{"title":"新墨西哥州Arriba县Cerro Pedernal的地质和地质考古意义","authors":"Gary A. Smith, B. Huckell","doi":"10.56577/ffc-56.425","DOIUrl":null,"url":null,"abstract":"—Cerro Pedernal is an isolated basalt-capped peak of substantial geologic and geoarchaeological significance. The peak is located on the Colorado Plateau near the boundary of the Rio Grande rift. Oligocene-Miocene stratigraphic units on Cerro Pedernal correlate to thicker sections within the rift and document initiation of rift-basin subsidence before 25 Ma. Cessation or near cessation of sedimentation on the nascent rift margin led to hypothesized extensive weathering and formation of pedogenic calcrete horizons that were later buried by volcaniclastic deposits that overlapped the rift margin. Diagenesis of vitric volcaniclastic detritus likely led to silica replacement of the calcareous soils to form the Pedernal chert, which was commonly used for lithic-tool manufacture for more than 13 millennia of human occupation in northern New Mexico. Heavily utilized chert quarries in the Cerro Pedernal-San Pedro Parks region were important lithic-material sources, but so were redeposited cobbles of chert that are ubiquitous in alluvial deposits on the Colorado Plateau and in the Rio Grande rift. The combination of primary and secondary chert sources has confounded efforts to determine the exact source locations of artifact raw materials. Fire, along with simple prying tools and hammerstones were likely used to dislodge large chert pieces for tool manufacture. Preliminary working of cores and bifaces produced large volumes of irregular flakes and rejected pieces that were mistaken by some early workers as finished products of more ancient tool-making cultures. FIGURE 1. View of Cerro Pedernal from the north. Miocene basalt caps a pinnacle of poorly exposed lower and middle Tertiary strata that rise above a base of Mesozoic rocks. Photo courtesy of Lisa W.Huckell. 426 SMITH AND HUCKELL Basalt flows and the intrusion of contemporary dikes along faults; they proposed that principal rift-basin subsidence in the Abiquiu embayment initiated at about 10 Ma. Smith et al. (2002) point out, however, that the basalt flows preserve a northward paleoslope from the Jemez Mountains that was eroded on southwest-dipping rift-basin fill (Fig. 2). The angular unconformity between the basalt and underlying strata implies that most basin subsidence occurred before basalt extrusion. Figure 3 illustrates the correlation of Cerro Pedernal stratigraphy to the stratigraphic section in the Cañones area in the western Rio Grande rift and only 5 km east of the peak. The correlation of rift-basin stratigraphy mapped by Manley (1982) and Moore (2000) to the undeformed section at Cerro Pedernal highlights evidence for the pre-basalt rifting history. Middle Miocene strata of the Tesuque Formation thicken dramatically from about 65 m at Cerro Pedernal to 330 m southeast of Cañones, indicating substantial movement on the Gonzales and Cañones faults (Figs. 2 and 3) before eruption of the Lobato Basalt. The underlying Abiquiu Formation consists of two thick members, a lower member of Precambrian-clast gravel and conglomerate, and an upper member of volcaniclastic sandstone and conglomerate (Smith, 1938; Vazzana, 1980; Moore, 2000). The lower member thickens only slightly between Cerro Pedernal and Cañones, whereas the upper member is roughly 25% thicker at Cañones (Fig. 3). Recognition of stratigraphic subdivisions within the upper member defined by changing volcanic provenance (Smith, 1995), allowed Moore (2000) and Smith et al. (2002) to further determine that the thinner section at Cerro Pedernal lacks the lowermost parts of the upper member that are present in outcrop near Cañones and farther east near Abiquiu. Clasts of the 25 Ma Amalia Tuff and sandstones with abundant quartz and alkali feldspar eroded from the tuff and coeval volcanic rocks of the Latir volcanic field (north of Taos, NM) occur at the base of the upper member at Cerro Pedernal (Smith et al., 2002; Fig. 3). This same marker horizon is about 15 m above the base of the upper member near Cañones and is more than 80 m above the base near Abiquiu (Smith et al., 2002). These observations imply that basin subsidence and rift-margin faulting were underway during