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Characterizing Early Solar System Fluids on the Allende (CV3) Parent Body: Nanosims Study of Phosphate Volatile Contents

Dyl, K. A. and Boyce, J. W. and Guan, Y. and Bland, P. A. and Eiler, J. M. (2014) Characterizing Early Solar System Fluids on the Allende (CV3) Parent Body: Nanosims Study of Phosphate Volatile Contents. Meteoritics and Planetary Science, 49 (S1). A104. ISSN 1086-9379. https://resolver.caltech.edu/CaltechAUTHORS:20141023-105133561

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Abstract

Much of our knowledge about the early Solar System comes from the study of CV3 meteorites, in particular Allende. Hydrothermal alteration is recognized as an important, ubiquitous process within these rocks (e.g. [1]). Nevertheless, we know little regarding the nature of these fluids. Volatile element abundances in phosphates from carbonaceous chondrites could constrain relative fugacities of H_2O, HF and HCl in the fluid present during metasomatism in primitive planetesimals.


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http://dx.doi.org/10.1111/maps.12359DOIAbstracts
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Additional Information:© 2014 The Meteoritical Society. Article first published online: 8 Sep. 2014.
Issue or Number:S1
Record Number:CaltechAUTHORS:20141023-105133561
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20141023-105133561
Official Citation:(2014), 77th Annual Meeting of the Meteoritical Society September 8–13, 2014. Meteoritics & Planetary Science, 49: A5–A454. doi: 10.1111/maps.12359
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:50733
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:23 Oct 2014 18:53
Last Modified:03 Oct 2019 07:26

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