Mineralogical constraints on the high-silica martian surface component observed by TES

By J. Michalski, M. Kraft, T. Sharp, L. Williams, Philip R. Christensen. 2005

139 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/3f99adbb661e2890e7a4894a6c4c75c7d38e5a1c

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In Artificial Intelligence

1. V. Hamilton
2. H. McSween
3. Janice L. Bishop
4. W. Koeppen
5. Melinda Darby Dyar
6. Adrian. J. Brown
7. M. Lane

In Astronomy and Astrophysics

1. V. Hamilton
2. H. McSween
3. J. Bibring
4. W. Koeppen
5. Yves Langevin
6. J. F. Mustard
7. B. Gondet
8. François Poulet

In Geophysics

1. V. Hamilton
2. H. McSween
3. W. Koeppen
4. Janice L. Bishop
5. Melinda Darby Dyar
6. Adrian. J. Brown
7. J. F. Mustard
8. M. Lane

Citations in the corpus

• Martian surface mineralogy from Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité on board the Mars Express spacecraft (OMEGA/MEx): Global mineral maps (2007, background): “6.3. Northern Low-Albedo Regions [44] Several hypotheses have been presented to explain the apparent andesitic character of the Acidalia-type spectrum: weathering of basalt to produce clay minerals [Wyatt and McSween, 2002], silica coating basalt [Kraft et al., 2003], water-bearing minerals such as ”
• Global distribution, composition, and abundance of olivine on the surface of Mars from thermal infrared data (2008, methodology): “... analyses included spectra of pure minerals and glasses, one nearly monomineralic Martian meteorite, atmospheric components, and a blackbody spectrum (unit emissivity at all wave numbers) (Table 4). The mineral spectral endmembers in our set were measured in laboratory conditions [Christensen et ”
• Petrology on Mars (2015, background): “Earlier reports of widespread andesites, based on TES thermal emission spectra, are now reinterpreted as partly altered basalt (e.g., Michalski et al. 2005).”
• Reflectance and emission spectroscopy study of four groups of phyllosilicates: smectites, kaolinite-serpentines, chlorites and micas (2008, background): “The bending vibrations for tetrahedral SiO4 groups occur near 18 25 mm (400 550 cm 1) in reflectance and emissivity spectra when little or no tetrahedral substitution occurs (Salisbury et al., 1991; Michalski et al., 2005).”