Hydrous melting of the martian mantle produced both depleted and enriched shergottites
By F. McCubbin, E. Hauri, S. Elardo, K. V. Kaaden, Jianhua Wang, C. Shearer. 2012
243 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/5c4ecbaf39b4735cef4067b2571a61b974c09e5f
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In Astronomy and Astrophysics
- A. Morbidelli
- Michiel Lambrechts
- Anders Johansen
- B. Bitsch
- Seth Andrew Jacobson
- A. Crida
- S. Raymond
- Elena Lega
In Atmospheric Science
- A. Crida
- B. Bitsch
- Michiel Lambrechts
- A. Morbidelli
- Seth Andrew Jacobson
- H. McSween
- William Bottke
- D. Nesvorný
Citations in the corpus
- The origin of water in the primitive Moon as revealed by the lunar highlands samples (2014, methodology): “Three terrestrial apatite standards (Ap003, Ap004, and Ap018 described in McCubbin et al., 2012) pressed in indium were used for calibration along with a “dry” San Carlos olivine crystal.”
- Heterogeneous distribution of H2O in the Martian interior: Implications for the abundance of H2O in depleted and enriched mantle sources (2016, methodology): “…Martian meteorites (McSween and Harvey 1993; Swindle et al. 2000; Bridges et al. 2001; Dann et al. 2001; McSween et al. 2001; Borg and Drake 2005; McCubbin et al. 2009, 2010a, 2012; Bridges and Schwenzer 2012; Filiberto and Schwenzer 2013; Muttik et al. 2014), models of impact-induced…”
- A hydrogen-based oxidation mechanism relevant to planetary formation (2013, background): “Mars, which has on the order of 10’s–100’s ppm H2O in its mantle (McCubbin et al., 2012; Usui et al., 2012), has lithologies ranging from as reduced as IW to about as oxidized as FMQ+1.”
- Petrology on Mars (2015, background): “Although the shergottites are nearly anhydrous, several lines of evidence suggest that their parent magmas were hydrous and lost water during ascent or eruption (e.g., McSween et al. 2001; McCubbin et al. 2012).”
- Fossilized condensation lines in the Solar System protoplanetary disk (2015, background): “ a signicant accretion of oxidized material would have led to an Earth with dierent chemical properties (Rubie et al., 2015). Mars is also a water-poor planet, with only 70{300ppm of water by mass (McCubbin et al., 2012). Thus, it seems that the water and, more generally, the volatile budget of Sola”