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Water in Terrestrial Planets: Always an Oxidant?Water is commonly assumed to be an oxidant in many planetary settings. Because it can affect Fe-FeO-Fe2O3 equilibria and thus bulk compositional properties of planets and asteroids, this is an important ingredient to understand. The role of water in two settings will be addressed - magmas, and mantles during accretion - along with the implications for planet growth and evolution.
Document ID
20040056067
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Righter, K. (NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2004
Publication Information
Publication: Lunar and Planetary Science XXXV: Special Session: Oxygen in the Solar System, II
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-20613
Distribution Limits
Public
Copyright
Public Use Permitted.
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IDRelationTitle20040056060Collected WorksLunar and Planetary Science XXXV: Special Session: Oxygen in the Solar System, II
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