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Mauna Loa volcano is not a methane source: Implications for Mars
Author(s) -
Ryan Steven,
Dlugokencky Edward J.,
Tans Pieter P.,
Trudeau Michael E.
Publication year - 2006
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2006gl026223
Subject(s) - volcano , mars exploration program , lava , martian , methane , tharsis , astrobiology , atmosphere of mars , geology , earth science , atmosphere (unit) , volcanic gases , atmospheric sciences , environmental science , geochemistry , meteorology , chemistry , physics , organic chemistry
Thirteen years of continuous atmospheric carbon dioxide and methane measurements at the Mauna Loa Observatory in Hawaii are used to determine the methane emission rate from the summit of Mauna Loa volcano. We find no measurable methane emissions coming from the summit area, with a 95% confidence upper limit of 9 t CH 4 yr −1 . Recent studies have detected 10 ppb CH 4 in the Martian atmosphere, requiring emissions of about 300 t CH 4 yr −1 . Volcanic activity has been suggested as a source of abiogenic CH 4 on Mars, either by magmatic degassing or reactions in hydrothermal fluids heated by a magma intrusion. The most recent lava flows on Mars (2 My ago) are on the Tharsis shield volcanoes, which may still be active. If Mauna Loa is a valid terrestrial analog, our findings suggest that volcanic activity is not a significant source of methane to the Martian atmosphere.