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9000 万个撞击坑揭示的 depleted shergottites 中 Tharsis 地幔源

The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters.

机构信息

Space Science and Technology Centre, School of Earth and Planetary Science, Curtin University, Perth, WA, Australia.

Department of Earth and Planetary Sciences, Western Australian Museum, Perth, WA, Australia.

出版信息

Nat Commun. 2021 Nov 3;12(1):6352. doi: 10.1038/s41467-021-26648-3.

Abstract

The only martian rock samples on Earth are meteorites ejected from the surface of Mars by asteroid impacts. The locations and geological contexts of the launch sites are currently unknown. Determining the impact locations is essential to unravel the relations between the evolution of the martian interior and its surface. Here we adapt a Crater Detection Algorithm that compile a database of 90 million impact craters, allowing to determine the potential launch position of these meteorites through the observation of secondary crater fields. We show that Tooting and 09-000015 craters, both located in the Tharsis volcanic province, are the most likely source of the depleted shergottites ejected 1.1 million year ago. This implies that a major thermal anomaly deeply rooted in the mantle under Tharsis was active over most of the geological history of the planet, and has sampled a depleted mantle, that has retained until recently geochemical signatures of Mars' early history.

摘要

地球上唯一的火星岩石样本来自于小行星撞击火星表面后抛出的陨石。这些陨石的发射地点及其地质背景目前尚不清楚。确定撞击地点对于揭示火星内部演化与其表面之间的关系至关重要。在这里,我们采用了一种撞击坑检测算法,该算法编制了一个包含 9000 万个撞击坑的数据库,通过观察二次撞击坑场,可以确定这些陨石的潜在发射位置。我们的研究表明,位于塔尔西斯火山省的图廷和 09-000015 陨石坑最有可能是 110 万年前喷出的亏损型辉玻陨石的来源。这意味着,在塔尔西斯下方地幔深处的一个主要热异常在火星的大部分地质历史中一直活跃,并从地幔中提取了一种亏损型物质,直到最近才保留了火星早期历史的地球化学特征。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8f74/8566585/cbf2be7258c4/41467_2021_26648_Fig1_HTML.jpg

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