The Abundance and Hydrogen Isotopic Composition of Water in SNC Meteorites: Implications for Water on Mars

The Abundance and Hydrogen Isotopic Composition of Water in SNC Meteorites: Implications for Water on Mars

<p>The water in the current martian atmosphere contains ~5 times more deuterium (D) than water on Earth (corresponding to a δD value of ~+4000) resulting from preferential loss of hydrogen relative to deuterium from the martian atmosphere. This thesis places constraints on the D/H of other mar...

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Bibliographic Details
Main Author: Leshin, Laurie Ann
Format: Others
Language:en
Published: 1995
Online Access:https://thesis.library.caltech.edu/4424/1/Leshin_la_1995.pdf
Leshin, Laurie Ann (1995) The Abundance and Hydrogen Isotopic Composition of Water in SNC Meteorites: Implications for Water on Mars. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/36AJ-NW91. https://resolver.caltech.edu/CaltechETD:etd-11062007-091745 <https://resolver.caltech.edu/CaltechETD:etd-11062007-091745>

Internet

https://thesis.library.caltech.edu/4424/1/Leshin_la_1995.pdf
Leshin, Laurie Ann (1995) The Abundance and Hydrogen Isotopic Composition of Water in SNC Meteorites: Implications for Water on Mars. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/36AJ-NW91. https://resolver.caltech.edu/CaltechETD:etd-11062007-091745 <https://resolver.caltech.edu/CaltechETD:etd-11062007-091745>

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