Composition of northern low-albedo regions of Mars

Insights from the Mars Odyssey Gamma Ray Spectrometer

Suniti Karunatillake, Steven W. Squyres, G. Jeffrey Taylor, John M. Keller, Olivier Gasnault, Larry G. Evans, Robert C. Reedy, Richard D. Starr, William V. Boynton, Daniel M. Janes, Kristopher E. Kerry, James M. Dohm, Ann L. Sprague, Brian C. Hahn, Dave Hamara

Research output: Contribution to journalArticle

21 Citations (Scopus)

Abstract

Analysis of data acquired by the Mars Global Surveyor Thermal Emission Spectrometer (TES) instrument led to the identification of two distinct surface types. "Surface type 1," lying mostly within southern low-albedo terrain, is likely to be composed of basalt. However, there are several competing mineralogical models for "surface type 2," which is found primarily in northern low-albedo terrain. We attempt to identify which models better agree with element concentrations determined through the Gamma Subsystem (GS) of the Gamma Ray Spectrometer (GRS) instrument suite aboard the Mars Odyssey spacecraft. We have binned GS data over threshold regions derived from maps of surface types 1 and 2 and examined the spatial correlation of element concentrations with surface type 2. The elements we have examined are Cl, Fe, H, K, Si, and Th. Our results show that K concentration, Th concentration, and the areal abundance of surface type 2 are strongly correlated, with significant enrichment of both K and Th in regions representative of surface type 2. In addition, Si does not appear to be significantly enriched in surface type 2. These results are more consistent with surface type 2 originating from a compositionally distinct mantle source than the aqueous alteration of basalts.

Original languageEnglish (US)
Article numberE03S05
JournalJournal of Geophysical Research: Space Physics
Volume112
Issue number3
DOIs
StatePublished - Mar 20 2007

Fingerprint

Gamma ray spectrometers
gamma ray spectrometers
albedo
mars
Mars
spectrometer
Chemical analysis
basalt
Mars Global Surveyor
thermal emission
mantle source
Spacecraft
Spectrometers
spacecraft
Earth mantle
spectrometers

ASJC Scopus subject areas

  • Oceanography
  • Astronomy and Astrophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences (miscellaneous)
  • Geophysics
  • Geochemistry and Petrology

Cite this

Karunatillake, S., Squyres, S. W., Taylor, G. J., Keller, J. M., Gasnault, O., Evans, L. G., ... Hamara, D. (2007). Composition of northern low-albedo regions of Mars: Insights from the Mars Odyssey Gamma Ray Spectrometer. Journal of Geophysical Research: Space Physics, 112(3), [E03S05]. https://doi.org/10.1029/2006JE002675

Composition of northern low-albedo regions of Mars : Insights from the Mars Odyssey Gamma Ray Spectrometer. / Karunatillake, Suniti; Squyres, Steven W.; Taylor, G. Jeffrey; Keller, John M.; Gasnault, Olivier; Evans, Larry G.; Reedy, Robert C.; Starr, Richard D.; Boynton, William V.; Janes, Daniel M.; Kerry, Kristopher E.; Dohm, James M.; Sprague, Ann L.; Hahn, Brian C.; Hamara, Dave.

In: Journal of Geophysical Research: Space Physics, Vol. 112, No. 3, E03S05, 20.03.2007.

Research output: Contribution to journalArticle

Karunatillake, S, Squyres, SW, Taylor, GJ, Keller, JM, Gasnault, O, Evans, LG, Reedy, RC, Starr, RD, Boynton, WV, Janes, DM, Kerry, KE, Dohm, JM, Sprague, AL, Hahn, BC & Hamara, D 2007, 'Composition of northern low-albedo regions of Mars: Insights from the Mars Odyssey Gamma Ray Spectrometer', Journal of Geophysical Research: Space Physics, vol. 112, no. 3, E03S05. https://doi.org/10.1029/2006JE002675
Karunatillake, Suniti ; Squyres, Steven W. ; Taylor, G. Jeffrey ; Keller, John M. ; Gasnault, Olivier ; Evans, Larry G. ; Reedy, Robert C. ; Starr, Richard D. ; Boynton, William V. ; Janes, Daniel M. ; Kerry, Kristopher E. ; Dohm, James M. ; Sprague, Ann L. ; Hahn, Brian C. ; Hamara, Dave. / Composition of northern low-albedo regions of Mars : Insights from the Mars Odyssey Gamma Ray Spectrometer. In: Journal of Geophysical Research: Space Physics. 2007 ; Vol. 112, No. 3.
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