indicates that none were found during U-Pb analysis, and “N/A” indicates that these are conglomerate cobbles so no DZ analysis was done. MDA—maximum depositional age. Sources: 1 (Litwin et al., 1998); 2 (Schudack et al.,1998); 3 (DeCelles and Burden, 1992); 4 (Kowallis et al., 1991); 5 (Kowallis et al., 1998); 6 (Peterson, 1992); 7 (Crittenden, 1963); 8 (Hale and Van de Graaf, 1964); 9 (Kauffman, 1969); 10 (Ryer, 1977); 11 (DeCelles et al., 1993); 12 (Furer et al., 1997); 13 (O’Malley, 1994); 14 (Way, 1997); 15 (Burton et al., 2006); 16 (Waagé, 1959); 17 (Post and Bell, 1961); 18 (Dahlstrom and Fox, 1995); 19 (Way et al., 1998); 20 (Zaleha, 2006); 21 (Sames et al., 2010); 22 (Johnson, 2003); 23 (Kirschbaum and McCabe, 1992); 24 (B.S. Currie, 2013, personal commun.); 25 (Cobban and Reeside, 1952); 26 (Merewether et al., 1976); 27 (Cobban, 1990); 28 (Jacobson and Nichols, 1982); 29 (DeCelles, 1994); 30 (Miller, 1977); 31 (Roehler, 1990); 32 (Devlin et al., 1993); 33 (Krystinik and Blakeney DeJarnett, 1995); 34 (Smith, 1961); 35 (Gill et al., 1970); 36 (Gill and Hail, 1975); 37 (Cullins, 1971); 38 (Molenaar and Wilson, 1993); 39 (Painter et al., 2013); 40 (Martinsen et al., 1999); 41 (Horton et al., 2004); 42 (Currie et al., 2011); 43 (Currie et al., 2012). Morrison Formation Cloverly Formation Cedar Mountain Formation Dakota Formation Formation/Member Equivalent stratigraphy TABLE 2. LATE JURASSIC TO LATE CRETACEOUS STRATIGRAPHIC AGES (conitnued) Exhumation of the North American Cordillera Cooling age Figure 6. Three hypothetical lag-time trends and what they suggest about exhumation (Garver et al., 1999; Bernet et al., 2001). Decreasing lag times indicate an increase in exhumation, constant lag times indicate a steady-state exhumation rate, and increasing lag times indicate a decreasing exhumation rate. contrast to zircon, apatite is more difficult to date using U-Pb because apatite has much lower amounts of U, generally <100 ppm, and generally higher amounts of common lead. However, recent advances have improved U-Pb thermochronology of apatites (Carrapa et al., 2009; Thomson et al., 2012). Although the error is much higher in U-Pb analyses of apatite than of zircon, this technique can establish whether the crystallization and/or metamorphic age of an apatite grain is near the AFT cooling age of the same apatite grain, and can thus discriminate between magmatic ages versus exhumation ages. We followed the procedure developed and outlined by Thomson et al. (2012) to analyze U-Pb ages of apatite in seven detrital samples, targeting ten apatite grains (with the youngest individual AFT ages) from each sample, and the complete analytical results can be found in the Data Repository (Table DR2). Grains from the youngest AFT age population were targeted in an effort to test whether their ages record exhumation or timing of crystallization in the case of volcanogenic apatites. These apatites were mounted on slides next to 485 Ma apatite standards from Madagascar and NIST reference material glass, to correct for elemental fractionation. Although a large laser (>65 µm) spot size is recommended for apatite (Thomson et al., 2012), the grain size of the available apatites did not allow this use of a large spot size. Instead, a 40-µm-diameter laser was used on all but one 9 Painter et al. of the samples analyzed; the remaining sample was analyzed with a 25-µm-diameter laser because of its small apatite crystals. The resulting interpreted U-Pb ages are shown on Pb/U concordia diagrams and relative age-probability diagrams using the routines in Isoplot software (Ludwig, 2008). The age-probability diagrams show each age and its uncertainty (for measurement error only) as a normal distribution, and sum all ages from a sample into a single curve. Composite age-probability plots are made from an in-house Microsoft Excel program (see Analysis Tools at www.laserchron .org for link) that normalizes each curve according to the number of constituent analyses, such that each curve contains the same area, and then stacks the probability curves. Maximum depositional ages (MDAs) for detrital zircon U-Pb analyses were calculated using three methods (described by Dickinson and Gehrels, 2009); (1) the youngest grain was selected from each of the samples, (2) the average age of the youngest three zircons was calculated, and (3) the weighted mean of the youngest Gaussian distribution of three or more grains was calculated. All three of these calculations are presented in Table 2. All analytical data are reported in the Data Repository (Table DR1). Zircon (U-Th-[Sm])/He Thermochronology Zircon He analyses were conducted at the University of Arizona following the method described by Reiners (2005). Nine samples were analyzed for this study (Table 1; Figs. 2, 3). Three zircons from each sample were handpicked, and the dimensions of each crystal were measured to approximate crystal volume to ensure a tetragonal prism width of greater than 60 µm. Each crystal was then packed in a Nb foil tube and heated with a focused 10 µm beam of a 1064 nm Nd:YAG laser for 15 min intervals to degas the He content of the zircon. Typically two to three intervals are required to sufficiently degas the zircon. The gas extracted from the zircon was then spiked with approximately –0.1 to 1.0 pmol 3He and was cryogenically concentrated and purified. This gas mixture was then expanded and measured with a quadrupole mass spectrometer. The U and Th contents were then measured by isotope dilution and solution ICPMS (Reiners, 2005). Apatite Fission Track (AFT) Thermochronology Eleven samples were analyzed using AFT thermochronology (Table 1; Figs. 2, 3). Here we present data from two different sample types: 10 apatites from conglomerate cobble clasts, and detrital apatites from sandstones. Cobble clasts can be considered as basement samples and have a uniform time-temperature history, and for these samples, 20 apatite grains per sample were analyzed and a mean age is presented (where χ2 > 5%). For sandstone samples, 100 detrital apatite crystals were analyzed in order to capture the different source cooling signals of the catchment area; the software package BINOMFIT was used to identify different age populations (Galbraith and Green, 1990; Brandon, 2002), and we considered only populations containing more than five grains as significant. Unless the individual age populations are contaminated with volcanogenic apatites, these populations are generally assumed to be an exhumation signal; in particular, the youngest age population is generally assumed to be a source exhumation signal. RESULTS Detrital Zircon U-Pb Geochronology The primary purpose of measuring the age of detrital zircons with U-Pb techniques was to determine the MDA of the collected samples by independent methods. Furthermore, because of the wide geographic area that these samples represent, detrital zircon (DZ) U-Pb analyses help to assess whether the analyzed samples share a similar provenance history. The samples that were analyzed using DZ U-Pb are found in Table 1, and the raw data can be found in the Data Repository (Table DR1). Two samples from previous work (York, 2010) with 200 individual zircon ages are included here together with four zircon ages from Leary (2011). In Table 2, we present how these DZ U-Pb ages compare to the existing stratigraphic age control determined from biostratigraphy and 40Ar/39Ar ages of bentonites. Figure 7 is a probability density plot of detrital zircons in each sample <200 Ma, and the youngest single zircon in each sample is listed as the MDA. Three samples from the Morrison Formation in Utah (sample 051108), Wyoming (sample 051214), and South Dakota (sample 051103) were analyzed (Fig. 7). In both Utah and Wyoming, the samples were taken from fluvial deposits. In South Dakota, the Morrison Formation is predominantly lacustrine. A weighted mean of the youngest statistically separable population of zircons for the Utah sample produced a Late Jurassic (Kimmeridgian) MDA of 155.3 ± 4.1 Ma. Sample 051214 from Wyoming does not have a young population with the requisite number of zircons (more than three); however, it does contain two young grains with an average MDA of 157.0 ± 3.2 Ma, which is consistent with sample 051108 from Utah. Sample 051103 from South Dakota has a young population with a weighted mean and Late Jurassic (Oxfordian) MDA of 161.8 ± 3.3 Ma. In all cases, these samples produce a Late Jurassic MDA (Oxfordian–Kimmeridgian). Four samples from the Lower Cretaceous Cloverly Formation, and its equivalents, were analyzed from Utah (sample 051204), Wyoming (sample 051213), and South Dakota (samples 051101 and 051102) (Fig. 7). Sample 051204 from Utah is from the Kelvin Formation, which is equivalent to the Cloverly Formation. The weighted mean of the youngest statistically separable population of zircons in the sample from Utah produced an Early Cretaceous (Aptian) MDA of 121.3 ± 3.2 Ma. A single young zircon in this sample is 117.2 ± 2.4 Ma, but this is not a statistically robust population. Sample 051213 from the A interval of the