A petrogenetic model for the origin and compositional variation of the martian basaltic meteorites
By L. Borg, D. Draper. 2003
227 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology
View Paper: https://www.semanticscholar.org/paper/586da8e7607bab91f5d85416737ad28cc019f26e
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In Astronomy and Astrophysics
- L. Elkins‐Tanton
- V. Hamilton
- A. Withers
- M. Hirschmann
- W. Koeppen
- E. Parmentier
- P. C. Hess
- T. O. S. University
In Ecology
- W. Koeppen
- L. Elkins‐Tanton
- E. Parmentier
- P. C. Hess
- V. Hamilton
- T. O. S. University
- Research School of Earth Sciences
- D. Geology
Citations in the corpus
- Ventilation of CO2 from a reduced mantle and consequences for the early Martian greenhouse (2008, background): “However, shergottites such as QUE 94201 and Y980459, which are isotopically depleted and, in the case of Y980459, petrologically primitive (Borg et al., 1997; Borg and Draper, 2003; McKay et al., 2004; Musselwhite et al., 2006), and therefore more likely to reflect mantle conditions, fall to the mor”
- Experimental petrology of the basaltic shergottite Yamato‐980459: Implications for the thermal structure of the Martian mantle (2006, background): “It could be an assimilated crustal component (e.g., Jones 2003), a separate mantle reservoir (e.g., Borg and Draper 2003), or a result of mantle metasomatism (Treiman 2003).”
- The composition of Mars (2019, background): “Petrological and geochemical data support the H chondrite like Mg# of the Martian mantle (Minitti et al., 2006; McCoy et al., 2016; Draper et al., 2005; White et al., 2006; Borg and Draper, 2003).”
- Possible formation of ancient crust on Mars through magma ocean processes (2005, methodology): “[34] The range of 176 Lu/ 177 Hf estimated to be appropriate for the SNC meteorite source regions (0.0276 to 0.0482) correlates well with the majority of the modeled Martian cumulate mantle (0.027 to 0.028), though not with the deeper source region that originally formed as majorite + ringwoodite in”
- Global distribution, composition, and abundance of olivine on the surface of Mars from thermal infrared data (2008, background): “ Borg and Draper [2003] have shown that the chemistry of the Martian shergottites can be modeled by melting a depleted component of the Martian mantle and adding trapped late stage liquid interacting with the cumulate stack, and perhaps this process formed the parent magmas of all the materials bea”
- Bulk composition and early differentiation of Mars (2007, background): “The geophysical data do, however, allow the value to be slightly lower (12–14 wt%), as suggested by high-pressure experiments on chondritic meteorites by Agee and Draper [2004] and supported by geochemical modeling [ Borg and Draper, 2003; Draper et al., 2005].”