Effects of H<sub>2</sub>O, pH, and oxidation state on the stability of Fe minerals on Mars
P. L. King(Australian National University), H. Y. McSween(University of Tennessee at Knoxville)
Cited by 174
Related Papers
The Thermal Emission Imaging System (THEMIS) for the Mars 2001 Odyssey Mission
|Space Science Reviews|2004|927
Overview of the Spirit Mars Exploration Rover Mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills
|Journal of Geophysical Research Atmospheres|2006|708
What we have learned about Mars from SNC meteorites
|Meteoritics|1994|620