德国里厄斯火山口沸石记录的温度和压力条件的多样性

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Meteoritics & Planetary Science Pub Date : 2024-11-07 DOI:10.1111/maps.14282
A. C. Stadermann, T. M. Erickson, L. B. Seifert, Y. Chang, Z. Zeszut, T. J. Zega, Z. D. Michels, J. J. Barnes
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引用次数: 0

摘要

岩石学和微观结构分析可以限制岩石在撞击过程中所经历的温度和压力条件,这对于提供撞击过程的地面真相至关重要。苏威岩是一种多晶岩,是德国里斯陨石坑特有的含熔融撞击角砾岩。关于浮岩的形成和就位,有一些相互竞争的模型,比如从火山口边缘喷出的碎屑流,或者喷出的羽流向后退去。温石内部颗粒记录的温度和压力路径的知识可以帮助区分这些模型和其他模型。辅助相锆石(ZrSiO4)及其高压多晶reidite在这种情况下特别有用,因为它们是高度难熔矿物,可以记录撞击事件的高温和/或高压条件。在这里,我们提供的证据表明,在一个单一的细石英截面的锆石颗粒中记录了广泛的温度和压力条件。本研究的锆石范围从未震到高震(>53 GPa),记录温度超过1673°C。这些发现证实了之前的研究结论,即在最初的冲击压缩和挖掘过程中,suveites包含的材料暴露在非常不同的压力和温度条件下,但总体上不会经历极端温度(1673°C)或压力(30gpa)。
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A diversity of temperature and pressure conditions recorded by zircon within suevite from Ries crater, Germany

The temperature and pressure conditions experienced by rocks during an impact event can be constrained using petrologic and microstructural analysis and is crucial to providing ground truth to the impact cratering process. Suevite is a polymict, impact melt-bearing breccia, specific to Ries crater in Germany. There are competing models for suevite formation and emplacement, such as clastic flows pushed out of the crater rim or ejecta plume fallback. Knowledge of the temperature and pressure pathways recorded by grains within the suevite can help distinguish between these and other models. The accessory phase zircon (ZrSiO4) and its high-pressure polymorph reidite are particularly useful in such circumstances as they are highly refractory minerals that can record the high-temperature and/or high-pressure conditions of an impact event. Here, we present evidence for a wide array of temperature and pressure conditions recorded in zircon grains within a single thin section of suevite. Zircons in this study range from unshocked to highly shocked (>53 GPa), and record temperatures more than 1673°C. These findings confirm previous studies concluding that suevites contain material exposed to very diverse pressure and temperature conditions during initial shock compression and excavation but do not, as a whole, experience extreme temperatures (>1673°C) or pressures (>30 GPa).

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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.
期刊最新文献
Issue Information Cover 2004 Barringer Medal for Peter Schultz A reappraisal of the petrogenesis of Apollo 17 lunar dunites 72415-72417: Relics of the deep lunar mantle? 2007 Service Award for John Schutt
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