Origin of water and mantle–crust interactions on Mars inferred from hydrogen isotopes and volatile element abundances of olivine-hosted melt inclusions of primitive shergottites
Authors:
- Tomohiro UsuiTUTomohiro Usui
- Conel M.O'D. AlexanderCAConel M.O'D. Alexander
- Jianhua WangJWJianhua Wang
- Justin I. SimonJSJustin I. Simon
- John H. JonesJJJohn H. Jones
- 1 December 2012
- journal article
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 357-358, 119-129
Abstract
No abstract availableFunding Information
- National Aeronautics and Space Administration
- NASA Astrobiology Institute
This publication has 62 references indexed in Scilit:
- The Provenances of Asteroids, and Their Contributions to the Volatile Inventories of the Terrestrial PlanetsScience, 2012
- Fe2+–Mg partitioning between olivine and basaltic melts: Applications to genesis of olivine-phyric shergottites and conditions of melting in the Martian interiorEarth and Planetary Science Letters, 2011
- Volatile accretion history of the terrestrial planets and dynamic implicationsNature, 2009
- Dehydration melting of nominally anhydrous mantle: The primacy of partitioningPhysics of the Earth and Planetary Interiors, 2009
- Pyroclastic Activity at Home Plate in Gusev Crater, MarsScience, 2007
- Experimental petrology of the basaltic shergottite Yamato-980459: Implications for the thermal structure of the Martian mantleMeteoritics & Planetary Science, 2006
- SIMS analysis of volatiles in silicate glassesChemical Geology, 2002
- Insights into Martian water reservoirs from analyses of Martian meteorite QUE94201Geophysical Research Letters, 2000
- The xenon isotopic composition of the primordial Martian atmosphere: Contributions from solar and fission componentsJournal of Geophysical Research, 1997
- Deuterium on Mars: The Abundance of HDO and the Value of D/HScience, 1988