Cloverly Formation in Wyoming contained no young, syndepositional zircons. Two samples (051101 and 051102) from the Chilson Member of the Lakota Formation (Cloverly Formation equivalent) in South Dakota were analyzed; however, no syndepositional zircons are present. One sample from the Lower Cretaceous Cedar Mountain Formation (sample 051107) in Utah, also equivalent to the Cloverly Formation, was sampled. The weighted mean of the youngest population of zircons produced an Early Cretaceous (Albian) MDA of 109.2 ± 2.5 Ma (Fig. 7). Two samples (samples 051218 and 051106) from the Lower to Upper Cretaceous Dakota Formation were collected in Utah, one from south-central Utah and the other from northeast Utah (Fig. 7). Neither of these samples has a population of more than three young zircons to calculate a weighted mean. However, the sample from south-central Utah (051218) contained one young zircon with the age of 94.5 ± 2.9 Ma, suggesting a Late Cretaceous (Cenomanian) MDA. Three samples from the Upper Cretaceous Frontier Formation were collected and analyzed, one from Utah (sample 051105) and two from Wyoming (samples 051206 and 051104). In Wyoming, sample 051206 was collected from the western part of the state, and sample 051104 was collected from the eastern side in the Powder River Basin (Fig. 7). The weighted mean of the youngest zircon population in sample 051105 from Utah is 94.0 ± 2.9 Ma, producing a Late Cretaceous (Cenomanian–Turonian) MDA. However, there are younger grains in this population that do not form a statistically separable peak. The average of the three youngest grains is 91.5 ± 2.5 Ma, suggesting a Turonian MDA. Neither of the Wyoming samples yielded young, syndepositional zircons. Geological Society of America Bulletin, Month/Month 2014 Exhumation of the North American Cordillera Wyoming Utah-Colorado 051211 Almond Fm. 051210 Canyon Creek Mbr. 051219 Rusty Mbr. 051209 Trail Mbr. n=100 Sam 18 upper Sego Sandstone Mbr. n=100 MDA=76.6±1.5 Sam 17 lower Sego Sandstone Mbr. n=83 n=79 051208 n=90 051212 Brooks Mbr. Rock Springs Fm. n=89 Chimney Rock Tongue lower Rock Springs Fm. 07.28.11 Adaville Fm. n=87 MDA=84.3±4.8 Ma 051207 basal Blair Fm. 051205 Lazeart SS. Mbr. Adaville Fm. n=80 MDA=85.3±1.3 Ma n=86 MDA=90.5±2.0 Ma 051105 Frontier Fm. n=86 MDA=94.5±2.9 Ma 051218 Dakota Fm. n=71 MDA=106.3±2.8 Ma 051107 n=87 MDA=117.2±3.2 Ma n=77 †MDA=147.6±5.9 Ma 0 50 100 Age (Ma) n=80 n=86 051104 051206 Frontier Fm. Cedar Mtn. Kelvin Fm. 051204 051108 Ericson Fm. n=87 n=87 MDA=72.1±1.5 Ma n=87 maximum depositional age=MDA n=number of single zircon ages in sample South Dakota Morrison Fm. 150 the A interval Cloverly Fm. 051213 n=84 MDA=154.2±3.8 Ma 051214 n=84 200 0 50 100 Age (Ma) Morrison Fm. 150 lower and upper n=88 051101 Chilson Mbr. n=89 051102 n=97 MDA=157.8±6.6 Ma 051103 Morrison Fm. 200 0 50 100 Age (Ma) 150 200 Figure 7. Probability density plots of all young detrital zircon (DZ) U-Pb analyses (0–200 Ma) presented here. See Table 1 for a comprehensive list of all the samples with DZ U-Pb. All curves are normalized to one another. Samples Sam 18 and Sam 17 come from York (2010). All the other samples are new. Where applicable, maximum depositional age (MDA) is given (see Table 2 for more detailed MDA information); n is the number of zircon grains analyzed from each whole sample (excluding those grains that have been filtered out given quality assurance standards). All data can be found in Table DR1 in the Data Repository [see footnote 1]. Two samples (051205 and 07.28.11) of the Upper Cretaceous Adaville Formation in western Wyoming were analyzed (Fig. 7), one from the Lazeart Sandstone Member and one in the upper Adaville Formation. The Lazeart Sandstone Member sample (051205) has three young zircons with an average age of 87.2 ± 2.2 Ma, suggesting a Late Cretaceous (Coniacian–Santonian) MDA. However, these three grains do not represent a statistically separable and robust population from which a weighted mean can be calculated. The sample from the upper Adaville Formation did not yield any young, syndepositional zircons. Three samples from the Rock Springs Formation in Wyoming were analyzed, one from the basal Blair Formation (sample 051207), one from the Chimney Rock Tongue Member (sample 051212), and one from the Brooks Member (sample 051208) (Fig. 7). Young zircons in the age range of 84.3–89.0 Ma are present in the Blair Formation sample, but they are overwhelmed by 90–98 Ma zircons and do not produce a statistically separable peak. However, three young zircons produced an average age of 85.6 ± 4.1 Ma, consistent with a Late Cretaceous (Santonian) MDA. The samples from the Chimney Rock Tongue Member and the Brooks Member did not yield young, syndepositional age zircons. Three samples from the Upper Cretaceous (Campanian) Ericson Formation in Wyoming were analyzed. Also, two samples from the Campanian Sego Sandstone Member of the Mesa Verde Group in northwest Colorado from York (2010) are presented here. Out of the Trail Member, Rusty Member, and Canyon Creek Member of the Ericson Formation, only the Canyon Creek Member (sample 051210) yielded young, near syndepositional age zircons, sample 051210, with an age of 73.3 ± 5.1 Ma. However, a sample presented in Leary (2011) from the Canyon Creek Member of the Ericson Formation in the same general geographic area yielded five ca. 73 Ma grains, which have been included in this data set in order to calculate a weighted mean MDA; those grains have suffixes of “rl1– rl5” in the data file in the Data Repository (Table DR1). The combined grains have a Late Campanian MDA of 72.9 ± 0.8 Ma (Fig. 7). One of the Sego Sandstone Member samples (Sam 17) contained one young zircon of 76.6 ± 5.1 Ma. However this is a single age and is not the more robust weighted mean of a population or the average of three young grains. One sample from the Upper Cretaceous Almond Formation in Wyoming was analyzed (sample 051211) but did not contain any young zircons with nearly syndepositional ages (Fig. 7). All of the calculated MDAs have been compared to existing depositional ages based on biostratigraphy and 40Ar/39Ar ages of bentonites (Table 2). In an effort to compare provenance of all the samples analyzed, a second probability density plot is presented (Fig. 8). In this prob- Geological Society of America Bulletin, Month/Month 2014 11 Wopmay Trans-Hudson Yavapai Mazatzal 3200 3000 2800 2600 2400 2200 2000 1800 1600 1.48–1.34 Ga magmatics 1400 1200 Grenville orogen 1000 800 Morrison Fm. 051214 0 3600 3400 3200 3000 2800 2600 2400 2200 2000 1800 1600 Age (Ma) the A interval 051213 Cloverly Fm. 051205 Lazeart SS. Mbr. Adaville Fm. 051104 Frontier Fm. 051206 basal Blair Fm. 200 051207 07.28.11 Adaville Fm. 400 Brooks Mbr. Rock Springs Fm. Chimney Rock Tongue 051212 lower Rock Springs Fm. 600 Peri-cratonic orogens Cordilleran magmatism 051208 Trail Mbr. 051209 051219 051210 Canyon Creek Mbr. 051211 Almond Fm. Ericson Fm. WYOMING Peri-cratonic orogens 1400 1200 1000 800 600 400 Sam 17 1.48–1.34 Ga magmatics Grenville orogen 051108 Morrison Fm. 0 3600 3400 3200 3000 2800 2600 2400 2200 2000 1800 1600 1400 1200 1000 800 Peri-cratonic orogens 600 Peri-cratonic orogens Cordilleran magmatism 400 200 0 12 Age (Ma) Wopmay 051105 Frontier Fm. 051106 Dakota SS 051218 051107Cedar Mtn. Fm. 051204 Kelvin Fm. lower Sego Sandstone Mbr. upper Sego Sandstone Mbr. Archean crust Trans-Hudson Yavapai Mazatzal Sam 18 UTAH-COLORADO 200 Figure 8. Probability density plots (PDPs) of pre-Sevier detrital zircon U-Pb ages (>160 Ma) to assess provenance. In these PDP curves, grains younger than 160 Ma (coeval with the Sevier orogeny) are excluded. All of the curves were then re-normalized and stretched uniformly along the vertical axis to make peaks more visible. Orogenic province ages are from Whitmeyer and Karlstrom (2007) and Gehrels et al. (2011). SOUTH DAKOTA Archean crust 3600 3400 Age (Ma) lower and upper Chilson Mbr. 051101 051102 Morrison Fm. 051103 Painter et al. ability density plot, all grains younger than 160 Ma, near the onset of the Sevier orogeny (DeCelles, 2004), are excluded in order to eliminate magmatic and volcanogenic synorogenic zircons and instead isolate zircons exhumed from the Paleozoic strata in the Sevier foldthrust belt and its hinterland region (Dickinson and Gehrels, 2008; Gehrels et al., 2011). The data were then renormalized and uniformly stretched vertically to make peak age differences more apparent (Fig. 8). The amplitude of some of the peaks varies (e.g., the 1.6–1.8 Ga peak); however, the presence of peak age clusters is similar throughout the 24 samples (Fig. 8), and no significant trends are evident. Zircon (U-Th-[Sm])/He Thermochronology In order to identify the most effective thermochronometer able to record cooling related to source exhumation in the North America Cordillera, nine samples from the Sevier fold-thrust belt and Cordilleran foreland were analyzed with zircon He thermochronology. These samples include Paleozoic strata in the fold-thrust belt itself, conglomerate cobbles of wedge-top deposits, and detrital samples in