Detrital zircon evidence for derivation of arkosic sand in the eolilan Narbona Pass Member of the Eocene-Oligocene Chuska Sandstone from Precambrian basement rocks in central Arizona

W. Dickinson, S. Cather, G. Gehrels, K. Zeigler
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引用次数: 11

Abstract

The Narbona Pass Member of the Chuska Sandstone, exposed only along the crest of the Chuska Mountains (Arizona–New Mexico), is the central remnant of the Oligocene Chuska erg, which is inferred to have occupied ~125,000 km2 of the southeastern Colorado Plateau within a subcircular area surrounded by Oligocene volcanic fields. The high paleotopography of active volcanic edifices delimited the lateral extent of erg deposition except to the west, which was upwind for eolian sand transport. The dominant arkosic petrofacies of the Narbona Pass Member, as exposed at Narbona Pass near Crystal (NM) and at Buffalo Pass near Lukachukai (AZ), was derived mainly from Precambrian basement in central Arizona. The principal subpopulations of detrital zircons (n=100 grains) by U-Pb age are 1770-1640 Ma (~70% with age peak at 1700 Ma), reflecting derivation from the Yavapai-Mazatzal belt of southwest Laurentia, and 1460-1400 Ma (~15% with age peak at 1425 Ma) derived from anorogenic granite bodies intrusive into Yavapai-Mazatzal basement. Precambrian detritus was apparently carried northward to alluvial plains deposited west of the Chuska erg and deflated to feed sand into the erg interior. Other remnants of the Chuska erg along the northern flank of the Mogollon-Datil volcanic field, in the subsurface of the Albuquerque basin of the Rio Grande rift, and near Whiskey Lake in the southernmost Chuska Mountains are petrographically distinct from the arkosic petrofacies of the erg interior, and were evidently derived from other sources as yet untested by detrital zircons. The areal variability of erg sand implies either different pathways for sand transport across the expanse of an integrated Chuska erg or segmentation of the Chuska erg into multiple subdivisions that were partly separated by inselbergs of the pre-Oligocene erg substratum.
亚利桑那中部前寒武纪基底岩石中始新统-渐新统Chuska砂岩风兰纳博纳山口段粗砂岩演化的碎屑锆石证据
恰斯卡砂岩的纳博纳山口段,仅沿恰斯卡山脉(亚利桑那州-新墨西哥州)的山顶露出,是渐新世恰斯卡砂岩的中心遗迹,据推测,它占据了科罗拉多高原东南部约125,000平方公里,位于一个被渐新世火山场包围的亚圆形区域内。活火山构造的高古地形限定了砂岩沉积的侧向范围,除了向西为风成沙输运的逆风外。在靠近Crystal (NM)的Narbona山口和靠近Lukachukai (AZ)的Buffalo山口,Narbona山口段的主要岩相来源于美国亚利桑那州中部的前寒武纪基底。根据U-Pb年龄,碎屑锆石(n=100粒)的主要亚群为1770 ~ 1640 Ma(~70%,年龄峰值为1700 Ma),反映了其来源于Laurentia西南部的yavaphai - mazatzal带,1460 ~ 1400 Ma(~15%,年龄峰值为1425 Ma)来源于侵入yavaphai - mazatzal基底的造山花岗岩体。前寒武纪的碎屑显然被带到北部的冲积平原,沉积在丘斯卡盆地西部,并被压缩成沙子进入盆地内部。沿着mogolon - datil火山场北侧、里约热内卢大裂谷的Albuquerque盆地地下以及Chuska山脉最南端的威士忌湖附近的其他Chuska erg遗迹,在岩石学上与erg内部的黑岩相截然不同,显然来自其他来源,但尚未经过碎屑锆石的检验。砾石砂的面积变变性表明,砾石砂在整个丘斯卡砾石上的输运路径不同,或者被丘斯卡砾石分割成多个小块,这些小块被前渐新世砾石基底的小块部分隔开。
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