The bulk composition of Mars
By Jeffrey Taylor. 2013
288 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology
View Paper: https://www.semanticscholar.org/paper/d0bcdf72005a8e77781c5b05a2d4c4663ff2e62e
How researchers see this paper
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In Astronomy and Astrophysics
- Mark A. Wieczorek
- A. Morbidelli
- F. Nimmo
- D. O'Brien
- Seth Andrew Jacobson
- C. Shearer
- F. McCubbin
- D. Rubie
In Ecology
- T. O. S. University
- Research School of Earth Sciences
- D. Geology
- Alison R. Santos
- T. Yoshizaki
- William F. McDonough Department of Earth Science
- P. Srinivasan
- Andrew Steele
Citations in the corpus
- Accretion and differentiation of the terrestrial planets with implications for the compositions of early-formed Solar System bodies and accretion of water (2014, background): “…the chemistry of the silicate mantles of the Earth and, to a lesser extent, Mars, Venus and Mercury (e.g. McDonough, 2003; Palme and O’Neill, 2013; Dreibus and Wänke, 1985; McSween, 2003; Taylor, 2013; Righter and Chabot, 2011; Treiman 2009; Robinson and Taylor, 2001; Taylor and Scott, 2003).”
- Heterogeneous distribution of H2O in the Martian interior: Implications for the abundance of H2O in depleted and enriched mantle sources (2016, methodology): “Based on the estimated concentrations of incompatible lithophile element abundances in the Martian crust (e.g., K, Th, U, and REE), the Martian crust hosts ~50% of the total inventory of incompatible lithophiles (McLennan 2001, 2003; Taylor et al. 2010; Taylor 2013).”
- What Martian Meteorites Reveal About the Interior and Surface of Mars (2020, methodology): “The martian volatile budget indicates that Mars likely accreted from inner 469 solar system material (Taylor, 2013).”
- The seismicity of Mars (2020, methodology): “For the mantle, we consider 5 different compositions (Lodders & Fegley, 1997; Mohapatra & Murty, 2003; Sanloup et al., 1999; Taylor, 2013; Brasser et al., 2018) deduced from the analysis of Martian meteorites.”
- The composition of Mars (2019, methodology): “1 Manganese, chromium and vanadium The MnO concentration in the BSM (Wänke and Dreibus, 1994; Taylor, 2013) is established foremost from the nearly constant FeO/MnO ratio in Martian meteorites (shergottite average 39.”