Ries magnetic mineralogy: Exploring impact and post-impact evolution of crater magnetism

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Bruno Daniel Leite Mendes, Agnes Kontny, Katarzyna Dudzisz, Franziska D. H. Wilke
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Abstract

Large-scale impact events are some of the most catastrophic and instantaneous geological processes in nature, and leave in their wake conspicuous geological structures with characteristic magnetic anomalies. Despite magnetic anomalies in craters being well-documented, their relationship with the magnetic mineral composition of the target and impactites is not always straightforward. Furthermore, the influence of impact shock and post-impact events in the magnetism of natural craters remains elusive. In the Ries crater, Germany, the negative magnetic anomalies are attributed to a reverse polarity remanent magnetization in the impact-melt bearing lithologies. We report new chemical, rock-, and mineral-magnetic data from the shocked basement and impactites, from surface samples, NR73 and SUBO-18 boreholes, and explore how temperature and hydrothermalism may influence the magnetic mineralogy in the crater. We identified shocked, pure magnetite in the basement, and low-cation substituted magnetite in the impactites as the main magnetic carriers. The shocked basement is demagnetized but remains largely unaltered by post-impact hydrothermalism, while the impactites show weak magnetization and are extensively altered by neutral-to-reducing post-impact hydrothermalism. We suggest that the magnetic mineralogy of the demagnetized uplifted basement may contribute significantly to the magnetic anomaly variation, in line with recent findings from the Chicxulub peak-ring.

Abstract Image

里斯磁性矿物学:探索撞击和撞击后陨石坑磁性的演变
大规模的撞击事件是自然界中最具灾难性和瞬时性的地质过程,并在其后留下明显的地质结构和特征性磁异常。尽管陨石坑中的磁异常已被详细记录,但它们与目标和撞击岩的磁性矿物成分之间的关系并不总是那么简单明了。此外,撞击冲击和撞击后事件对天然陨石坑磁性的影响仍然难以捉摸。在德国的里斯陨石坑,负磁性异常被归因于含有撞击熔融物的岩性中的反极性剩磁。我们报告了来自冲击基底和冲击岩、地表样本、NR73 和 SUBO-18 钻孔的新化学、岩石和矿物磁性数据,并探讨了温度和热液如何影响陨石坑中的磁性矿物学。我们确定基底中的冲击纯磁铁矿和撞击岩中的低阳离子替代磁铁矿是主要的磁性载体。冲击基底已经退磁,但基本上没有受到冲击后热液作用的改变,而撞击岩则显示出弱磁化,并受到中性到还原性冲击后热液作用的广泛改变。我们认为,消磁的隆起基底的磁矿物学可能在很大程度上导致了磁异常的变化,这与奇克苏卢布峰环的最新发现一致。
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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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