Comparing detrital zircon U-Pb age data to determine provenance relationships of Upper Cretaceous strata southwest NewMexico and southeast Arizona

J. Gilbert, T. Lawton
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Abstract

Analysis of detrital zircon U-Pb age data of the Early Cretaceous Hell-to-Finish Formation of the Little Hatchet Mountains in New Mexico and the Late Jurassic Glance Conglomerate and Early Cretaceous Morita Formation of the Huachuca Mountains in Arizona indicates different provenance histories. Formerly, the Hell-to-Finish Formation has been considered genetically similar and correlative with the redbeds of the Glance Conglomerate and Morita Formation based on outcrop appearance and stratigraphic position. In the SW Huachuca Mountains, a detrital zircon sample from a volcanic litharenite high in the Glance Conglomerate contains dominantly Early to Middle Jurassic grains (81 of 96 grains) derived from underlying volcanic rocks. Unconformably overlying the Glance Conglomerate, the lower Morita Formation transitions from nearshore facies rocks at the base to fluvial facies rocks. A detrital zircon sample of 90 grains from a nearshore subarkose contains mostly Triassic (n=12) and Proterozoic grains (n=60) but only a few Early Jurassic grains (n=6), reflecting burial or late stage erosion of Jurassic rocks. Higher in the section, a fluvial volcanic litharenite contains abundant Cretaceous grains (ca. 145 – 120 Ma) from the arrival of volcanic material to the west. In the Little Hatchet Mountains, the lower Hell-to-Finish Formation is fluvial, and the sandstones are litharenites that contain abundant chert and carbonate clasts and no volcanic fragments. A detrital zircon sample of the Hell-to-Finish Formation is composed almost exclusively of pre-Triassic grains (78 of 79 grains) and was sourced from the Burro uplift to the north. In contrast, the Morita Formation received a significant component of material from a western source that is not reflected in the Hell-to-Finish Formation, suggesting the basins were isolated. Material for the Glance Conglomerate was locally derived and is not an input for the Hell-to-Finish Formation.
对比碎屑锆石U-Pb年龄数据,确定新墨西哥州西南部和亚利桑那州东南部上白垩统地层物源关系
新墨西哥州小哈切特山早白垩世Hell-to-Finish组与美国亚利桑那州华楚卡山晚侏罗世Glance砾岩和早白垩世森田组碎屑锆石U-Pb年龄分析表明,物源历史不同。以前,根据露头形态和地层位置,认为Hell-to-Finish组与Glance砾岩和Morita组红层具有遗传相似性和相关性。在华楚卡山西南部的Glance砾岩中,一个火山岩屑岩的碎屑锆石样品主要含有早-中侏罗统(96粒中有81粒)的火山岩颗粒。下森田组不整合覆于Glance砾岩之上,由基底近岸相岩向河流相岩过渡。来自近岸亚长砂岩的90粒碎屑锆石样品中,主要含有三叠纪(n=12)和元古代(n=60)颗粒,但只有少量早侏罗世(n=6)颗粒,反映了侏罗纪岩石的埋藏或晚期侵蚀作用。在剖面的较高位置,一条河流火山岩岩屑岩含有大量的白垩纪颗粒(约145 - 120 Ma),这些颗粒来自火山物质的到达。小哈切特山下部“地狱至完成”组为河流沉积,砂岩为岩屑岩,含丰富的燧石和碳酸盐碎屑,无火山碎屑。地狱至完工组的碎屑锆石样品几乎完全由前三叠纪颗粒组成(79粒中的78粒),来自北部的Burro隆起。相比之下,森田组从西部吸收了大量物质,而这些物质在“地狱至完工”组中没有反映出来,这表明这些盆地是孤立的。Glance砾岩的材料来自当地,而不是“难以完成”地层的原料。
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