Searching for the source regions of martian meteorites using MGS TES: Integrating martian meteorites into the global distribution of igneous materials on Mars
By V. Hamilton, Philip R. Christensen, H. McSween, J. Bandfield. 2003
169 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology
View Paper: https://www.semanticscholar.org/paper/bd9b2308f4d9aca73e04587e545532f9a4a29048
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- Michael D. Smith
- V. Hamilton
- Philip R. Christensen
- H. McSween
- J. Bandfield
- Michael J. Wolff
- W. Koeppen
- R. Clancy
In Ecology
- V. Hamilton
- H. McSween
- J. Bandfield
- Michael D. Smith
- W. Koeppen
- Philip R. Christensen
- T. Grove
- M. Wyatt
Citations in the corpus
- Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on Mars Reconnaissance Orbiter (MRO) (2007, background): “Some outcrops of ancient crust exhibit high concentrations of olivine [Hoefen et al., 2003] and lowcalcium pyroxene (LCP) in thermal emission data [Hamilton et al., 2003].”
- Global distribution, composition, and abundance of olivine on the surface of Mars from thermal infrared data (2008, methodology): “This anomaly is difficult to detect automatically, and it can result in erroneous mineral detections in full-spectrum mixture modeling of the data [ Hamilton et al., 2003 ].”
- Identification of quartzofeldspathic materials on Mars (2004, methodology): “[19] The deconvolution surface-atmosphere separation also provides areal mineral and spectral unit abundances that can be used for compositional analysis [Smith et al., 2000; Bandfield et al., 2000a; Bandfield, 2002; Hamilton et al., 2003].”
- Constraints on the composition and petrogenesis of the Martian crust (2003, methodology): “…of hematite [e.g., Christensen et al., 2000b], orthopyroxene [e.g., Hamilton et al., 2003; Bandfield, 2002], and olivine [e.g., Clark et al., 1982; Hamilton et al., 2003; Bandfield, 2002] have also been identified in regional and local occurrences where surface type 1 compositions dominate…”
- Thermal infrared (vibrational) spectroscopy of Mg–Fe olivines: A review and applications to determining the composition of planetary surfaces (2010, methodology): “Chassigny is a dunite comprised of 490 vol% olivine with r5 vol% each pyroxene and feldspar.”