Origin of a polymict, mega-clast-bearing impact breccia in the crater floor of Wetumpka Impact Structure, Elmore County, Alabama: Insights from surface outcrops and a drill core

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Neeraja S. Chinchalkar, David T. King Jr, Willis E. Hames
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Abstract

Wetumpka impact structure is a Late Cretaceous, marine-target impact crater of about 5 km diameter. The apparent crater rim is mostly made of crystalline local basement, and the apparent crater floor consists of a mixed sediments of target lithology. These sediments are the provenance of the crater-filling impactite sands, overlying trans-crater slide unit, and the capping polymict impact breccia deposit, often referred to by previous workers as “central polymict breccia.” The unit has been known to contain elongated mega-clasts of up to tens of meters in size. This study attempted to understand the mode of emplacement of this polymict breccia, which occurs in some places on the apparent crater floor and resembles a polymict proximal ejecta deposit. This work also reports the first documentation of rare, potential impact spherules in the polymict impact breccia, interpreted to be a part of distal ejecta. The presence of large, decimeter-sized clasts in the breccia can be best explained by the movement of overturned rim flap forming part of proximal ejecta from the crater rim to the apparent crater floor during early modification stage of impact cratering. Our work highlights the bimodal clast size distribution of the polymict breccia, and so we propose that the term “mega-clast-bearing impact breccia” be used for this unit. We attribute a generally steep orientation of the decameter sized clasts to primary imbrication during emplacement. The emplacement of this breccia is interpreted as associated with the ejecta emplacement process that occurred before the return of marine resurge.

Abstract Image

阿拉巴马州埃尔莫尔县韦坦普卡撞击结构陨石坑底部多岩体、巨型碎屑岩撞击角砾岩的起源:地表露头和钻孔岩芯的启示
韦坦普卡撞击结构是一个白垩纪晚期的海洋目标撞击坑,直径约 5 千米。明显的陨石坑边缘主要由当地的结晶基底构成,明显的陨石坑底部由目标岩性的混合沉积物组成。这些沉积物是填满陨石坑的撞击岩砂、上覆跨陨石坑滑动单元和覆盖的多岩体撞击角砾岩沉积物(以前的工作者通常称之为 "中央多岩体角砾岩")的产状。据了解,该单元包含长达数十米的细长巨型碎屑岩。这项研究试图了解这种多岩浆角砾岩的堆积方式,这种角砾岩出现在明显的陨石坑底部的某些地方,类似于多岩浆近端喷出沉积物。这项工作还首次记录了多岩体撞击角砾岩中罕见的潜在撞击球,被解释为远端喷出物的一部分。角砾岩中存在分米大小的大型碎屑的最佳解释是,在撞击陨石坑的早期改造阶段,形成近端喷出物一部分的翻转边缘瓣从陨石坑边缘移动到明显的陨石坑底部。我们的研究突出了多岩屑角砾岩的双峰碎屑分布,因此我们建议将这一单元称为 "巨型碎屑冲击角砾岩"。我们认为,十米大小的碎屑岩普遍呈陡峭走向,是由于在成岩过程中发生了原生交错作用。据解释,这种角砾岩的成岩过程与海洋重现之前的喷出物成岩过程有关。
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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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