Abiquiu Formation deposition, which commenced in this area before eruption of the 25 Ma Amalia Tuff (Smith et al., 2002). Deposition of approximately 400 m of Abiquiu Formation outside of the rift at Cerro Pedernal also implies aggradation mechanisms other than rift-basin subsidence. Moore (2000) and Smith et al. (2002) provide the results of simple flexural-loading and sediment-transport models that can partially account for deposition of the Abiquiu Formation by two mechanisms. First, the loading of the crust by construction of the coeval San Juan and Latir volcanic fields (in southern Colorado and north-central New Mexico, respectively) likely produced a flexural moat of sufficient dimensions to produce sediment accommodation space FIGURE 2. Generalized geologic map of the Abiquiu region showing the location of Cerro Pedernal near the boundary between the Colorado Plateau and the Abiquiu embayment of the Rio Grande rift (after Smith et al., 2002). FIGURE 3. Correlation of Oligocene and Miocene rocks eastward from Cerro Pedernal shows abrupt thickening of strata across rift-margin faults, except for the Pedernal member, which is restricted to the footwall of the Cañones fault. Thickening across faults implies syndepositional movement on rift-margin faults. The restricted distribution of the Pedernal member, along with condensation of the lowest strata of the upper member implied by the lowest appearance of Amalia Tuff clasts, is consistent with an initial pedogenic origin for the Pedernal member. 427 GEOLOGICAL AND GEOARCHAEOLOGICAL SIGNIFICANCE OF CERRO PEDERNAL in the Cerro Pedernal area. Second, the inundation of rivers by large volumes of volcanically produced pyroclastic sediment would likely lead to regrading of river profiles that would cause modest aggradation in this region. This volcanism-driven aggradation allowed sedimentation to extend beyond the nascent rift margin, whereas stratigraphic thickening into the rift, relative to the section at Cerro Pedernal, demonstrates the contemporaneity of deposition and rift-basin subsidence (Smith et al., 2002). Nature and Origin of the “Pedernal Chert” In Abiquiu Formation outcrops west of the Cañones fault, the Pedernal member is present between the lower and upper members (Fig. 3; Bryan, 1938, 1939; Smith, 1938; Church and Hack, 1939). The Pedernal member is a 4to 8-m thick interval of gravel that resembles the lower member but is notable for the presence of one to four, discontinuous, irregular bodies of chalcedonic and cherty silica with varying proportions of associated calcite. Figure 4 presents the approximate extent of the Pedernal chert member as mapped by Church and Hack and others (Banks, 1990; LeTourneau, 2000). Most of the chert is massive with scattered pebbles but in places also consists of nodular cement within gravel. The siliceous layers compose the informally known “Pedernal chert.” The siliceous horizons are best exposed as outcrop ledges more than 2 m thick near the tapered base of Cerro Pedernal (at an elevation of ~1900 m), but continue southwestward around the western margin of the Jemez Mountains and form much of the summit plateau of the Sierra Nacimiento at the San Pedro Parks (at an elevation of 3100-3200 m; Fig. 4; Church and Hack, 1939). Although sedimentary deep-sea chert and chert replacement of limestone are common rocks, the Pedernal chert is very unusual as a nonmarine occurrence of stratiform silica. The siliceous horizons are very heterogeneous in thickness, color, and texture. Individual layers range from 20 cm to more than 2 m thick. Upper and lower contacts are undulatory and are sharp in some places but gradational through a nodular-chert zone in other places. As Bryan (1939, p. 17) described it: “The chert is commonly white to pearly gray in color though in places the color may vary considerably. Near the base and sometimes near the top the chert shows bands 1/4” to 1/2” thick and is black in color. In places near the top, weathering has changed the color to pink, red, or yellow. The red color also occurs as flecks or spots in the white to pearly gray mass. Generally the yellow color is associated with clear, very translucent phases of the chert. This translucent type usually occurrs in small masses near the top of the bed.” Most