Published September 2014
| Version Published
Journal Article
Open
Characterizing Early Solar System Fluids on the Allende (CV3) Parent Body: Nanosims Study of Phosphate Volatile Contents
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.
Additional Information
© 2014 The Meteoritical Society. Article first published online: 8 Sep. 2014.Attached Files
Published - 5386.pdf
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5386.pdf
Additional details
Identifiers
- Eprint ID
- 50733
- DOI
- 10.1111/maps.12359
- Resolver ID
- CaltechAUTHORS:20141023-105133561
Related works
- Describes
- 10.1111/maps.12359 (DOI)
Dates
- Created
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2014-10-23Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)