Thermal modeling of shock melts in Martian meteorites: Implications for preserving Martian atmospheric signatures and crystallization of high-pressure minerals from shock melts-Reference-Cited by-同舟云学术

Thermal modeling of shock melts in Martian meteorites: Implications for preserving Martian atmospheric signatures and crystallization of high-pressure minerals from shock melts

Published:2013-03-28 Issue:5 Volume:48 Page:758-770
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Shaw Cliff S. J.¹,Walton Erin

Affiliation:

1. Department of Earth Sciences; University of New Brunswick; Fredericton; New Brunswick; E3B 5A3; Canada

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1111/maps.12100/fullpdf

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3. Time scales of shock processes in chondritic and Martian meteorites;Beck;Nature,2005

4. Shock-induced compaction, melting, and entrapment of atmospheric gases in Martian meteorites;Beck;Geophysical Research Letters,2007

5. Impact ages of meteorites: A synthesis;Bogard;Meteoritics,1995

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