Background levels of methane in Mars' atmosphere show strong seasonal variations
- PMID: 29880682
- DOI: 10.1126/science.aaq0131
Background levels of methane in Mars' atmosphere show strong seasonal variations
Abstract
Variable levels of methane in the martian atmosphere have eluded explanation partly because the measurements are not repeatable in time or location. We report in situ measurements at Gale crater made over a 5-year period by the Tunable Laser Spectrometer on the Curiosity rover. The background levels of methane have a mean value 0.41 ± 0.16 parts per billion by volume (ppbv) (95% confidence interval) and exhibit a strong, repeatable seasonal variation (0.24 to 0.65 ppbv). This variation is greater than that predicted from either ultraviolet degradation of impact-delivered organics on the surface or from the annual surface pressure cycle. The large seasonal variation in the background and occurrences of higher temporary spikes (~7 ppbv) are consistent with small localized sources of methane released from martian surface or subsurface reservoirs.
Copyright © 2018 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.
Comment in
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Organic molecules on Mars.Science. 2018 Jun 8;360(6393):1068-1069. doi: 10.1126/science.aat2662. Science. 2018. PMID: 29880670 No abstract available.
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Comments on the June 7, 2018, NASA News Release and Papers.Astrobiology. 2018 Jul;18(7):841-842. doi: 10.1089/ast.2018.1922. Epub 2018 Jul 16. Astrobiology. 2018. PMID: 30010389 Free PMC article. No abstract available.
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