exposures consist of vitreous chert (equant, microcrystalline quartz) and chalcedony (fibrous quartz) dominated by translucent gray and yellowish gray colors with patches and swirls of more opaque red, maroon, and black coloration. Discontinuous micritic calcite, in horizons as much as 50 centimeters thick, is present in the lower parts of, or beneath, most siliceous layers. Petrographic observations by Vazzana (1980) and Moore (2000) show evidence of replacement of micritic calcite by both chalcedony and chert, with subsequent infilling of vugs by chalcedony, drusy quartz, or sparry calcite. Although cropping out only in a narrow stratigraphic interval over an area of only 300 km2, chert pebbles and cobbles from this unit are notable in rift-basin and younger valley-fill alluvial deposits southward into the Albuquerque basin, westward into the San Juan basin, and eastward into the Española basin (Fig. 4). The persistence of the siliceous clasts attests to the resistance to weathering and the hardness of Pedernal chert. No researchers have systematically studied the siliceous horizons of the Pedernal member, although Vazzana (1980) and Moore (2000) provided some important observations and data as part of broad studies of the Abiquiu Formation. Vazzana (1980) described mineralogical and whole-rock-geochemical variations within sandy gravel below a Pedernal chert horizon that he ascribed to a buried weathering profile. Along with the widespread replacement of micritic calcite by silica, Vazzana (1980) and Moore (2","PeriodicalId":345302,"journal":{"name":"Geology of the Chama Basin","volume":"4 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":"{\"title\":\"The geological and geoarchaeological significance of Cerro Pedernal, Rio Arriba County, New Mexico\",\"authors\":\"Gary A. Smith, B. Huckell\",\"doi\":\"10.56577/ffc-56.425\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"—Cerro Pedernal is an isolated basalt-capped peak of substantial geologic and geoarchaeological significance. The peak is located on the Colorado Plateau near the boundary of the Rio Grande rift. Oligocene-Miocene stratigraphic units on Cerro Pedernal correlate to thicker sections within the rift and document initiation of rift-basin subsidence before 25 Ma. Cessation or near cessation of sedimentation on the nascent rift margin led to hypothesized extensive weathering and formation of pedogenic calcrete horizons that were later buried by volcaniclastic deposits that overlapped the rift margin. Diagenesis of vitric volcaniclastic detritus likely led to silica replacement of the calcareous soils to form the Pedernal chert, which was commonly used for lithic-tool manufacture for more than 13 millennia of human occupation in northern New Mexico. Heavily utilized chert quarries in the Cerro Pedernal-San Pedro Parks region were important lithic-material sources, but so were redeposited cobbles of chert that are ubiquitous in alluvial deposits on the Colorado Plateau and in the Rio Grande rift. The combination of primary and secondary chert sources has confounded efforts to determine the exact source locations of artifact raw materials. Fire, along with simple prying tools and hammerstones were likely used to dislodge large chert pieces for tool manufacture. Preliminary working of cores and bifaces produced large volumes of irregular flakes and rejected pieces that were mistaken by some early workers as finished products of more ancient tool-making cultures. FIGURE 1. View of Cerro Pedernal from the north. Miocene basalt caps a pinnacle of poorly exposed lower and middle Tertiary strata that rise above a base of Mesozoic rocks. Photo courtesy of Lisa W.Huckell. 