the proximal to distal foreland basin. Three zircons from each sample were picked and dated, except for sample Sam 11, from which only two zircons were dated. Complete data from these analyses can be found in Table 3. Sample Sam 11 is from the Inkom Formation, a Proterozoic quartzite from the Canyon Range Culmination in the Canyon Range, Utah (DeCelles et al., 1995) (Table 1; Fig. 2). The two zircon He ages are 22.8 ± 0.5 and 139.7 ± 3.1 Ma (Table 3; Fig. 9). Samples Sam 19, Sam 16, and Sam 15 are detrital samples from the Upper Cretaceous Castlegate Formation in both Utah and northwest Colorado (Table 1; Figs. 2, 3). Sample Sam 19 produced three zircon He ages, 348.7 ± 13.7, 396.3 ± 14.3, and 152.2 ± 6.2 Ma. Sample Sam 16 records three ages, 64.5 ± 5.1, 249.5 ± 9.5, and 357.2 ± 15.2 Ma. Sample Sam 15 records three ages, 96.0 ± 5.2, 125.8 ± 5.5, and 177.4 ± 6.7 Ma (Table 3; Fig. 9). Sample Sam 17 is a sandstone sample from the Upper Cretaceous Sego Sandstone Member of the Mesaverde Group in northwest Colorado (Table 1; Figs. 2, 3). It produced three zircon He ages that are 84.0 ± 3.6, 347.6 ± 12.1, and 506.9 ± 20.7 Ma (Table 3; Fig. 9). Two samples from the Upper Cretaceous Price River Formation were analyzed, one sandstone and one conglomerate cobble (Table 1; Figs. 2, 3). The sandstone sample, Sam 13, produced three zircon He ages that are 97.3 ± 3.8, 141.1 ± 4.8, and 272.4 ± 8.6 Ma. The con- Geological Society of America Bulletin, Month/Month 2014 Stratigraphic unit North Horn Formation North Horn Formation North Horn Formation North Horn Formation North Horn Formation North Horn Formation Sego Sandstone Member Sego Sandstone Member Sego Sandstone Member Price River conglomerate Price River conglomerate Price River conglomerate Price River conglomerate Price River conglomerate Price River conglomerate Castlegate Formation Castlegate Formation Castlegate Formation Castlegate Formation Castlegate Formation Castlegate Formation Castlegate Formation Castlegate Formation Castlegate Formation Inkom Formation Inkom Formation TABLE 3. ZIRCON (U-Th-[Sm])/He DATA Mass Half-width U Sample type (μg) (μm) (ppm) Detrital 2.93 45.50 538.71 Detrital 0.63 28.50 527.40 2.87 45.00 705.73 Detrital 0.97 31.50 62.83 Detrital 1.07 35.25 290.09 Detrital Detrital 0.70 29.00 430.94 Detrital 2.56 43.50 209.77 Detrital 1.60 38.50 303.33 Detrital 5.03 41.25 24.46 Conglomerate cobble 2.10 41.25 99.32 Conglomerate cobble 2.78 43.25 192.13 Conglomerate cobble 3.39 44.25 293.47 Detrital 15.68 79.50 394.60 Detrital 1.75 34.25 261.95 Detrital 5.81 52.00 17.93 Detrital 0.39 23.75 211.81 Detrital 0.54 26.75 226.65 Detrital 0.46 24.75 172.01 Detrital 1.06 33.50 78.04 Detrital 32.25 0.95 297.05 Detrital 26.25 0.83 235.06 Detrital 42.25 2.51 165.95 Detrital 1.30 36.00 251.26 Detrital 1.75 37.00 113.72 Paleozoic strata 47.75 55.14 5.65 Paleozoic strata 6.46 45.50 117.77 Th (ppm) 228.04 206.64 280.44 47.95 318.99 176.78 191.51 82.98 7.89 59.38 101.20 117.50 195.61 159.46 51.27 63.03 127.73 149.86 75.69 88.29 109.07 106.45 98.67 76.20 39.34 59.46 4 He (nmol/g) 451.40 509.49 382.93 67.11 82.38 199.16 469.66 116.95 73.11 34.57 278.69 376.27 318.76 129.00 42.91 85.70 141.98 171.85 120.91 594.94 64.77 405.53 200.35 241.61 6.17 78.16 Ft 0.76 0.63 0.76 0.66 0.68 0.64 0.75 0.72 0.76 0.74 0.75 0.76 0.86 0.70 0.79 0.57 0.61 0.58 0.67 0.67 0.63 0.75 0.70 0.69 0.78 0.78 Corrected age (Ma) 154.08 184.63 105.71 185.90 56.68 99.86 347.55 84.04 506.85 76.18 253.12 231.14 141.09 97.32 272.39 95.95 125.76 177.35 249.49 357.16 64.47 396.34 152.23 348.72 22.82 139.69 Analytical error ± 2σ (m.y.) 5.64 7.63 3.77 8.12 2.03 3 .9 7 12.14 3.59 20.74 2.58 8.42 7.73 4.81 3 .7 9 8.56 5.15 5.45 6.71 9.54 15.20 5.08 14.27 6 .1 7 13.65 0.50 3.14 Note: Sample type identifies whether the sample was a sandstone (i.e., detrital), a conglomerate cobble, or Paleozoic strata in the thrust belt. Mass is the mass of the zircon, and half-width is the half width of the zircon (one dimension used to approximate volume). Ft is the fraction of 4He retained within the crystal based on Farley et al. (1996). Sample name– zircon grain number Sam 7-z1 Sam 7-z2 Sam 7-z3 Sam 5-z1 Sam 5-z2 Sam 5-z3 Sam 17-z1 Sam 17-z2 Sam 17-z3 Sam 3-z1 Sam 3-z2 Sam 3-z3 Sam 13-z1 Sam 13-z2 Sam 13-z3 Sam 15-z1 Sam 15-z2 Sam 15-z3 Sam 16-z1 Sam 16-z2 Sam 16-z3 Sam 19-z1 Sam 19-z2 Sam 19-z3 Sam 11-z1 Sam 11-z2 Exhumation of the North American Cordillera glomerate cobble sample, Sam 3, recorded three ages that are 76.2 ± 2.6, 231.1 ± 7.7, and 253.1 ± 8.4 Ma (Table 3; Fig. 9). Two sandstone samples from the Upper Cretaceous North Horn Formation from Utah were analyzed, samples Sam 5 and Sam 7 (Table 1; Figs. 2, 3). Sample Sam 5 records three ages that are 56.7 ± 2.0, 99.9 ± 4.0, and 185.9 ± 8.1 Ma. Sample Sam 7 records three ages that are 105.7 ± 3.8, 154.1 ± 5.6, and 184.6 ± 7.6 Ma. All of the zircon He ages are plotted against their stratigraphic age in Figure 9 (Table 3). Apatite Fission Track Thermochronology Four samples from conglomerate cobbles (051201, 060922, 060923, and Sam 8) and seven samples from sandstone samples from foreland basin strata (051204, 051207, 051208, 051212, 051218, Sam 17, and NSD4 B) (Tables 1, 4) were analyzed with AFT thermochronology. These data are presented in stratigraphic order below. Sample 051204 is a sandstone sample from the Lower Cretaceous Kelvin Formation in north-central Utah (near Rockport Reservoir) (Table 1; Figs. 2, 3). Because of poor apatite yield and quality, only 30 apatite grains were available to be analyzed for AFT in this sample, instead of the desired 100 grains per detrital sample. The individual grain cooling age distribution ranges from 34.0 to 247.2 Ma (Table 5). Two populations are identified with BINOMFIT (Brandon, 2002), one of 52.1 ± 11.9/9.7 Ma and one of 122.9 ± 12.2/11.7 Ma (Table 5). However, we reject the 52.1 Ma population (Table 5; Figs. 10, 11) because it is based on <5 grains, its distribution does not appear to be Gaussian in the probability-density plot, and it is younger than the depositional age. Another interpretation for the 52.1 Ma age population is that this sample has been partially reset by post-depositional burial; however, given the magnitude of subsidence and stratigraphic thickness for the area, we consider partial resetting unlikely. We report 122.9 ± 12.2/11.7 Ma as the youngest population in Table 5. One hundred grains from sample 051218, from the Dakota Formation, were analyzed. Three binomial-fit peak ages are 88.8 ± 7.0/6.5 Ma, 155.6 ± 13.6/12.6 Ma and 310.3 ± 35.5/32.0 Ma (Table 5; Figs. 10, 11). Twenty grains from a conglomerate cobble (sample 051201) from the Echo Canyon Conglomerate were analyzed, producing a central age of 90.5 ± 14.0 Ma. The χ2 probability for this population is 99.98%, indicating that this sample is represented by a single age population, sharing the same cooling history (Table 4; Figs. 10, 11). Geological Society of America Bulletin, Month/Month 2014 13 Painter et al. zircon (U-Th-[Sm])/He cooling age (Ma) 0 100 60 300 400 500 600 Legend North Horn Fm. (Sam 7 detrital) North Horn Fm. (Sam 5 detrital) Price River Fm. (Sam 3 cobble) Sego SS Mbr. (Sam 17 detrital) Price River Fm. (Sam 13 detrital) Castlegate Fm. (Sam 19 detrital) Castlegate Fm. (Sam 15 detrital) Castlegate Fm. (Sam 16 detrital) Inkom Fm. (Sam 11 Proterozoic quartzite) 65 depositional age (Ma) Figure 9. Depositional age versus zircon (U-Th-[Sm])/He data. Detailed (U-Th-[Sm])/He data are reported in Table 3. Note the discordant ages of the nondetrital samples (i.e., Sam 3 and Sam 11), which indicate that the zircon (U-Th-[Sm])/He system was not fully reset. Also note that there is a break in the y axis to accommodate the plotting of the Proterozoic sample, Sam 11. 200 e 10 Myr lag tim e 0 Myr lag tim 55 70 75 80 85 PC One hundred grains from sample 051207, from the Blair Formation in Wyoming, were analyzed (Table 4). Three binomial-fit peak ages were identified, 85.6 ± 9.7/8.7 Ma, 162.1 ± 50.6/38.7 Ma, 271.9 ± 147.0/96.1 Ma. These three ages are reported in Table 5 (Figs. 10, 11). One hundred grains from sample 051212, from the Chimney Rock Tongue Member of the Rock Springs Formation in Wyoming, were analyzed. They produced three binomial-fit peak ages, 90.3 ± 5.5/5.2 Ma, 172.0 ± 18.0/16.3 Ma, and 454.9 ± 121.1/96.3 Ma (Table 5; Figs. 10, 11). One hundred grains from sample 051208, from the Brooks Member of the Rock Springs Formation in Wyoming, produced three binomial-fit peak ages, 33.9 ± 21.2/13.3 Ma, 112.0 ± 6.2/5.9 Ma, and 327.7 ± 51.0/44.3 Ma. The youngest peak age of 33.9 Ma was rejected because it is based on three grain ages, which statistically are not enough to constitute a robust population (Table 4; Figs. 10, 11). Two conglomerate cobble samples from the Price River Formation were analyzed. Twenty grains from sample 060922, from the lower Price River Formation, have a central age of 79.8 ± 6.3 Ma. This population has a χ2 probability of 79.2%. Twenty grains from sample 060923, from the upper Price River Formation, have a central age of 74.5 ± 6.3 Ma. This population has 14 a χ2 probability of 