Suppr超能文献

碳质球粒陨石中的水:火星存在水圈的证据。

Water in SNC meteorites: evidence for a martian hydrosphere.

作者信息

Karlsson H R, Clayton R N, Gibson E K, Mayeda T K

机构信息

Planetary Science Branch, National Aeronautics and Space Administration, Johnson Space Center, Houston, TX 77058.

出版信息

Science. 1992 Mar 13;255:1409-11. doi: 10.1126/science.11537889.

Abstract

The Shergotty-Nakhla-Chassigny (SNC) meteorites, purportedly of martian origin, contain 0.04 to 0.4 percent water by weight. Oxygen isotopic analysis can be used to determine whether this water is extraterrestrial or terrestrial. Such analysis reveals that a portion of the water is extraterrestrial and furthermore was not in oxygen isotopic equilibrium with the host rock. Lack of equilibrium between water and host rock implies that the lithosphere and hydrosphere of the SNC parent body formed two distinct oxygen isotopic reservoirs. If Mars was the parent body, the maintenance of two distinct reservoirs may result from the absence of plate tectonics on the planet.

摘要

舍戈蒂-纳赫拉-沙西尼(SNC)陨石据称起源于火星,其重量含0.04%至0.4%的水。氧同位素分析可用于确定这种水是来自外星还是地球。这种分析表明,一部分水是外星的,而且与母岩不存在氧同位素平衡。水与母岩之间缺乏平衡意味着SNC母体的岩石圈和水圈形成了两个不同的氧同位素储库。如果火星是母体,两个不同储库的维持可能是由于该行星不存在板块构造。

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验