印度达拉撞击构造的单角砾岩就位和陨石坑大小估计

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Meteoritics & Planetary Science Pub Date : 2025-02-14 DOI:10.1111/maps.14323
Sonal Tiwari, Gaurav Joshi, Pradyut Phukon, Amar Agarwal, Mamilla Venkateshwarlu
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引用次数: 0

摘要

在达拉撞击构造中,单粒角砾岩与撞击熔融岩露头接近。一般来说,这些冲击岩岩性是由不同的机制在火山口的不同部位形成的。对达拉地区冲击熔融岩的侵位背景进行了较深入的研究。因此,我们利用野外、显微和磁组构研究了单粒角砾岩的侵位。结果表明,单片角砾岩的岩石磁性参数强度与达拉未受冲击的目标花岗岩类相当。因此,磁性织物是在预冲击过程中形成的,不会因冲击而改变。磁性织物没有重新定向,表明峰值冲击压力低于0.5 GPa。这种冲击压力通常存在于陨石坑壁/底附近或陨石坑外。此外,在同一露头的不同位置,磁性织物的取向没有局部变化。因此,单粒角砾岩没有从撞击前的位置移位。根据激波气压测量和没有位移,我们认为现在的单粒角砾岩环形露头位于最后的陨石坑外。此外,单一角砾岩环形露头环的内径约为4.5 km,并与陨石坑内形成的撞击熔融岩并列(先前的研究)。因此,我们认为现在的陨石坑直径约为4.5公里。
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Emplacement of monomict breccia and crater size estimate at the Dhala impact structure, India

At the Dhala impact structure, the monomict breccia and the impact melt rock outcrops are present in proximity. Generally, these impactite lithologies are formed by different mechanisms and in different parts of the crater. The emplacement setting of impact melt rocks at Dhala has been well studied. Therefore, we studied the emplacement of monomict breccia using field, microscopic, and magnetic fabric investigations. Our results show that the intensities of the rock magnetic parameters in monomict breccia are comparable with the unshocked target granitoid at Dhala. Thus, the magnetic fabrics developed during pre-impact processes and were not altered due to impact. The absence of the reorientation of magnetic fabrics indicates that the peak shock pressures were below 0.5 GPa. Such shock pressures typically exist near the crater wall/floor or outside the crater. Moreover, there is no local variation in the orientations of magnetic fabrics at different locations in the same outcrop. Thus, the monomict breccia was not displaced from their pre-impact position. Based on the shock barometry and absence of displacement, we propose that the present-day annular outcrops of monomict breccia are located just outside the final crater. Furthermore, the monomict breccia annular outcrop ring has an internal diameter of ~4.5 km and is juxtaposed with impact melt rocks, which formed within the crater (previous studies). We, thus, suggest that the present-day crater diameter is ~4.5 km.

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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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