Effects of H2O, pH, and oxidation state on the stability of Fe minerals on Mars

By P. King, H. McSween. 2005

161 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geochemistry and Petrology, Paleontology

View Paper: https://www.semanticscholar.org/paper/dbe1a0c3f366b0525b3d6d44bc76bbf8e2683f2e

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Ralph E. Milliken
2. Bethany L. Ehlmann
3. J. Bibring
4. J. F. Mustard
5. F. Gaillard
6. Bruno Scaillet
7. R. Arvidson
8. Janice L. Bishop

In Paleontology

1. F. Gaillard
2. Bruno Scaillet
3. Ralph E. Milliken
4. Bethany L. Ehlmann

Citations in the corpus

• The sulfur content of volcanic gases on Mars (2009, background): “…that nearly all atmospheric sulfur would ultimately fall back on the ground, this would yield a 60 m thick layer of sulfates if uniformly distributed over Mars surface (for simplicity, we considered here only anhydrite but clearly other sulfate phases would be present; King et al., 2004).”
• A synthesis of Martian aqueous mineralogy after 1 Mars year of observations from the Mars Reconnaissance Orbiter (2009, background): “SO 4 -Cl solutions will precipitate Fe sulfates with low OH/(OH + SO 4 ) levels such as copiapite and bilinite, Fe (hydr)oxides, Fe phosphates, Ca-Mg-Na sulfates, Si-rich phases, and possibly Mg-Na + K-Ca halides [King and McSween, 2005].”