426 SMITH AND HUCKELL Basalt flows and the intrusion of contemporary dikes along faults; they proposed that principal rift-basin subsidence in the Abiquiu embayment initiated at about 10 Ma. Smith et al. (2002) point out, however, that the basalt flows preserve a northward paleoslope from the Jemez Mountains that was eroded on southwest-dipping rift-basin fill (Fig. 2). The angular unconformity between the basalt and underlying strata implies that most basin subsidence occurred before basalt extrusion. Figure 3 illustrates the correlation of Cerro Pedernal stratigraphy to the stratigraphic section in the Cañones area in the western Rio Grande rift and only 5 km east of the peak. The correlation of rift-basin stratigraphy mapped by Manley (1982) and Moore (2000) to the undeformed section at Cerro Pedernal highlights evidence for the pre-basalt rifting history. Middle Miocene strata of the Tesuque Formation thicken dramatically from about 65 m at Cerro Pedernal to 330 m southeast of Cañones, indicating substantial movement on the Gonzales and Cañones faults (Figs. 2 and 3) before eruption of the Lobato Basalt. The underlying Abiquiu Formation consists of two thick members, a lower member of Precambrian-clast gravel and conglomerate, and an upper member of volcaniclastic sandstone and conglomerate (Smith, 1938; Vazzana, 1980; Moore, 2000). The lower member thickens only slightly between Cerro Pedernal and Cañones, whereas the upper member is roughly 25% thicker at Cañones (Fig. 3). Recognition of stratigraphic subdivisions within the upper member defined by changing volcanic provenance (Smith, 1995), allowed Moore (2000) and Smith et al. (2002) to further determine that the thinner section at Cerro Pedernal lacks the lowermost parts of the upper member that are present in outcrop near Cañones and farther east near Abiquiu. Clasts of the 25 Ma Amalia Tuff and sandstones with abundant quartz and alkali feldspar eroded from the tuff and coeval volcanic rocks of the Latir volcanic field (north of Taos, NM) occur at the base of the upper member at Cerro Pedernal (Smith et al., 2002; Fig. 3). This same marker horizon is about 15 m above the base of the upper member near Cañones and is more than 80 m above the base near Abiquiu (Smith et al., 2002). These observations imply that basin subsidence and rift-margin faulting were underway during Abiquiu Formation deposition, which commenced in this area before eruption of the 25 Ma Amalia Tuff (Smith et al., 2002). Deposition of approximately 400 m of Abiquiu Formation outside of the rift at Cerro Pedernal also implies aggradation mechanisms other than rift-basin subsidence. Moore (2000) and Smith et al. (2002) provide the results of simple flexural-loading and sediment-transport models that can partially account for deposition of the Abiquiu Formation by two mechanisms. First, the loading of the crust by construction of the coeval San Juan and Latir volcanic fields (in southern Colorado and north-central New Mexico, respectively) likely produced a flexural moat of sufficient dimensions to produce sediment accommodation space FIGURE 2. Generalized geologic map of the Abiquiu region showing the location of Cerro Pedernal near the boundary between the Colorado Plateau and the Abiquiu embayment of the Rio Grande rift (after Smith et al., 2002). FIGURE 3. Correlation of Oligocene and Miocene rocks eastward from Cerro Pedernal shows abrupt thickening of strata across rift-margin faults, except for the Pedernal member, which is restricted to the footwall of the Cañones fault. Thickening across faults implies syndepositional movement on rift-margin faults. The restricted distribution of the Pedernal member, along with condensation of the lowest strata of the upper member implied by the lowest appearance of Amalia Tuff clasts, is consistent with an initial pedogenic origin for the Pedernal member. 427 GEOLOGICAL AND GEOARCHAEOLOGICAL SIGNIFICANCE OF CERRO PEDERNAL in the Cerro Pedernal area. Second, the inundation of rivers by large volumes of volcanically produced pyroclastic sediment would likely lead to regrading of river profiles that would cause modest aggradation in this region. This volcanism-driven aggradation allowed sedimentation to extend beyond the nascent rift margin, whereas stratigraphic thickening into the rift, relative to the section at Cerro Pedernal, demonstrates the contemporaneity of deposition and rift-basin subsidence (Smith et al., 2002). Nature and Origin of the “Pedernal Chert” In Abiquiu Formation outcrops west of the Cañones fault, the Pedernal member is present between the lower and upper members (Fig. 3; Bryan, 1938, 1939; Smith, 1938; Church and Hack, 1939). The Pedernal member is a 4to 8-m thick interval of gravel that resembles the lower member but is notable for the presence of one to four, discontinuous, irregular bodies of chalcedonic and cherty silica with