Highly siderophile element (HSE) abundances in the mantle of Mars are due to core formation at high pressure and temperature

Author:

Righter K.1,Danielson L. R.2,Pando K. M.2,Williams J.3,Humayun M.3,Hervig R. L.4,Sharp T. G.4

Affiliation:

1. Mailcode KT; NASA Johnson Space Center; 2101 NASA Parkway Houston Texas 77058 USA

2. Jacobs Technology; JETS; NASA Johnson Space Center; 2101 NASA Parkway Houston Texas 77058 USA

3. National High Magnetic Field Laboratory and Department of Earth, Ocean and Atmospheric Science; Florida State University; Tallahassee Florida 32310-3706 USA

4. ASU School of Earth and Space Exploration; PO Box 871404 Tempe Arizona 5287-1404 USA

Funder

National Aeronautics and Space Administration

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference166 articles.

1. Unique meteorite from Early Amazonian Mars: Water-rich basaltic breccia Northwest Africa 7034;Agee;Science,2013

2. Anand M. James S. Greenwood R. C. Johnson D. Franchi I. A. Grady M. M. 2008 Mineralogy and geochemistry of shergottite RBT 04262 (abstract #2173)

3. The significance of multiple saturation points in the context of polybaric near-fractional melting;Asimow;Journal of Petrology,2004

4. The origin of the fractionation of platinum group elements in terrestrial magmas;Barnes;Chemical Geology,1985

5. Geochemistry of the Martian meteorite ALH 84001, revisited;Barrat;Meteoritics & Planetary Science,2010

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