The age of the martian meteorite Northwest Africa 1195 and the differentiation history of the shergottites
By S. Symes, L. Borg, C. Shearer, A. Irving. 2007
146 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics
View Paper: https://www.semanticscholar.org/paper/3e0a05a932ebb9cc462c9aaf5f2cd2a150d95388
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In Astronomy and Astrophysics
- F. McCubbin
- 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
In Geophysics
- T. O. S. University
- Research School of Earth Sciences
- D. Geology
- T. Yoshizaki
- William F. McDonough Department of Earth Science
- Japan.
- College Park
- Usa
Citations in the corpus
- Heterogeneous distribution of H2O in the Martian interior: Implications for the abundance of H2O in depleted and enriched mantle sources (2016, background): “Geochemically, the shergottites form three distinct groups typically referred to as depleted, intermediate, and enriched (Borg et al. 1997, 2003; Herd et al. 2002; Borg and Draper 2003; Herd 2003; Symes et al. 2008; Wadhwa 2008; Shearer et al. 2013).”
- The composition of Mars (2019, background): “in the Martian mantle and crust. Incompatible element compositions (McLennan, 2003), radiogenic isotope systematics (e.g., initial 87Sr/86Sr and 143Nd/144Nd; Norman, 1999; Blichert-Toft et al., 1999; Symes et al., 2008) and redox state (Wadhwa, 2001; Hui et al., 2011) of shergottites indicate the pr”