varying proportions of associated calcite. Figure 4 presents the approximate extent of the Pedernal chert member as mapped by Church and Hack and others (Banks, 1990; LeTourneau, 2000). Most of the chert is massive with scattered pebbles but in places also consists of nodular cement within gravel. The siliceous layers compose the informally known “Pedernal chert.” The siliceous horizons are best exposed as outcrop ledges more than 2 m thick near the tapered base of Cerro Pedernal (at an elevation of ~1900 m), but continue southwestward around the western margin of the Jemez Mountains and form much of the summit plateau of the Sierra Nacimiento at the San Pedro Parks (at an elevation of 3100-3200 m; Fig. 4; Church and Hack, 1939). Although sedimentary deep-sea chert and chert replacement of limestone are common rocks, the Pedernal chert is very unusual as a nonmarine occurrence of stratiform silica. The siliceous horizons are very heterogeneous in thickness, color, and texture. Individual layers range from 20 cm to more than 2 m thick. Upper and lower contacts are undulatory and are sharp in some places but gradational through a nodular-chert zone in other places. As Bryan (1939, p. 17) described it: “The chert is commonly white to pearly gray in color though in places the color may vary considerably. Near the base and sometimes near the top the chert shows bands 1/4” to 1/2” thick and is black in color. In places near the top, weathering has changed the color to pink, red, or yellow. The red color also occurs as flecks or spots in the white to pearly gray mass. Generally the yellow color is associated with clear, very translucent phases of the chert. This translucent type usually occurrs in small masses near the top of the bed.” Most exposures consist of vitreous chert (equant, microcrystalline quartz) and chalcedony (fibrous quartz) dominated by translucent gray and yellowish gray colors with patches and swirls of more opaque red, maroon, and black coloration. Discontinuous micritic calcite, in horizons as much as 50 centimeters thick, is present in the lower parts of, or beneath, most siliceous layers. Petrographic observations by Vazzana (1980) and Moore (2000) show evidence of replacement of micritic calcite by both chalcedony and chert, with subsequent infilling of vugs by chalcedony, drusy quartz, or sparry calcite. Although cropping out only in a narrow stratigraphic interval over an area of only 300 km2, chert pebbles and cobbles from this unit are notable in rift-basin and younger valley-fill alluvial deposits southward into the Albuquerque basin, westward into the San Juan basin, and eastward into the Española basin (Fig. 4). The persistence of the siliceous clasts attests to the resistance to weathering and the hardness of Pedernal chert. No researchers have systematically studied the siliceous horizons of the Pedernal member, although Vazzana (1980) and Moore (2000) provided some important observations and data as part of broad studies of the Abiquiu Formation. Vazzana (1980) described mineralogical and whole-rock-geochemical variations within sandy gravel below a Pedernal chert horizon that he ascribed to a buried weathering profile. Along with the widespread replacement of micritic calcite by silica, Vazzana (1980) and Moore (2\",\"PeriodicalId\":345302,\"journal\":{\"name\":\"Geology of the Chama Basin\",\"volume\":\"4 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"3\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Geology of the Chama Basin\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.56577/ffc-56.425\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geology of the Chama Basin","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.56577/ffc-56.425","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 3
摘要
