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. http://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.
| Item Type: | Article | |||||||||
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| Additional Information: | © 2014 The Meteoritical Society. Article first published online: 8 Sep. 2014. | |||||||||
| Record Number: | CaltechAUTHORS:20141023-105133561 | |||||||||
| Persistent URL: | http://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: | 23 Oct 2014 18:53 |
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