Published July 2011 | Version Published
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Abundances of Cl, F, H, and S in Apatites From SNC Meteorites

Abstract

Magmatic volatiles influence igneous phase equilibria, eruptive behavior, atmospheric composition, and climate. Several lines of evidence suggest that Mars is rich in halogens and S relative to Earth. However, magmatic volatile abundances and their effects on magmatic processes on Mars are controversial. Here we examine igneous apatites in SNC meteorites as indicators of magmatic volatile abundances.

Additional Information

© 2011 The Meteoritical Society. Article first published online: 25 Jul. 2011.

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Identifiers

Eprint ID
39783
DOI
10.1111/j.1945-5100.2011.01221.x
Resolver ID
CaltechAUTHORS:20130806-110936227

Dates

Created
2013-08-09
Created from EPrint's datestamp field
Updated
2021-11-09
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Caltech groups
Division of Geological and Planetary Sciences (GPS)