-Cerro Pedernal是一个孤立的玄武岩覆盖的高峰,具有重要的地质和地质考古意义。这座山峰位于科罗拉多高原上,靠近里奥格兰德裂谷的边界。Cerro penal上渐新世-中新世地层单元与裂谷内较厚的剖面相对应,并记录了25ma之前裂谷盆地沉降的开始。新生裂谷边缘沉积的停止或接近停止导致了假设的广泛风化作用和成土钙质层的形成,这些层后来被重叠在裂谷边缘的火山碎屑沉积所掩埋。玻璃质火山碎屑的成岩作用很可能导致二氧化硅取代钙质土壤,形成了石英岩,在新墨西哥州北部人类居住的1.3万多年中,石英岩通常用于制造石器工具。Cerro Pedernal-San Pedro Parks地区大量利用的燧石采石场是重要的岩石材料来源,但在科罗拉多高原和里奥格兰德裂谷的冲积矿床中普遍存在的燧石鹅卵石再沉积也是如此。主要和次要燧石来源的结合使得确定人工制品原材料的确切来源位置的努力变得混乱。火,连同简单的撬动工具和锤石很可能被用来移除大型燧石块,用于制造工具。对铁芯和双面的初步加工产生了大量不规则的薄片和废弃的碎片,一些早期工人误以为是更古老的工具制造文化的成品。图1所示。从北面俯瞰Cerro Pedernal。中新世玄武岩覆盖着一层暴露不良的下第三纪和中第三纪地层的顶端,这些地层从中生代岩石的底部上升起。图片由Lisa W.Huckell提供。[26]史密斯和哈克尔玄武岩流和沿断层的当代岩脉侵入;他们认为阿比基乌盆地的主要裂谷沉降开始于10 Ma左右。然而,Smith等人(2002)指出,玄武岩流保留了Jemez山脉的北向古斜坡,该斜坡被西南倾的断陷盆地充填物侵蚀(图2)。玄武岩与下伏地层之间的角度不整合表明,大多数盆地沉降发生在玄武岩挤压之前。图3显示了Cerro Pedernal地层与里奥格兰德裂谷西部、峰以东仅5 km处Cañones地区地层剖面的对比。Manley(1982)和Moore(2000)绘制的裂谷盆地地层学与Cerro Pedernal未变形剖面的对比突出了前玄武岩裂谷历史的证据。中中新世Tesuque组地层从Cerro Pedernal的约65米急剧增厚到Cañones东南330米,表明在Lobato玄武岩喷发之前,Gonzales和Cañones断层发生了实质性的运动(图2和3)。下伏的阿比基乌组由两个厚段组成,下段为前寒武纪碎屑砾石和砾岩,上段为火山碎屑砂岩和砾岩(Smith, 1938;Vazzana, 1980;摩尔,2000)。下部段在Cerro Pedernal和Cañones之间仅略微增厚,而上部段在Cañones处大约增厚25%(图3)。通过改变火山物源定义的上部段地层细分(Smith, 1995),使Moore(2000)和Smith等人(2002)进一步确定,Cerro Pedernal较薄的部分缺少上部段的最下部,而这些部分在Cañones附近和更东的阿比基乌附近的出头岩层中都有。Cerro Pedernal上段底部出现了25 Ma Amalia凝灰岩碎屑和富含石英和碱长石的砂岩,这些砂岩是由Latir火山田(Taos北部)的凝灰岩和同期火山岩侵蚀而成(Smith et al., 2002;图3)。同样的标记地平线位于Cañones附近上部构件底部上方约15米,位于Abiquiu附近底部上方80米以上(Smith et al., 2002)。这些观测结果表明,在阿比奎组沉积期间,盆地沉降和裂谷边缘断裂正在进行,阿比奎组沉积开始于25 Ma Amalia凝灰岩喷发之前(Smith et al., 2002)。Cerro Pedernal裂谷外约400 m的阿比奎组沉积也暗示了除裂谷-盆地沉降外的其他沉积机制。Moore(2000)和Smith等人(2002)提供了简单的弯曲载荷和沉积物运输模型的结果,这些模型可以通过两种机制部分解释阿比奎组的沉积。首先,同时期的圣胡安和拉蒂尔火山场(分别位于科罗拉多州南部和新墨西哥州中北部)的构造对地壳的负荷可能产生了一个足够大的弯曲护城河,以产生沉积物容纳空间(图2)。 阿比基乌地区的广义地质图,显示了Cerro Pedernal位于科罗拉多高原和里奥格兰德裂谷阿比基乌河口交界处附近(根据Smith et al., 2002)。图3。从Cerro Pedernal向东的渐新世和中新世岩石对比显示,除Pedernal段局限于Cañones断裂下盘外,整个裂谷边缘断裂上的地层突然增厚。断层上的增厚意味着裂谷边缘断层的同沉积运动。底端段的有限分布,以及阿玛利亚凝灰岩碎屑最低面所暗示的上部段最低层的凝析作用,与底端段最初的成土成因相一致。CERRO PEDERNAL在CERRO PEDERNAL地区的地质和考古意义。其次,大量火山喷发产生的火山碎屑沉积物淹没河流可能会导致河流剖面的退化,从而导致该地区的适度淤积。这种火山作用驱动的沉积作用使沉积延伸到新生的裂谷边缘之外,而相对于Cerro Pedernal的剖面,地层增厚进入裂谷,证明了沉积和裂谷盆地沉降的同时代性(Smith et al., 2002)。在Cañones断裂以西的阿比奎乌组露头,基底岩段位于下部和上部岩段之间(图3;布莱恩,1938年,1939年;史密斯,1938;Church and Hack, 1939)。底层是一层4 - 8米厚的砾石层,与下层相似,但最显著的是存在1 - 4个不连续的、不规则的玉髓质和硅质硅体,并伴有不同比例的方解石。图4显示了Church和Hack等人绘制的Pedernal chert成员的大致范围(Banks, 1990;一起,2000)。大多数燧石是块状的,有零散的鹅卵石,但在某些地方也由砾石中的结节状水泥组成。这些硅质层组成了俗称的“石英岩”。在Cerro Pedernal的锥形底部(海拔约1900米)附近,硅质层最适合作为超过2米厚的露头岩架暴露出来,但沿着Jemez山脉的西部边缘继续向西南延伸,并形成了圣佩德罗公园(海拔3100-3200米;图4;Church and Hack, 1939)。虽然沉积的深海燧石和代替石灰岩的燧石是常见的岩石,但作为层状硅石的非海相产状,滨岸燧石是非常罕见的。硅质层在厚度、颜色和结构上都很不均匀。单个层的厚度从20厘米到2米多不等。上下触点是起伏的,在一些地方是尖锐的,但在另一些地方是通过结核-燧石带渐变的。正如Bryan (1939, p. 17)所描述的那样:“燧石通常是白色到珍珠灰色的,尽管在某些地方颜色可能相差很大。在底部附近,有时在顶部附近,燧石显示1/4“到1/2”厚的带,颜色为黑色。在靠近山顶的地方,风化作用使颜色变成了粉红色、红色或黄色。红色也出现在白色到珍珠灰色的肿块中的斑点或斑点。通常黄色与燧石的透明、半透明相联系。这种半透明类型通常出现在靠近床顶的小块体中。”大多数暴露物由玻璃质燧石(等温、微晶石英)和玉髓(纤维石英)组成,以半透明的灰色和黄灰色为主,带有不透明的红色、栗色和黑色斑块和漩涡。不连续的泥晶方解石,在50厘米厚的地层中,存在于大多数硅质层的下部或下方。Vazzana(1980)和Moore(2000)的岩石学观察表明,有证据表明泥晶方解石被玉髓和燧石取代,随后由玉髓、粗砂石英或亮晶方解石填充孔洞。虽然仅在300平方公里的狭窄地层间隔中出现,但该单元的燧石卵石和鹅卵石在裂谷盆地和较年轻的山谷填充冲积矿床中非常明显,向南进入阿尔伯克基盆地,向西进入圣胡安盆地,向东进入Española盆地(图4)。硅质碎屑的持久性证明了贝德尔燧石的耐风化性和硬度。尽管Vazzana(1980)和Moore(2000)提供了一些重要的观察和数据,作为阿比奎组广泛研究的一部分,还没有研究人员系统地研究过Pedernal成员的硅质层位。Vazzana(1980)描述了沉积岩层下砂砾石的矿物学和全岩地球化学变化,他将其归因于埋藏的风化剖面。 随着微晶方解石被二氧化硅广泛取代,Vazzana(1980)和Moore (2 .
The geological and geoarchaeological significance of Cerro Pedernal, Rio Arriba County, New Mexico
—Cerro Pedernal is an isolated basalt-capped peak of substantial geologic and geoarchaeological significance. The peak is located on the Colorado Plateau near the boundary of the Rio Grande rift. Oligocene-Miocene stratigraphic units on Cerro Pedernal correlate to thicker sections within the rift and document initiation of rift-basin subsidence before 25 Ma. Cessation or near cessation of sedimentation on the nascent rift margin led to hypothesized extensive weathering and formation of pedogenic calcrete horizons that were later buried by volcaniclastic deposits that overlapped the rift margin. Diagenesis of vitric volcaniclastic detritus likely led to silica replacement of the calcareous soils to form the Pedernal chert, which was commonly used for lithic-tool manufacture for more than 13 millennia of human occupation in northern New Mexico. Heavily utilized chert quarries in the Cerro Pedernal-San Pedro Parks region were important lithic-material sources, but so were redeposited cobbles of chert that are ubiquitous in alluvial deposits on the Colorado Plateau and in the Rio Grande rift. The combination of primary and secondary chert sources has confounded efforts to determine the exact source locations of artifact raw materials. Fire, along with simple prying tools and hammerstones were likely used to dislodge large chert pieces for tool manufacture. Preliminary working of cores and bifaces produced large volumes of irregular flakes and rejected pieces that were mistaken by some early workers as finished products of more ancient tool-making cultures. FIGURE 1. View of Cerro Pedernal from the north. Miocene basalt caps a pinnacle of poorly exposed lower and middle Tertiary strata that rise above a base of Mesozoic rocks. Photo courtesy of Lisa W.Huckell. 