On the isotopic chemistry of carbon at the Martian surface
On the isotopic chemistry of carbon at the Martian surface
复制标题
火星表面碳的同位素化学
DOI：
10.1098/rsta.1994.0134
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发表时间：
1994
期刊：
影响因子：
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通讯作者：
C. Pillinger
中科院分区：
文献类型：
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作者：
I. Wright;C. Pillinger
简要概述了利用陨石了解火星本身的可能性，陨石被认为是火星起源的。文章还给出了认为这些样本是火星后裔的主要原因。作为可以通过分析火星陨石获得的各种信息的一个例子，本文讨论了以前未发表的对冲击产生的玻璃中碳的研究结果，该玻璃来自一个特定的样本。这些实验数据被用来洞察利用同位素数据理解火星上的碳循环的潜力。
A brief overview is presented concerning the possibilities of using meteorites, that are thought to have a Martian origin, to learn something about Mars itself. The main reasons for believing the samples are of Martian descent are also given. As an example of the sorts of information that can be obtained by analysing Martian meteorites, previously unpublished results from a study of the carbon in shock-produced glass from one particular sample are discussed. The experimental data are used to give an insight into the potential of using isotopic data to comprehend the carbon cycle on Mars.
影响因子：
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作者：
T. Owen;K. Biemann;D. R. Rushneck;J. Biller;D. W. Howarth;A. Lafleur
通讯作者：
T. Owen;K. Biemann;D. R. Rushneck;J. Biller;D. W. Howarth;A. Lafleur