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Abundances of Cl, F, H, and S in Apatites From SNC Meteorites

Channon, M. B. and Boyce, J. W. and Stolper, E. M. and Eiler, J. M. (2011) Abundances of Cl, F, H, and S in Apatites From SNC Meteorites. Meteoritics and Planetary Science, 46 (S1). A39-A39. ISSN 1086-9379.

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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.

Item Type:Article
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Stolper, E. M.0000-0001-8008-8804
Additional Information:© 2011 The Meteoritical Society. Article first published online: 25 Jul. 2011.
Issue or Number:S1
Record Number:CaltechAUTHORS:20130806-110936227
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Official Citation:(2011), 74th Annual Meeting of the Meteoritical Society, August 8–12, 2011, London, U.K. Meteoritics & Planetary Science, 46: A3–A264. doi: 10.1111/j.1945-5100.2011.01221.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:39783
Deposited By: Tony Diaz
Deposited On:09 Aug 2013 18:51
Last Modified:03 Oct 2019 05:10

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