70.8%. The high χ2 probability of both of these samples suggests that they are composed of single populations, sharing the same cooling history (Table 4; Figs. 10, 11). One hundred grains from the lower Sego Sandstone Member (sample NSD4 B) of the Mesaverde Group produced three binomialfit peak ages of 66.6 ± 7.3/6.6 Ma, 111.9 ± 11.0/10.1 Ma, and 382.2 ± 46.4/41.5 Ma. One hundred grains from the upper Sego Sandstone Member, sample Sam 17, produced three binomial-fit peak ages, 66.6 ± 6.0/5.5 Ma, 110.7 ± 22.5/18.7 Ma, and 204.3 ± 47.3/38.6 Ma; however, the 204.3 Ma peak consisted of <5 grains and was rejected (Table 5; Figs. 10, 11). Twenty grains from a conglomerate cobble sample, Sam 8, from the North Horn Formation produced a central age of 66.1 ± 6.2 Ma. These ages have a χ2 probability of 30.6%, which indicates it is a single population (Table 4; Figs. 10, 11). Detrital Apatite U-Pb Thermochronology In order to interpret the youngest cooling age population in detrital AFT analysis as a source exhumation signal, it is important to ensure that these apatites are not young volcanogenic apatites derived from the Cordilleran magmatic arc. To address this issue, apatite grains from the youngest age populations, P1, were targeted from each of the seven detrital AFT samples (Table 5) for apatite U-Pb thermochronology. At least ten grains were selected from the P1 population from each sample. All of the data and concordia diagrams from these U-Pb apatite ages can be found in the Data Repository (Table DR2, Figure DR1). We compare all of these apatite U-Pb ages to the sample’s depositional age, the AFT P1 age, and the individual AFT grain ages (Table 6). Nine apatite grains from 051204, a sample from the Lower Cretaceous Kelvin Formation in Utah, were dated with U-Pb thermochronology. The small grain size of these apatites required a 25 µm laser diameter, instead of the preferred 40 µm diameter laser used on all of the other samples. This increased the error on each analysis and makes some grains plot off of concordia. Grain ages range from 134.3 ± 21.3 to 892.1 ± 23.6 Ma; six of the nine apatites are >160 Ma, whereas the other three are <160 Ma (Table 6). Nine apatite grains from sample 051218, from the Dakota Formation in south-central Utah, produced reliable U-Pb ages ranging from 320.6 ± 6.7 to 1602.0 ± 17.0 Ma. All nine apatites are older than the youngest AFT P1 of 160 Ma, and most are Proterozoic in age (Table 6). Eight apatite grains from sample 051207, from the Cedar Mountain Formation in Utah, Geological Society of America Bulletin, Month/Month 2014 TABLE 4. SAMPLES WITH APATITE FISSION TRACK DATA Number of Induced ρi Dosimeter ρd P(χ2) Central age ± 1σ Spontaneous ρs Sample Latitude Longitude Stratigraphic unit Sample type grains (× 106 cm–2) [Ns ] (× 106 cm–2) [Ni ] (× 106 cm–2) [Nd ] (%) (Ma) Conglomerate North Horn Sam 8 N40.20167 W108.86312 20 1.58 [203] 4.66 [599] 1.31 30.6 66.1 ± 6.2 cobble Formation Sego Sandstone Sam 17 N40.20236 W108.86123 Detrital 100 0.919 [3186] 2.70 [9374] 1.36 [9253] 0.0 80.2 ± 6.8 Member Sego Sandstone NSD4 B N40.17529 W108.82601 Detrital 100 0.923 [2064] 2.43 [5442] 1.68 [9253] 0.0 119.3 ± 12.1 Member Price River Conglomerate 060923 N39.96532 W111.47127 20 1.52 [193] 5.17 [658] 1.73 70.8 74.5 ± 6.4 cobble Formation Price River Conglomerate 060922 N39.96674 W111.47218 20 2.06 [240] 6.46 [752] 1.71 79.2 79.8 ± 6.3 Formation cobble Brooks 051208 N41.35810 W108.93082 Detrital 100 0.686 [1521] 1.55 [3444] 1.50 [6202] 0.0 128.7 ± 8.8 Member Chimney Rock 051212 N41.39890 W108.93394 Detrital 100 0.582 [1685] 1.50 [4354] 1.63 [6202] 0.0 123.4 ± 8.5 Tongue Member 051207 N41.48659 W108.96523 Blair Formation Detrital 100 0.643 [1122] 1.47 [2568] 1.46 [6202] 0.0 130.3 ± 9.8 Echo Canyon Conglomerate 051201 N40.96344 W111.41634 20 0.640 [62] 1.641 [159] 1.27 99.98 90.5 ± 14.0 Conglomerate cobble Dakota 051218 N37.11554 W111.85088 Detrital 100 1.01 [2076] 2.38 [4925] 1.76 [6202] 0.0 149.2 ± 10.1 Formation Kelvin 051204 N40.76712 W111.40012 Detrital 30 0.759 [327] 1.87 [806] 1.37 [6202] 0.4 105.7 ± 10.2 Formation Note: All samples with apatite fission track thermochronology. In all conglomerate cobbles, 20 grains were analyzed. In detrital samples, 100 grains were analyzed, except for in sample 051204 where only 30 apatite grains were analyzed because of the low apatite yield. ρs is the spontaneous track density, and Ns is the number of spontaneous tracks counted. ρi is the induced track density on the external detector (muscovite), and Ni is the number of induced tracks counted. Nd and ρd are the number of tracks and density of tracks calculated from the CN-5 dosimeter glass. P(χ2) is the χ2 probability. Fission-track ages were calculated using a weighted mean zeta calibration factor (Hurford and Green, 1983) based on IUGS age standards (Durango and Fish Canyon Tuff apatites). The ζ for C.S. Painter is 367.7 ± 14.1 (± 2σ); ζ is a factor that accounts for analyst bias in fission track counting for apatite fission track thermochronology. Bold ages in the central age column indicate that it is from a conglomerate cobble, and is the only age population for the sample. Exhumation of the North American Cordillera produced ages ranging from 89.0 ± 10.8 to 1869.0 ± 159.5 Ma. Although one grain is Proterozoic in age, the other seven are all approximately Jurassic and younger (Table 6). Two samples from the Rock Springs Formation, near Rock Springs, Wyoming, were analyzed; one from the lower Chimney Rock Tongue Member (sample 051212) and the other from the overlying Brooks Member (sample 051208). Ten grains from the Chimney Rock Tongue Member produced ages that range from 100.2 ± 10.7 to 1571.2 ± 22.6 Ma. Only one grain (1571.2 ± 22.6 Ma) is older than Late Jurassic age. Eight grains from the Brooks Member produced a range of ages of 83.7 ± 6.0 to 143.3 ± 31.7 Ma, indicating that all of the grains are Early Cretaceous and younger in age (Table 6). Two samples, NSD4 B and Sam 17, from the Upper Cretaceous Sego Sandstone Member in northwest Colorado, were analyzed. Nine apatite grains from NSD4 B produced ages ranging from 89.2 ± 59.0 to 1687.4 ± 41.9 Ma. Although two of the nine grains are >160 Ma, the rest are all <120 Ma. Ten apatite grains from Sam 17 have U-Pb ages of 85.0 ± 7.5 to 867.2 ± 17.5 Ma. Two of the ten grains are older than the young Cordilleran arc magmatic signal (i.e., >160 Ma); however, the other eight grain ages are all <160 Ma (Table 6). DISCUSSION Zircon U-Pb Geochronology and Biostratigraphy Out of 22 samples analyzed using DZ U-Pb, 10 yielded zircon U-Pb ages that are near syndepositional age, thus producing an MDA that represents the stratigraphic age of the sampled strata. The extent of biostratigraphic work conducted in the Cretaceous western U.S.A. is vast, and DZ analysis is an independent test of precision and accuracy of the biostratigraphic ages (Table 2; Fig. 12), thus testing the validity of stratigraphic correlations. The MDAs presented in this study are mostly concordant with the stratigraphic ages derived from biostratigraphy and 40Ar/39Ar age on bentonite beds (Table 2; Fig. 12). Where there is slight disagreement between the results of the different methods (e.g., an MDA that is younger than the accepted biostratigraphic age), the ages are within error of one another (Table 2; Fig. 12). For example, the youngest zircon in sample 051107, a sample from the Lower Cretaceous Cedar Mountain Formation in eastern Utah, is 106.3 ± 2.8 Ma, whereas the accepted biostratigraphic age is 117–109 Ma; however, 106.3 ± 2.8 Ma is within error of 109 Ma (Table 2; Fig. 12). These results also indicate that DZ U-Pb analysis can be Geological Society of America Bulletin, Month/Month 2014 15 Painter et al. TABLE 5. DETAILED APATITE FISSION TRACK DATA—ALL POPULATIONS Stratigraphic age FT age range P1 P2 P3 P4 Sample Stratigraphic unit (Ma) N (Ma) (Ma) (Ma) (Ma) (Ma) North Horn 66.1 ± 6.2 Sam 8 65.5 ± 4.5 20 39.6–143.0 N/A N/A N/A Formation [100%] Sego Sandstone 66.6 ± 6.0/5.5 110.7 ± 22.5/18.7 Sam 17 73 ± 1.5 100 34.2–268.4 xx xx Member [72.0%] [24.9%] Sego Sandstone 66.6 ± 7.3/6.6 111.9 ± 11.0/10.1 382.2 ± 46.4/41.5 NSD4 B 76.6 ± 1.5 100 40.9–901.7 xx Member [33.1%] [52.2%] [14.7%] Price River 74.5 ± 6.3 060923 77 ± 2 20 43.9–147.3 N/A N/A N/A Formation [100%] Price River 79.8 ± 6.3 060922 78 ± 2 20 51.6–161.6 N/A N/A N/A Formation [100%] 112.0 ± 6.2/5.9 327.7 ± 51.0/44.3 051208 Brooks Member 81 ± 3 100 25.0–624.6 xx xx [82.8%] [13.9%] Chimney Rock Tongue 90.3 ± 5.5/5.2 172.0 18.0/16.3 454.9 ± 121.1/96.3 051212 81.5 ± 1 100 39.6–782.6 xx Member [64.2%] [31.1%] [4.7%] Blair 85.6 ± 9.7/8.7 162.1 ± 50.6/38.7 271.9 ± 147.0/96.1 xx 051207 82.5 ± 1 100 39.6–1459.4 Formation [52.8%] [37.4%] [8.8%] Echo Canyon 90.5 ± 14.03 051201 86 ± 1 20 58.1–153.9 N/A N/A N/A Conglomerate [100%] Dakota 88.8 ± 7.0/6.5 155.6 ± 13.6/12.6 310.3 ± 35.5/32.0 051218 94.5 ± 2.9 100 43.9–579.0 xx Formation [35.2%] [46.4%] [18.4%] Kelvin 122.9 ± 12.2/11.7 051204 117.2 ± 3.2 30 34.0–247.2 xx xx xx Formation [78.1%] Note: Binomial-fit peak ages (P1 –P4 ) are as determined with BINOMFIT (Brandon, 2002) and are indicated by their mean age ± 1σ (note that errors are asymmetrical). Percentages listed in peak ages represent the percentage of the entire sample contained in that age population. For non-detrital samples, the weighted mean is listed here for reference, and “N/A” is listed in the other populations, given that there is only one population. Where a population is absent in the detrital samples, “xx” is listed. N represents the number of apatite grains analyzed in the sample. FT age range is the entire age range for single crystal apatite fission track ages in the sample. crucial in areas where a biostratigraphic framework is sparse. Also, many stratigraphic units are time transgressive, and establishing a MDA with DZ U-Pb can better indicate the stratigraphic position of a sample within a section. Sediment Provenance Constrained by Zircon U-Pb Geochronology Paleozoic stratigraphy exhumed in the Sevier fold-thrust belt (Dickinson, 2004; Dickinson and Gehrels, 2008; Gehrels et al., 2011; Laskowski et al., 2013). We interpret all of our DZ curves to represent recycled zircons from the Sevier foldthrust belt with variable contributions of young volcanic zircons from the Cordilleran arc. Source-to-Sink Exhumation History Zircon U-Pb geochronology can not only indicate the depositional age of the analyzed deposits, but also its provenance. Our study area covers ~600 km along strike of the Sevier fold-thrust belt and ~400 km along depositional dip into the foreland basin. Such a widespread geographical area includes multiple catchments and drainage areas. Despite this, the DZ signal is remarkably uniform (Fig. 8). This indicates a similar source and a well-connected drainage system without large geographic barriers to act as filters to certain signals. For example, distal deposits in South Dakota have similar-amplitude peaks of Cordilleran magmatic zircons (Fig. 8), showing that the forebulge did not block a westerly sediment supply derived from the Cordilleran arc. This suggests that the forebulge was an area of condensed deposition rather than erosion and that the foreland basin was overfilled (Flemings and Jordan, 1989). All DZ curves contain populations of Trans-Hudson, Yavapai, Mazatzal, 1.48–1.34 Ga magmatic rocks, Grenville, and pericratonic orogenic-age zircons. Smalleramplitude populations include Wopmay- and Archean-age zircons. This age distribution is consistent with zircon ages from miogeoclinal 16 Zircon He thermochronology was initially performed to identify the most effective thermochronometer to measure the timing of exhumation of Paleozoic strata during Mesozoic Cordilleran tectonics. Both sandstone and conglomerate cobbles produced a mix of ages ranging from 506.9 Ma to 22.8 Ma (Table 3; Fig. 9). Ages from individual samples vary widely, with up to ~400 m.y. internal variation, indicating only partial resetting of the fold-thrust belt sediment sources, and suggest that this material, once incorporated into the orogenic system and later deposited within synorogenic deposits, was never fully reset by subsequent basin burial; this implies exhumation depths of <8–9 km, assuming a 20 °C/km geothermal gradient and a partial retention zone for zircon He of 170–190 °C (Reiners et al., 2004). A sample from the Proterozoic Inkom Formation in the Canyon Range duplex structure also produced mixed ages between 139.7 Ma and 22.8 Ma (Table 3; Fig. 9). Another possibility for nonuniform zircon He ages is that Paleozoic and Proterozoic strata were exhumed from temperatures greater than ~190 °C but that excess He was being retained in these zircons because of alpha-decay damage (Guenthner et al., 2013), as diffusion of He is impeded in crystals with large amounts of radiation damage (i.e., damage to the crystal caused by alpha decay and spontaneous fission) (Shuster et al., 2006; Flowers et al., 2009). Guenthner et al. (2013) documented that He diffusion is impeded in zircons with moderate to high levels of radiation damage, but that in zircons that have very high amounts of radiation damage, He diffusion is accelerated. In contrast, we interpret all of our AFT samples to contain fully reset populations that record source exhumation (or volcanogenesis in the case of some of the detrital samples) related to Cordilleran tectonics. The age populations in the conglomerate cobbles all have a χ2 probability greater than 5%, suggesting a single population and full resetting of the conglomerate source during Cretaceous time (Table 4). The individual populations in the detrital samples also have a χ2 probability greater than 5%. Whereas burial of conglomerate and sandstone may cause partial annealing, we do not think that the analyzed samples were reheated enough to initiate significant annealing. This interpretation is based on the observation that in general, our samples display an upsection younging of cooling ages (populations). If post-depositional partial annealing was significant, we should expect deeper samples to record younger ages and vice versa, resulting in a downsection younging of cooling ages. BINOMFIT (Brandon, 2002) identifies a young AFT population of ca. 52.1 Ma in the ca. 118 Ma Kelvin Formation (sample 051204) (Table 2), Geological Society of America Bulletin, Month/Month 2014 Exhumation of the North American Cordillera 84 0 69 –1 57 47 –2 38 –3 32 –4 26 0.24 2.44 0.61 0.35 SE[z] (~RSE[age]) 4 Density (% per delta z=0.1) 102 FT grain age (Ma) 123 2 1 176 d) 060923 Price River Fm. 3 109 1 93 0 79 –1 67 57 –2 –3 –4 2.01 12 0.50 0.29 SE[z] (~RSE[age]) 051212 Chimney Rock 12 12 10 10 8 8 6 6 2 0 0 960 30 20 60 120 240 FT grain age (Ma) 480 051204 Kelvin Fm. 1 40 80 160 FT grain age (Ma) 320 12 12 Density (% per delta z=0.1) 16 4 4 0 20 40 80 160 FT grain age (Ma) 0 60 120 240 480 FT grain age (Ma) 960 189 e) 051208 Brooks Fm. 160 f) 12 12 10 10 136 2 116 1 98 0 83 –1 71 60 –2 51 43 2.07 37 0.21 0.52 0.30 SE[z] (~RSE[age]) 8 8 6 6 4 4 2 2 0 20 40 3 h) 10 051207 Blair Fm. 8 8 6 6 4 4 80 160 320 FT grain age (Ma) 051201 Echo Canyon Cgl. 640 0 250 i) 209 174 145 1 120 100 0 83 –1 2 2 –2 0 0 –3 30 16 8 2 69 57 48 14 j) 20 8 3 2 0 Standardized variance 2 4 3 2 Density (% per delta z=0.1) 4 4 0 30 10 4 5 1 g) 12 6 5 0 –4 6 7 6 0 20 35 0.20 8 7 6 2 –3 Density (% per delta z=0.1) Density (% per delta z=0.1) 8 8 2 42 10 c) 9 4 Tongue Mbr. 10 NSD4 B Sego Sandstone Mbr. 8 4 3 49 9 14 060922 Price River Fm. 128 2 b) 14 4 150 Standardized variance Standardized variance Sam 17 Sego Sandstone Mbr. 150 FT grain age (Ma) Standardized variance 3 182 FT grain age (Ma) a) Density (% per delta z=0.1) North Horn Fm. Standardized variance Sam 8 FT grain age (Ma) 4 60 120 240 480 FT grain age (Ma) 960 0.77 0.44 SE[z] (~RSE[age]) 40 0.31 k) 14 051218 Dakota SS. 12 12 10 10 8 8 6 6 4 4 2 2 0 30 3.10 0 60 120 240 FT grain age (Ma) 480 Figure 10. Probability density plots for all detrital apatite fission track (AFT) samples, and radial plots for all conglomerate cobble AFT samples (Table 5). Dashed lines outline grain populations as chosen by BINOMFIT (Brandon, 2002). Each plot is labeled with its corresponding sample name. Note that axis scales are variable. X-axis indicates the standard error (SE) of log of age (z). This is approximately equal to the relative standard error (RSE). Geological Society of America Bulletin, Month/Month 2014 17 Painter et al. 60 0 100 200 AFT cooling age (Ma) 300 400 500 600 70 90 100 g time 10 Myr la g time 0 Myr la Depostional age (Ma) 80 Figure 11. Depositional age versus apatite fission track cooling age of all samples analyzed with apatite fission track thermochronology (AFTT) (both detrital and non-detrital samples). See Tables 4 and 5 for details. 0 m.y., 5 m.y., and 10 m.y. lag times are shown with gray lines. 