Published July 2011
| Published
Journal Article
Open
Abundances of Cl, F, H, and S in Apatites From SNC Meteorites
Chicago
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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.Attached Files
Published - Eiler_2010pA39.pdf
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Additional details
- Eprint ID
- 39783
- DOI
- 10.1111/j.1945-5100.2011.01221.x
- Resolver ID
- CaltechAUTHORS:20130806-110936227
- Created
-
2013-08-09Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)