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Mars Methane Detection and Variability at Gale Crater

journal contribution
posted on 2015-02-02, 10:29 authored by CR Webster, P Mahaffy, SK Atreya, GJ Flesch, MA Mischna, P-Y Meslin, KA Farley, PG Conrad, LE Christensen, AA Pavlov, J Martin-Torres, M-P Zorzano, TH McConnochie, T Owen, JE Eigenbrode, DP Glavin, A Steele, A Malespin, DP Archer, B Sutter, P Coll, P Freissinet, CP McKay, JE Moores, SP Schwenzer, John C. Bridges, R Navarro-Gonzalez, R Gellert, MT Lemmon
Reports of plumes or patches of methane in the Martian atmosphere that vary over monthly timescales have defied explanation to date. From in situ measurements made over a 20-month period by the Tunable Laser Spectrometer (TLS) of the Sample Analysis at Mars (SAM) instrument suite on Curiosity at Gale Crater, we report detection of background levels of atmospheric methane of mean value 0.69 ±0.21 ppbv at the 95% confidence interval (CI). This abundance is lower than model estimates of ultraviolet (UV) degradation of accreted interplanetary dust particles (IDP’s) or carbonaceous chondrite material. Additionally, in four sequential measurements spanning a 60-sol period, we observed elevated levels of methane of 7.19 ±1.99 (95% CI) ppbv implying that Mars is episodically producing methane from an additional unknown source.

Funding

UK Space Agency

History

Citation

Science, 2015, 347, pp. 415-417 (2)

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • AM (Accepted Manuscript)

Published in

Science

Publisher

AGU

issn

0036-8075

eissn

1095-9203

Available date

2015-02-02

Publisher version

http://www.sciencemag.org/content/347/6220/415

Notes

Supplementary materials http://www.sciencemag.org/content/347/6220/415/suppl/DC1

Language

en

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