110 Legend North Horn Fm. (Sam 8) upper Sego SS Mbr. (Sam 17) lower Sego SS Mbr. (NSD4 B) Price River Fm. (060923) Price River Fm. (060922) Brooks Mbr. (051208) Chimney Rock Tng. Mbr. (051212) Blair Fm. (051207) Echo Canyon Cgl. (051201) Dakota Fm. (051218) Kelvin Fm. (051204) 120 130 which could represent post-depositional partial annealing. However, this age population is based on <5 apatite grains, which is too few to determine an age population with confidence. Also, sample 051204 was collected in northeastern Utah, where the Kelvin Formation is overlain by only ~2 km of Cretaceous to Cenozoic stratigraphy (Royse, 1993; DeCelles and Currie, 1996), which is not enough to reach temperatures that could partially anneal fission tracks in apatite (Gleadow and Duddy, 1981). This independent evidence suggests that the sampled conglomerate cobbles and detrital sandstone populations represent sediment source cooling ages and implies that the Paleozoic miogeoclinal sources were exhumed during the Cretaceous from temperatures greater than 110 ± 10 °C (Gleadow and Duddy, 1981), corresponding to ~4–5 km depths assuming a 20 °C/km geothermal gradient. Detrital samples produce populations that range from ca. 455 to 67 Ma (Table 5). The youngest population, P1, has an age range from ca. 133 Ma (sample 051204 from the Lower Cretaceous Kelvin Formation) to ca. 67 Ma (sample Sam 17 from the Upper Cretaceous Sego Sandstone Member) (Tables 5). This suggests that AFT, on both conglomerate cobbles and detrital foreland basin samples, is an effective thermochronometer to measure cooling and exhumation related to the development of the Cordilleran thrust belt. 18 Lag-time measurements (Fig. 5) are useful in identifying provenance (e.g., Hurford and Carter, 1991; Ireland, 1992; Carter, 1999; Garver et al., 1999). Also, lag times can provide information on the long-term orogenic-scale exhumation (e.g., Zeitler et al., 1986; Bernet et al., 2001). A decrease in lag time can be correlated to an increase in source region exhumation rates, whereas an increase in lag time indicates a decrease in exhumation rates (Bernet et al., 2001). Constant lag times are associated with steady-state exhumation (Garver et al., 1999) (Fig. 6). Lag-time trends can also be associated with exhumation in response to different orogenic wedge dynamics (Davis et al., 1983; Dahlen, 1984; Suppe and Medwedeff, 1990; Carrapa, 2009) (Fig. 13). Orogenic wedge theory treats the orogen as a wedge and associates its behavior to its taper angle (α + β), where β is the angle of the basal detachment and α is the angle of the topographic slope (Davis et al., 1983). If α decreases because of erosion or other process, then the wedge will build internally to restore critical taper. If the wedge builds too much, then it will collapse and propagate into the foreland (Davis, et al., 1983; Dahlen, 1984) (Fig. 13). Increased exhumation rates have been predicted for a wedge in a subcritical state (where the wedge shortens internally to achieve critical taper), whereas decreased exhumation trends have been predicted for a wedge that is in a supercritical state and propagating toward the foreland (Carrapa, 2009) (Fig. 13). Different orogenic states and trends of exhumation also correlate with the behavior of the rate of propagation of deformation through the foreland. When a wedge is deforming internally, the rate of foreland-ward propagation of deformation is expected to decrease, and vice versa (Davis et al., 1983; Carrapa, 2009). In detrital thermochronologic studies, the youngest age is typically considered a source exhumation signal and used to measure lag time (Garver et al., 1999; Carrapa et al., 2004, 2006; Spiegel et al., 2004; van der Beek et al., 2006) (Fig. 14). However, this assumes that the youngest cooling age, P1, only includes minerals that represent source exhumation rather than volcanic contamination. Our study shows that the youngest detrital AFT component in the Cordilleran foreland basin often includes volcanogenic grains (i.e., minerals that were erupted near the time of exhumation). Volcanic minerals should have a cooling age close to or the same as crystallization age. Our double dating results show that all but two of the P1 populations of all of our detrital samples are significantly contaminated with apatites that have U-Pb ages within error of the youngest AFT age component (Table 6). An alternative explanation is that P1 for all the samples represents rapidly exhumed plutonic apatites, but the methodological error prevents Geological Society of America Bulletin, Month/Month 2014 Exhumation of the North American Cordillera TABLE 6. DOUBLE DATES—APATITE FISSION TRACK (AFT) AND U-Pb AGE OF SINGLE APATITE GRAINS Depositional age AFT P1 age AFT grain age 6/8 U-Pb age Sample name–apatite grain number Stratigraphic unit (Ma) (Ma) (Ma) (Ma) Sam 17-10 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 70.5 ± 50.7 93.5 ± 5.1 Sam 17-11 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 73.6 ± 48.6 142.1 ± 15.8 Sam 17-12 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 76.1 ± 24.4 510.7 ± 59.7 Sam 17-15 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 59.8 ± 26.3 100.6 ± 3.8 Sam 17-16 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 48.3 ± 28.9 85.0 ± 7.5 Sam 17-17 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 51.5 ± 28.9 95.2 ± 10.4 Sam 17-19 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 68.9 ± 49.6 867.2 ± 17.5 Sam 17-22 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 39.2 ± 22.2 150.9 ± 9.6 Sam 17-24 Sego Sandstone Member 73 ± 1.5 73.2 ± 45.0 99.8 ± 9.0 66.6 ± 6.0/5.5 [72.0%] Sam 17-25 Sego Sandstone Member 73 ± 1.5 66.6 ± 6.0/5.5 [72.0%] 67.0 ± 51.4 131.0 ± 2.1 NSD4 B-5 Sego Sandstone Member 76.6 ± 1.5 58.2 ± 30.8 89.2 ± 59.0 66.6 ± 7.3/6.6 [33.1%] NSD4 B-6 Sego Sandstone Member 76.6 ± 1.5 66.6 ± 7.3/6.6 [33.1%] 52.1 ± 19.3 101.7 ± 5.1 NSD4 B-10 Sego Sandstone Member 49.3 ± 22.2 1676.5 ± 80.0 76.6 ± 1.5 66.6 ± 7.3/6.6 [33.1%] NSD4 B-13 Sego Sandstone Member 76.6 ± 1.5 66.6 ± 7.3/6.6 [33.1%] 67.4 ± 46.3 103.9 ± 3.7 NSD4 B-15 Sego Sandstone Member 53.0 ± 23.8 90.9 ± 8.7 76.6 ± 1.5 66.6 ± 7.3/6.6 [33.1%] NSD4 B-21 Sego Sandstone Member 76.6 ± 1.5 66.6 ± 7.3/6.6 [33.1%] 48.8 ± 23.8 1687.38 ± 41.9 NSD4 B-22 Sego Sandstone Member 78.0 ± 54.7 116.8 ± 6.0 76.6 ± 1.5 66.6 ± 7.3/6.6 [33.1%] NSD4 B-23 Sego Sandstone Member 76.6 ± 1.5 66.6 ± 7.3/6.6 [33.1%] 54.5 ± 13.2 98.0 ± 98.4 NSD4 B-25 Sego Sandstone Member 63.4 ± 36.8 119.4 ± 5.5 76.6 ± 1.5 66.6 ± 7.3/6.6 [33.1%] 051208-2 Brooks Member 81 ± 3 112.0 ± 6.2/5.9 [82.8%] 95.1 ± 49.0 92.6 ± 6.2 051208-8 76.8 ± 47.6 83.7 ± 6.0 Brooks Member 81 ± 3 112.0 ± 6.2/5.9 [82.8%] 051208-9 Brooks Member 81 ± 3 112.0 ± 6.2/5.9 [82.8%] 125.9 ± 34.0 132.5 ± 35.2 051208-10 Brooks Member 81 ± 3 112.0 ± 6.2/5.9 [82.8%] 54.0 ± 15.8 89.6 ± 8.4 051208-12 Brooks Member 81 ± 3 81.0 ± 29.1 143.9 ± 31.7 112.0 ± 6.2/5.9 [82.8%] 051208-21 Brooks Member 81 ± 3 112.0 ± 6.2/5.9 [82.8%] 114.3 ± 58.0 125.1 ± 19.0 051208-24 71.3 ± 29.8 108.7 ± 31.9 Brooks Member 81 ± 3 112.0 ± 6.2/5.9 [82.8%] 051208-25 Brooks Member 81 ± 3 112.0 ± 6.2/5.9 [82.8%] 85.3 ± 33.0 98.4 ± 51.3 051212-6 Chimney Rock Tongue Member 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 54.9 ± 9.9 161.4 ± 14.1 051212-9 Chimney Rock Tongue Member 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 63.1 ± 31.6 138.4 ± 9.1 79.4 ± 55.0 100.2 ± 10.7 051212-11 Chimney Rock Tongue Member 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 051212-14 Chimney Rock Tongue Member 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 39.8 ± 4.2 156.6 ± 41.4 124.0 ± 78.2 106.2 ± 5.0 051212-20 Chimney Rock Tongue Member 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 051212-24 Chimney Rock Tongue Member 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 86.7 ± 42.7 140.4 ± 17.7 051212-25 Chimney Rock Tongue Member 84.6 ± 24.1 135.6 ± 22.1 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 051212-28 Chimney Rock Tongue Member 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 68.5 ± 25.1 127.2 ± 8.7 051212-29 Chimney Rock Tongue Member 83.2 ± 66.9 1571.2 ± 22.6 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 051212-30 Chimney Rock Tongue Member 81.5 ± 1 90.3 ± 5.5/5.2 [64.2%] 75.2 ± 37.3 148.7 ± 13.3 051207-2 Cedar Mountain Formation 111.4 ± 10.2 213.3 ± 26.0 82.5 ± 1 85.6 ± 9.7/8.7 [52.8%] 051207-3 Cedar Mountain Formation 82.5 ± 1 85.6 ± 9.7/8.7 [52.8%] 103.3 ± 17.2 102.8 ± 7.2 051207-5 Cedar Mountain Formation 105.2 ± 36.8 89.0 ± 10.8 82.5 ± 1 85.6 ± 9.7/8.7 [52.8%] 051207-10 Cedar Mountain Formation 82.5 ± 1 85.6 ± 9.7/8.7 [52.8%] 121.1 ± 78.3 171.1 ± 6.6 051207-14 Cedar Mountain Formation 44.2 ± 8.0 128.8 ± 12.6 82.5 ± 1 85.6 ± 9.7/8.7 [52.8%] 051207-16 Cedar Mountain Formation 82.5 ± 1 85.6 ± 9.7/8.7 [52.8%] 118.1 ± 40.8 100.8 ± 3.5 051207-17 Cedar Mountain Formation 75.5 ± 47.2 96.0 ± 5.6 82.5 ± 1 85.6 ± 9.7/8.7 [52.8%] 051207-18 Cedar Mountain Formation 82.5 ± 1 85.6 ± 9.7/8.7 [52.8%] 107.7 ± 45.9 1869.0 ± 159.5 051218-1 Dakota Formation 125.0 ± 76.2 1558.4 ± 26.4 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 051218-2 Dakota Formation 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 67.2 ± 37.8 1591.9 ± 40.9 051218-13 Dakota Formation 110.7 ± 66.4 1327.9 ± 15.3 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 051218-17 Dakota Formation 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 120.9 ± 74.6 1477.4 ± 30.0 051218-19 84.9 ± 30.8 1477.4 ± 30.0 Dakota Formation 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 051218-20 Dakota Formation 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 107.9 ± 79.6 320.6 ± 6.7 71.2 ± 38.5 1602.0 ± 17.0 051218-21 Dakota Formation 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 051218-23 Dakota Formation 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 107.1 ± 61.4 1578.1 ± 16.5 051218-24 Dakota Formation 94.5 ± 2.9 88.8 ± 7.0/6.5 [35.2%] 86.8 ± 51.5 1594.3 ± 12.5 051204-1 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 106.5 ± 40.1 227.4 ± 27.7 051204-2 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 35.3 ± 0.7 303.0 ± 71.0 051204-3 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 32.7 ± 12.3 141.8 ± 22.5 051204-4 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 87.6 ± 8.3 283.9 ± 37.7 051204-9 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 136.9 ± 61.7 333.5 ± 43.8 051204-10 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 110.7 ± 38.2 134.3 ± 21.3 051204-11 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 139.5 ± 57.5 892.1 ± 23.6 051204-13 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 48.2 ± 22.6 140.3 ± 18.2 051204-16 Kelvin Formation 117.2 ± 3.2 122.9 ± 12.2/11.7 [78.1%] 77.9 ± 13.4 184.2 ± 23.7 Note: Individual AFT population and grain ages compared to the U-Pb age. Detailed apatite U-Pb data and concordia plots can be found in the Data Repository. Italicized percentages represent how many of the total analyzed apatites are within that AFT age population. 