426 SMITH AND HUCKELL Basalt flows and the intrusion of contemporary dikes along faults; they proposed that principal rift-basin subsidence in the Abiquiu embayment initiated at about 10 Ma. Smith et al. (2002) point out, however, that the basalt flows preserve a northward paleoslope from the Jemez Mountains that was eroded on southwest-dipping rift-basin fill (Fig. 2). The angular unconformity between the basalt and underlying strata implies that most basin subsidence occurred before basalt extrusion. Figure 3 illustrates the correlation of Cerro Pedernal stratigraphy to the stratigraphic section in the Cañones area in the western Rio Grande rift and only 5 km east of the peak. The correlation of rift-basin stratigraphy mapped by Manley (1982) and Moore (2000) to the undeformed section at Cerro Pedernal highlights evidence for the pre-basalt rifting history. Middle Miocene strata of the Tesuque Formation thicken dramatically from about 65 m at Cerro Pedernal to 330 m southeast of Cañones, indicating substantial movement on the Gonzales and Cañones faults (Figs. 2 and 3) before eruption of the Lobato Basalt. The underlying Abiquiu Formation consists of two thick members, a lower member of Precambrian-clast gravel and conglomerate, and an upper member of volcaniclastic sandstone and conglomerate (Smith, 1938; Vazzana, 1980; Moore, 2000). The lower member thickens only slightly between Cerro Pedernal and Cañones, whereas the upper member is roughly 25% thicker at Cañones (Fig. 3). Recognition of stratigraphic subdivisions within the upper member defined by changing volcanic provenance (Smith, 1995), allowed Moore (2000) and Smith et al. (2002) to further determine that the thinner section at Cerro Pedernal lacks the lowermost parts of the upper member that are present in outcrop near Cañones and farther east near Abiquiu. Clasts of the 25 Ma Amalia Tuff and sandstones with abundant quartz and alkali feldspar eroded from the tuff and coeval volcanic rocks of the Latir volcanic field (north of Taos, NM) occur at the base of the upper member at Cerro Pedernal (Smith et al., 2002; Fig. 3). This same marker horizon is about 15 m above the base of the upper member near Cañones and is more than 80 m above the base near Abiquiu (Smith et al., 2002). These observations imply that basin subsidence and rift-margin faulting were underway during Abiquiu Formation deposition, which commenced in this area before eruption of the 25 Ma Amalia Tuff (Smith et al., 2002). Deposition of approximately 400 m of Abiquiu Formation outside of the rift at Cerro Pedernal also implies aggradation mechanisms other than rift-basin subsidence. Moore (2000) and Smith et al. (2002) provide the results of simple flexural-loading and sediment-transport models that can partially account for deposition of the Abiquiu Formation by two mechanisms. First, the loading of the crust by construction of the coeval San Juan and Latir volcanic fields (in southern Colorado and north-central New Mexico, respectively) likely produced a flexural moat of sufficient dimensions to produce sediment accommodation space FIGURE 2. Generalized geologic map of the Abiquiu region showing the location of Cerro Pedernal near the boundary between the Colorado Plateau and the Abiquiu embayment of the Rio Grande rift (after Smith et al., 2002). FIGURE 3. Correlation of Oligocene and Miocene rocks eastward from Cerro Pedernal shows abrupt thickening of strata across rift-margin faults, except for the Pedernal member, which is restricted to the footwall of the Cañones fault. Thickening across faults implies syndepositional movement on rift-margin faults. The restricted distribution of the Pedernal member, along with condensation of the lowest strata of the upper member implied by the lowest appearance of Amalia Tuff clasts, is consistent with an initial pedogenic origin for the Pedernal member. 