The DOI matches its Crossref record; 76 of the 76 references it cites were found in a registry or an index.
Concentration of H, Si, Cl, K, Fe, and Th in the low‐ and mid‐latitude regions of Mars
Abstract
We report maps of the concentrations of H, Si, Cl, K, Fe, and Th as determined by the Gamma Ray Spectrometer (GRS) on board the 2001 Mars Odyssey Mission for ±∼45° latitudes. The procedures by which the spectra are processed to yield quantitative concentrations are described in detail. The concentrations of elements determined over the locations of the various Mars landers generally agree well with the lander values except for Fe, although the mean of the GRS Fe data agrees well with that of Martian meteorites. The water‐equivalent concentration of hydrogen by mass varies from about 1.5% to 7.5% (by mass) with the most enriched areas being near Apollinaris Patera and Arabia Terra. Cl shows a distribution similar to H over the surface except that the Cl content over Medusae Fossae is much greater than elsewhere. The map of Fe shows enrichment in the northern lowlands versus the southern highlands. Silicon shows only very modest variation over the surface with mass fractions ranging from 19% to 22% over most of the planet, though a significant depletion in Si is noted in a region west of Tharsis Montes and Olympus Mons where the Si content is as low as 18%. K and Th show a very similar pattern with depletions associated with young volcanic deposits and enrichments associated with the TES Surface Type‐2 material. It is noted that there appears to be no evidence of significant globally distributed thick dust deposits of uniform composition.
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Cites
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Sulfates in Martian Layered Terrains: The OMEGA/Mars Express View
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Mars Surface Diversity as Revealed by the OMEGA/Mars Express Observations
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In Situ Evidence for an Ancient Aqueous Environment at Meridiani Planum, Mars
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Self-citationDistribution of Hydrogen in the Near Surface of Mars: Evidence for Subsurface Ice Deposits
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Self-citationJarosite and Hematite at Meridiani Planum from Opportunity's Mössbauer Spectrometer
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Self-citationAncient oceans, ice sheets and the hydrological cycle on Mars
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“Subsequent hydrologic activity resulted in a transferal of weathered products from the cratered highlands to the lowlands, including via Tharsis- (and to a lesser extent Elysium-) induced flooding and deep dissection of the Martian crust to form outflow channels [e.g., Baker et al., 1991; Dohm et al., 2001a, 2001b; Fa…”
BackgroundSelf-citationRemote geochemical analysis: elemental and mineralogical composition
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A Global View of Martian Surface Compositions from MGS-TES
Bandfield, J. L., Hamilton, V. E., & Christensen, P. R. (2000) · Science · doi:10.1126/science.287.5458.1626 · Cited by 675
Water and the martian landscape
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Elemental composition of the martian crust
McSween, H. Y., Taylor, G. J., & Wyatt, M. B. (2009) · Science · doi:10.1126/science.1165871 · Cited by 506
Self-citationGeologic context of proposed chloride‐bearing materials on Mars
Osterloo, M. M., Anderson, F. S., Hamilton, V. E., & Hynek, B. M. (2010) · Journal of Geophysical Research: Planets · doi:10.1029/2010je003613 · Cited by 274
Soil Diversity and Hydration as Observed by ChemCam at Gale Crater, Mars
Meslin, P.-Y., Gasnault, O., Forni, O., Schröder, S., Cousin, A., Berger, G., Clegg, S. M., Lasue, J., Maurice, S., Sautter, V., et al. (2013) · Science · doi:10.1126/science.1238670 · Cited by 268
Self-citationSustainable life support on Mars – the potential roles of cyanobacteria
Verseux, C., Baqué, M., Lehto, K., de Vera, J.-P. P., Rothschild, L. J., & Billi, D. (2016) · International Journal of Astrobiology · doi:10.1017/s147355041500021x · Cited by 194
Evidence for the Distribution of Perchlorates on Mars
Clark, B. C., & Kounaves, S. P. (2016) · International Journal of Astrobiology · doi:10.1017/s1473550415000385 · Cited by 121
Metadata
- Authors
- Boynton, W. V., Taylor, G. J., Evans, L. G., Reedy, R. C., Starr, R., Janes, D. M., Kerry, K. E., Drake, D. M., Kim, K. J., Williams, R. M. S., Crombie, M. K., Dohm, J. M., Baker, V., Metzger, A. E., Karunatillake, S., Keller, J. M., Newsom, H. E., Arnold, J. R., Brückner, J., Englert, P. A. J., Gasnault, O., Sprague, A. L., Mitrofanov, I., Squyres, S. W., Trombka, J. I., d'Uston, L., Wänke, H., & Hamara, D. K.
- Venue
- Journal of Geophysical Research: Planets
- Publisher
- American Geophysical Union (AGU)
- Published
- 2007-12
- Volume
- 112
- Issue
- E12
- ISSN
- 0148-0227 (ISSN-L)
- OpenAlex
- W2034754132
- Cited by
- 351
- References
- 76
- FWCI
- 8.66
- Type
- journal article
- Language
- en
- Open access
- closed
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- The paper
- Boynton, W. V., Taylor, G. J., Evans, L. G., Reedy, R. C., Starr, R., Janes, D. M., Kerry, K. E., Drake, D. M., Kim, K. J., Williams, R. M. S., Crombie, M. K., Dohm, J. M., Baker, V., Metzger, A. E., Karunatillake, S., Keller, J. M., Newsom, H. E., Arnold, J. R., Brückner, J., . . . Hamara, D. K. (2007). Concentration of H, Si, Cl, K, Fe, and Th in the low‐ and mid‐latitude regions of Mars. Journal of Geophysical Research: Planets. https://doi.org/10.1029/2007je002887
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.