6/8 U-Pb age indicates the 206Pb/238U age. Errors are 2σ. the differentiation between these and volcanogenic apatites. In an attempt to calculate lag times for the distal foreland basin sandstone samples, and to avoid misinterpretation of possible volcanogenic apatites, we consider only P1 from two samples: 051204 from the Lower Cretaceous Kelvin Formation, and 051218 from the Upper Cretaceous Dakota Formation (Table 5; Fig. 12). This is because the apatite U-Pb ages for P1 in these two samples are significantly older than the associated AFT ages. Plotting these P1 AFT ages that are not contaminated with volcanogenic apatites together with the conglomerate cobble AFT ages, versus depositional ages, shows a lag time between ~0 and 5 m.y. from 118 to 66 Ma (Fig. 15). The lag-time trend (Fig. 15) appears to be relatively constant, or slightly decreasing, which suggests either steady-state or slightly increasing exhumation rate through time in the source region (Garver et al., 1999; Bernet et al., 2001). Our lag times are consistent with rapid steady-state exhumation, suggesting that the Cordilleran orogenic wedge was at or Geological Society of America Bulletin, Month/Month 2014 19 Painter et al. 70 70 80 90 Depositional age from biostratigraphy and Ar/Ar (Ma) 100 110 120 130 140 80 MDA from youngest grain of DZ U-Pb (Ma) 90 100 110 U- Pb = bio s tra t 150 160 Legend Canyon Creek Mbr. (051210) Sego Sandstone Mbr. (Sam 17) Lazeart SS Mbr. (051205) Blair Fm. (051207) Frontier Fm. (051105) Dakota Fm. (051218) Cedar Mtn. Fm. (051107) Kelvin Fm. (051204) Morrison Fm. (051108) Morrison Fm. (051214) Morrison Fm. (051103) 120 130 140 150 160 170 Figure 12. Depositional age from biostratigraphy and Ar/Ar versus maximum depositional age (MDA) from detrital zircon (DZ) U-Pb. Gray dashed line is where U-Pb age equals that from biostratigraphy. Detailed data are included in Table 2. near critical throughout the Cretaceous (Fig. 15). However, as these techniques become more refined (reducing error) and are further applied to North America Cordilleran foreland deposits, spatial and temporal resolution may improve, and a more complex and detailed exhumation history may emerge. Lag-time measurements are also useful to approximate exhumation rates, and we use mea- sured lag times to estimate exhumation rates in the Sevier fold-thrust belt using the following equation (Garver et al. 1999): ⎡T − T ⎤ ε = ⎢ c s ⎥ tL , ⎣ G ⎦ (2) where ε is the effective exhumation rate in km/m.y., Tc and Ts are the closure temperatures of apatite and the surface temperature respectively, G is the geothermal gradient in °C/km, and tL is the lag time in years. We have already calculated tL as ~0–5 m.y. Given that a true lag time of 0 m.y. is impossible, an assumption of ~1–5 m.y. is more reasonable. Assuming a closure temperature of ~110 °C (Gleadow and Duddy, 1981), a surface temperature of 20 °C, and a geothermal gradient of 20 °C/km results in an average exhumation rate for the P1 source terrain of 0.9 km/m.y. during the Early Cretaceous and >1 km/m.y. during the Late Cretaceous. Exhumation rates of 0.9–>1 km/m.y. are relatively high for non-collisional systems such as the North America Cordillera, whereas they are more typical of rates recorded in collisional systems such as the Himalaya, the Pyrenees, and the Alps. Lag times between 0 and 5 m.y. have been recorded in Cenozoic foreland basin deposits of the western Alps (e.g., Carrapa et al., 2003). Garver et al. (1999) calculated exhumation rates based on detrital thermochronology of modern sediments in the Indus River draining the foothills of the Himalaya to be 0.6–1 km/m.y., whereas Najman et al. (2003) measured much more rapid Miocene exhumation rates in the Pakistan Himalaya, up to 4.5 km/m.y. Thiede and Ehlers (2013) reported highly varied exhumation rates through space and time in the Himalaya, ranging from 0.5 to 3 km/m.y. In the Pyrenees, Fitzgerald et al. (1999) measured exhumation rates to be ~0.2– >2 km/m.y., depending on the location in the orogen and time during the orogeny. In non-collisional systems such as the central Andes, the modern counterpart to the North America Cordillera (Coney and Evenchick, 1994; Dickinson, 2004), relatively low exhumation rates, 0.2 km/m.y., have been measured from synorogenic Mio-Pliocene deposits preserved on the south- decreasing exhumation Depositional age g la Foreland basin stratigraphic section nt e tim Geological Society of America Bulletin, Month/Month 2014 ta ns 20 co Exhumation of a crustal column Figure 13. Orogenic wedge Source exhumation and theory applied to lag times and deposition of eroded material exhumation rates (from Carin the adjacent foreland rapa, 2009). Orogenic wedge Pro-wedge and/or retro-wedge behavior 2 theory treats the orogen as a tA st wedge and associates its beea dy tC tA -st havior to the angle of the deat tB e tachment (β), the angle of the ex tB 120 °C inc tB 1 h rea um topographic slope (α), and a sing tC tA 2 at c exh tC io critical angle (θc) (Davis et al., u 350 °C ma 1 n tion 1983). If the sum of β and α is greater than θc then thrusting e.g., tA: cooling age at time tA < tB < tC rapidly propagates into the Detrital cooling age foreland; if the sum of β and α is less than θc, then the orogen builds internally (Davis et al., 1983). Increased exhumation rates correspond to subcritical wedges, when the wedge is building internally, and decreased exhumation trends correspond to times when the orogenic wedge is supercritical (Carrapa, 2009). “1” indicates that when the orogen builds internally (shown by the internal thrust fault), exhumation will increase (decreasing lag times). “2” indicates that when the thrusting rapidly propagates into the foreland, exhumation with decrease (increasing lag times). Exhumation of the North American Cordillera 50 60 70 80 AFT cooling age (Ma) 90 100 110 120 130 140 60 70 Depostional age (Ma) 80 90 100 110 120 130 Legend North Horn Fm. (Sam 8) upper Sego SS Mbr. (Sam 17) lower Sego SS Mbr. (NSD4 B) Price River Fm. (060923) Price River Fm. (060922) Brooks Mbr. (051208) Chimney Rock Tng. Mbr. (051212) Blair Fm. (051207) Echo Canyon Cgl. (051201) Dakota Fm. (051218) Kelvin Fm. (051204) 0 M 10 yr lag M tim yr lag e tim e Figure 14. All ages from the youngest apatite grain populations (P1) plotted against depositional ages. Note the scatter. Typically this would be used to interpret lag time, but as stated, this population is contaminated with volcanogenic apatites (Table 6). Interpreting all of these as lag times would produce an erroneous exhumation interpretation. that of the central Andean arc, Puna-Altiplano, and eastern Cordillera zones (Dickinson, 2004; DeCelles, 2004). Just as the high-elevation Puna Plateau has been subject to low exhumation rates (0.2 km/m.y.) since Eocene time (Deeken et al., 2006), it is likely that the Nevadaplano expe- 50 50 60 AFT cooling age of young exhumed apatites (Ma) 70 80 90 100 110 120 130 140 60 70 80 Depostional age (Ma) ern Puna Plateau (Carrapa et al., 2006). Similar exhumation rates to those presented in this study (>1 km/m.y.) have instead been recorded by Eocene–Oligocene wedge-top deposits on the eastern side of the Puna Plateau (Carrapa and DeCelles, 2008) and in Miocene deposits of the Eastern Cordillera of northwest Argentina (Coutand et al., 2006), suggesting that exhumation rates can be rapid and geographically concentrated during periods of tectonic activity. These high exhumation rates could not have been sustainable over the entire North American Cordillera for long periods of time, indicated by the fact that even low-grade metamorphic rocks were not exposed in the Cordillera during the Cretaceous (DeCelles, 2004; Long, 2012). Our AFT and zircon He thermochronology data suggest that material was exhumed from between 5 and 8 km depths, at exhumation rates of 0.9–>1 km/m.y. from 118 Ma to 66 Ma; however, this could not have taken place over the entire orogen without exhuming deep-crustal material. Instead, we propose that high rates of exhumation were concentrated in the frontal foldthrust belt along the eastern margin of the North America Cordillera (Fig. 16). DeCelles (2004) divided the retroarc side of the North America Cordillera into five zones: the Luning-Fencemaker thrust belt, central Nevada thrust belt, the Nevadaplano (a >3-km-high plateau during the mid- to Late Cretaceous), the frontal Sevier foldthrust belt, and the younger Laramide basementcored uplifts. This orogenic profile is similar to rienced low exhumation rates, and that rapid