427 GEOLOGICAL AND GEOARCHAEOLOGICAL SIGNIFICANCE OF CERRO PEDERNAL in the Cerro Pedernal area. Second, the inundation of rivers by large volumes of volcanically produced pyroclastic sediment would likely lead to regrading of river profiles that would cause modest aggradation in this region. This volcanism-driven aggradation allowed sedimentation to extend beyond the nascent rift margin, whereas stratigraphic thickening into the rift, relative to the section at Cerro Pedernal, demonstrates the contemporaneity of deposition and rift-basin subsidence (Smith et al., 2002). Nature and Origin of the “Pedernal Chert” In Abiquiu Formation outcrops west of the Cañones fault, the Pedernal member is present between the lower and upper members (Fig. 3; Bryan, 1938, 1939; Smith, 1938; Church and Hack, 1939). The Pedernal member is a 4to 8-m thick interval of gravel that resembles the lower member but is notable for the presence of one to four, discontinuous, irregular bodies of chalcedonic and cherty silica with varying proportions of associated calcite. Figure 4 presents the approximate extent of the Pedernal chert member as mapped by Church and Hack and others (Banks, 1990; LeTourneau, 2000). Most of the chert is massive with scattered pebbles but in places also consists of nodular cement within gravel. The siliceous layers compose the informally known “Pedernal chert.” The siliceous horizons are best exposed as outcrop ledges more than 2 m thick near the tapered base of Cerro Pedernal (at an elevation of ~1900 m), but continue southwestward around the western margin of the Jemez Mountains and form much of the summit plateau of the Sierra Nacimiento at the San Pedro Parks (at an elevation of 3100-3200 m; Fig. 4; Church and Hack, 1939). Although sedimentary deep-sea chert and chert replacement of limestone are common rocks, the Pedernal chert is very unusual as a nonmarine occurrence of stratiform silica. The siliceous horizons are very heterogeneous in thickness, color, and texture. Individual layers range from 20 cm to more than 2 m thick. Upper and lower contacts are undulatory and are sharp in some places but gradational through a nodular-chert zone in other places. As Bryan (1939, p. 17) described it: “The chert is commonly white to pearly gray in color though in places the color may vary considerably. Near the base and sometimes near the top the chert shows bands 1/4” to 1/2” thick and is black in color. In places near the top, weathering has changed the color to pink, red, or yellow. The red color also occurs as flecks or spots in the white to pearly gray mass. Generally the yellow color is associated with clear, very translucent phases of the chert. This translucent type usually occurrs in small masses near the top of the bed.” Most exposures consist of vitreous chert (equant, microcrystalline quartz) and chalcedony (fibrous quartz) dominated by translucent gray and yellowish gray colors with patches and swirls of more opaque red, maroon, and black coloration. Discontinuous micritic calcite, in horizons as much as 50 centimeters thick, is present in the lower parts of, or beneath, most siliceous layers. Petrographic observations by Vazzana (1980) and Moore (2000) show evidence of replacement of micritic calcite by both chalcedony and chert, with subsequent infilling of vugs by chalcedony, drusy quartz, or sparry calcite. Although cropping out only in a narrow stratigraphic interval over an area of only 300 km2, chert pebbles and cobbles from this unit are notable in rift-basin and younger valley-fill alluvial deposits southward into the Albuquerque basin, westward into the San Juan basin, and eastward into the Española basin (Fig. 4). The persistence of the siliceous clasts attests to the resistance to weathering and the hardness of Pedernal chert. No researchers have systematically studied the siliceous horizons of the Pedernal member, although Vazzana (1980) and Moore (2000) provided some important observations and data as part of broad studies of the Abiquiu Formation. Vazzana (1980) described mineralogical and whole-rock-geochemical variations within sandy gravel below a Pedernal chert horizon that he ascribed to a buried weathering profile. Along with the widespread replacement of micritic calcite by silica, Vazzana (1980) and Moore (2