NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Phosphates at the Surface of Mars: Primary Deposits and Alteration ProductsPhosphorus is an essential element in terrestrial organisms and thus characterizing the occurrences of phosphate phases at the martian surface is crucial in the assessment of habitability. The Alpha Particle X-Ray Spectrometers onboard Spirit, Opportunity and Curiosity discovered a variety of primary and secondary phosphate phases allowing direct comparisons across the three landing sites. The Spirit rover at Gusev Crater encountered the "Wishstone/Watchtower" class of P-rich (up to 5.2 wt% P2O5) rocks interpreted to be alkaline volcanic rocks with a physical admixture of approximately 10 to 20% merrillite [Usui et al 2008]. These rocks are characterized by elevated Ti and Y and anomalously low Cr and Ni, which could largely reflect the nature of the protoliths: Evolved magmatic rocks. Many of these chemical signatures are also found in pyroclastic deposits at nearby "Home Plate" and in phosphate precipitates derived from fluid interactions with these rocks ("Paso Robles" soils). The Opportunity rover at Meridiani Planum recently analyzed approximately 4 cm clast in a fine-grained matrix, one of numerous rocks of similar appearance at the rim of Endeavour Crater. This clast, "Sarcobatus," has minor enrichments in Ca and P relative to the matrix, and like the P-rich rocks at Gusev, Sarcobatus also shows elevated Al and Ti. On the same segment of the Endeavour rim, subsurface samples were found with exceptional levels of Mn (approximately 3.5 wt% MnO). These secondary and likely aqueous deposits contain strong evidence for associated Mg-sulfate and Ca-phosphate phases. Finally, the Curiosity traverse at Gale crater encountered P-rich rocks compositionally comparable to Wishstone at Gusev, including elevated Y. Phosphorous-rich rocks with similar chemical characteristics are prevalent on Mars, and the trace and minor element signatures provide constraints on whether these are primary deposits, secondary products of physical weathering or secondary products of chemical weathering.
Document ID
20140012978
Document Type
Conference Paper
Authors
Yen, Albert S. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Gellert, Ralf (Guelph Univ. Ontario, Canada)
Clark, Benton C. (Space Science Inst. Boulder, CO, United States)
Ming, Douglas W. (NASA Johnson Space Center Houston, TX, United States)
Mittlefehldt, David W. (NASA Johnson Space Center Houston, TX, United States)
Arvidson, Raymond E. (Washington Univ. Saint Louis, MO, United States)
McSween, Harry Y., Jr. (Tennessee Univ. Knoxville, TN, United States)
Schroder, Christian (Stirling Univ. United Kingdom)
Date Acquired
October 15, 2014
Publication Date
December 13, 2014
Subject Category
Lunar and Planetary Science and Exploration
Report/Patent Number
JSC-CN-32076
Meeting Information
American Geophysical Union (AGU) Fall Meeting(San Francisco, CA)
Distribution Limits
Public
Copyright
Public Use Permitted.

Available Downloads

NameType 20140012978.pdf STI