Global distribution, composition, and abundance of olivine on the surface of Mars from thermal infrared data

By W. Koeppen, V. Hamilton. 2008

195 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/d0b9b8691f436c9a251c09e457ccf18ce40a96af

How researchers see this paper

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

In Aerospace Engineering

1. J. Bibring
2. Bethany L. Ehlmann
3. E. Kite
4. Christopher S. Edwards
5. Yves Langevin
6. B. Gondet
7. J. Carter
8. V. Hamilton

In Astronomy and Astrophysics

1. Bethany L. Ehlmann
2. E. Kite
3. Christopher S. Edwards
4. J. Bibring
5. Yves Langevin
6. B. Gondet
7. J. Carter
8. V. Hamilton

Citations in the corpus

• Geologic Constraints on Early Mars Climate (2018, background): “Despite this fragility, olivine is widespread in Mars rocks and soil (Hamilton and Christensen 2005; Koeppen and Hamilton 2008; McGlynn et al. 2012; Ody et al. 2013).”
• Mineralogy of the Martian Surface (2014, background): “Argyre Hellas Isidis Tharsis Acidalia Terra Sirenum Arabia Terra Terra Meridiani Utopia Elysium Valles Marineris –135 13590450– 45–90 180–180 Longitude (˚E) La ti tu de (˚ N ) 45 – 45 0 – 90 90 0% 20%TES olivine abundance Low HighOMEGA total olivine a b c 20 km20 km A nn u.”
• Global investigation of olivine on Mars: Insights into crust and mantle compositions (2013, methodology): “[34] Olivine on the surface of Mars was also inferred from TES data [McSween et al., 2006; Koeppen and Hamilton, 2008].”
• Thermal infrared (vibrational) spectroscopy of Mg–Fe olivines: A review and applications to determining the composition of planetary surfaces (2010, methodology): “After Koeppen and Hamilton (2008). from Fo53–39, considerably more Fe-rich than observed in most Martian meteorites.”