Volatility in Martian magmas

Harry Y. McSween
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Harry Y. McSween: University of Tennessee, Knoxville, Tennessee 37996-1410, USA. mcsween@utk.edu

Nature, 2009, vol. 458, issue 7234, 45-45

Abstract: The geochemistry of the Martian surface has largely been determined by the eruption of magmas to form basaltic rocks. A new line of argument has chlorine as an influential agent in that process.

Date: 2009
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DOI: 10.1038/458045a

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