exhumation was instead concentrated along the eastward-propagating Sevier fold-thrust belt (Long, 2012). While the Sevier fold-thrust belt was active, new material was constantly being exhumed in the frontal part of orogenic wedge, allowing consistently fast but localized exhumation rates of >1 km/m.y. (Fig. 16). Multiple researchers have used subsidence histories to document initial thrusting and flexural loading of the Sevier fold-thrust belt, total subsidence, and flexural wave migration (e.g., Heller et al., 1986; Pang and Nummedal, 1995; DeCelles and Currie, 1996; Allen et al., 2000; Liu and Nummedal, 2004). Focusing on the samples that are free of volcanic contamination (Fig. 15), all are from units deposited in proximal to distal foredeep depozones. Subsidence histories show that these ca. 118–66 Ma samples come from strata deposited during active shortening and subsidence (Heller et al., 1986; DeCelles and Currie, 1996; Pang and Nummedal, 1995; Liu and Nummedal, 2004), and the consistent small lag times (i.e., rapid exhumation) support this (Fig. 15). Small lag times recorded in this study are inconsistent with significant reworking and do not support the hypothesis that coarse clastics are associated with tectonic quiescence and reworking of more proximal foreland basin material. Currently, there is no agreement on the significance of distal upward-coarsening deposits. Horton et al. (2004) linked distal coarsegrained sedimentary rocks to active shortening 90 100 110 Legend North Horn Fm. (Sam 8) Price River Fm. (060923) Price River Fm. (060922) Echo Canyon Cgl. (051201) Dakota Fm. (051218) Kelvin Fm. (051204) 0 120 M 10 yr l ag tim e M yr lag tim e (2) (1) 130 Figure 15. Lag time plot. All populations that have been contaminated with volcanic apatites have been removed from the youngest grain populations (P1). Gray arrows outline two possible exhumation interpretations: (1) constant lag time and steadystate exhumation; (2) decreasing lag times and increasing exhumation rates. Geological Society of America Bulletin, Month/Month 2014 21 Painter et al. low exhumation rates ~0.2 km/Myr Nevadaplano west arc high exhumation rates 0.9−>>1 km/Myr Sevier fold-thrust belt east North America Fara l lon Plat e Figure 16. Schematic of the North America Cordillera during the Cretaceous, outlining the position of the arc, Nevadaplano, and Sevier fold-thrust belt and exhumation rates (modified from DeCelles, 2004). Exhumation rates for the Nevadaplano are estimated using measurements from the Puna Plateau in Carrapa et al. (2006). The dashed lines above the subducting slab represent the shallowing slab during the Late Cretaceous. and exhumation in the Charleston-Nebo portion of the Sevier fold-thrust belt, but others (Willis, 2000) used the two-phase stratigraphic model as described by Heller et al. (1988) to explain the progradation of the Castlegate Formation and the Sego Sandstone Member as the result of periods of tectonic quiescence (Fig. 4). The two-phase stratigraphic model applies to retroarc foreland basins dominated by flexural processes (Heller et al., 1988). However, the North America Cordilleran foreland was partitioned by Laramide-style basement-cored uplifts by Maastrichtian time (ca. 71 Ma) (Dickinson et al., 1988; DeCelles, 2004), and Aschoff and Steel (2011) proposed that Laramide deformation initiated during the Campanian, as early as ca. 77 Ma. This implies that stratigraphic and thermochronologic studies of Campanian distal sandstones in the North America Cordilleran foreland may not be a good test for the two-phase stratigraphic model. However, lagtime measurements presented here are small (<5 m.y.) for all pre-Laramide samples (ca. 119 Ma–80 Ma) (Fig. 15). Data resolution is an issue in detrital thermochronology studies, and higher vertical (stratigraphic) and spatial lagtime resolution would be ideal; however, our lag-time measurements do not support the existence of tectonically quiescent periods between ca. 95 and 66 Ma and arguably between ca. 118 and 66 Ma (Fig. 15), but instead suggest active tectonics within the North American Cordillera throughout those time intervals. SUMMARY AND CONCLUSIONS The combination of DZ U-Pb geochronology, detrital AFT, and zircon He thermochronology provides constraints on the depositional ages of 22 synorogenic deposits. Our new data show good agreement between the youngest DZ U-Pb grain ages and existing 40Ar/39Ar ages of ashes and biostratigraphic ages of ammonite zones, supporting and further refining the stratigraphic age of Upper Jurassic to Upper Cretaceous foreland basin deposits in Western Interior U.S.A. Zircon He thermochronology on conglomerate cobbles from the Price River Conglomerate produced mixed ages of 76.2 ± 2.6 Ma, 253.1 ± 8.4 Ma, and 231.1 ± 7.7 Ma, which indicates maximum exhumation of source material from depths with temperatures <190 °C and from no deeper than ~8–9 km, assuming a 20 °C/km geothermal gradient, during the development of the North American Cordillera. In contrast, AFT ages of conglomerate cobbles in wedge-top deposits produce single near-syndepositional age populations, indicating that fission tracks were completely annealed in the thrust belt prior to exhumation. This suggests that source material was exhumed from depths with temperatures >120 °C, ~4–5 km deep. Zircon He and AFT limit exhumation depths to between ~4 and 9 km. None of the detrital foreland basin samples appears to be significantly annealed following deposition, so burial in these areas likely did not exceed 3–4 km, which is also supported by independent stratigraphic information (DeCelles and Currie, 1996). Although AFT proves to be an effective thermochronometer in the North America Cordilleran foreland basin, measuring lag time is challenged by several factors, including: (1) low yield of apatite grains in foreland basin deposits—only 11 out of the >37 samples processed for apatite yielded enough for AFT analysis, even with >10 kg sample size; and (2) young volcanic or arc-derived contamination. The prevalence of young volcanic or arc-derived apatites indicates that the assumption that volcanic contamination in the foreland basin deposits is negligible is not always applicable, and U-Pb thermochronology needs to be routinely applied on detrital apatites to identify co-magmatic apatites versus older exhumed apatites. Future thermochronologic studies of foreland basin deposits may be key in identifying whether orogenic growth of the North American Cordillera initiated during the Late Jurassic or Early Cretaceous (Heller et al., 1986; DeCelles and Burden, 1992; DeCelles and Currie, 1996; Currie, 1997). Small lag times (i.e., rapid exhumation rates) measured in the Upper Jurassic Morrison Formation would indicate Late Jurassic orogenic growth. However, none of the samples included in this study yielded sufficient apatite to measure lag time. Our measurements indicate small lag times of ~0–5 m.y. throughout Cretaceous time. Though the spatial and temporal resolution is limited, the short lag times are consistent with overall steady-state to slightly increasing source exhumation at rates of 0.9 to >1 km/m.y. Lag times are similar in both synorogenic wedge-top conglomerates (i.e., the Price River Conglomerate and the North Horn Formation) and distal foredeep sandstones (i.e., the Kelvin and Dakota Formations), suggesting that both proximal and distal foreland basin coarse-grained deposits represent periods of active tectonics and exhumation, rather than tectonic quiescence, in the Cordilleran foreland basin. These data also indicate that apatites in distal sandstones in the Cordilleran foreland basin were likely not stored in the proximal part of the foreland for a measureable amount of time and then reworked into the distal foreland basin. Furthermore, these Geological Society of America Bulletin, Month/Month 2014 Exhumation of the North American Cordillera consistently rapid exhumation rates indicate that exhumation was likely focused along the eastern flank of the Nevadaplano and the Sevier foldthrust belt, and that the hinterland experienced much slower exhumation rates. ACKNOWLEDGMENTS We thank the team at the Arizona LaserChron Center. Particularly we thank Mark Pecha, Clayton Loehn, Nicky Geisler, Intan Yokelson, and Chelsi White. Also, we thank Peter Reiners and Stefan Nicolescu for support during our zircon (U-Th-[Sm])/He data acquisition. Xennephone Hadeen was of great help during some of the sample preparation steps. Facilities at the Arizona LaserChron Center are supported by National Science Foundation awards NSF-EAR 0732436 and 1032156. We thank Shell Oil, ExxonMobil, and a 2012 GSA research grant for funding support. We thank Brian S. Currie and Shari A. Kelley for their thorough and constructive reviews. We also thank Timothy F. Lawton, the Associate Editor, for his detailed comments and review. All of their input helped with the clarity of this manuscript. In addition, we thank Heidi Carroll for reading the manuscript and giving technical writing feedback. 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