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来自早期亚马逊火星的独特陨石:富含水的玄武质角砾岩 西北非 7034.

Unique meteorite from early Amazonian Mars: water-rich basaltic breccia Northwest Africa 7034.

机构信息

Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA.

出版信息

Science. 2013 Feb 15;339(6121):780-5. doi: 10.1126/science.1228858. Epub 2013 Jan 3.

Abstract

We report data on the martian meteorite Northwest Africa (NWA) 7034, which shares some petrologic and geochemical characteristics with known martian meteorites of the SNC (i.e., shergottite, nakhlite, and chassignite) group, but also has some unique characteristics that would exclude it from that group. NWA 7034 is a geochemically enriched crustal rock compositionally similar to basalts and average martian crust measured by recent Rover and Orbiter missions. It formed 2.089 ± 0.081 billion years ago, during the early Amazonian epoch in Mars' geologic history. NWA 7034 has an order of magnitude more indigenous water than most SNC meteorites, with up to 6000 parts per million extraterrestrial H(2)O released during stepped heating. It also has bulk oxygen isotope values of Δ(17)O = 0.58 ± 0.05 per mil and a heat-released water oxygen isotope average value of Δ(17)O = 0.330 ± 0.011 per mil, suggesting the existence of multiple oxygen reservoirs on Mars.

摘要

我们报告了火星陨石 NWA 7034 的数据,它与 SNC(即辉玻陨石、辉橄无球粒陨石和钙长辉长无球粒陨石)群组中已知的火星陨石具有一些岩石学和地球化学特征,但也具有一些独特的特征,使其无法归入该群组。NWA 7034 是一种地球化学上富集的壳层岩石,组成上类似于玄武岩和最近的 Rover 和轨道器任务测量的平均火星地壳。它形成于 20.89 ± 0.081 亿年前,处于火星地质历史上的早期亚马逊纪。NWA 7034 比大多数 SNC 陨石具有数量级更多的原生水,在逐步加热过程中释放出多达 6000 个 ppm 的天外 H(2)O。它还具有 0.58 ± 0.05‰的 Δ(17)O 整体氧同位素值和 0.330 ± 0.011‰的释放水氧同位素平均值,表明火星上存在多个氧储库。

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