A search for SO2, H2S and SO above Tharsis and Syrtis volcanic districts on Mars using ground-based high-resolution submillimeter spectroscopy
Icarus (New York, N.Y. 1962)
We surveyed the Tharsis and Syrtis volcanic regions on Mars during 23 November 2011 to 13 May 2012 which corresponded to its mid Northern Spring and early Northern Summer seasons (L s = 34-110°). Strong submillimeter rotational transitions of sulfur dioxide (SO 2 ), sulfur monoxide (SO) and hydrogen sulfide (H 2 S) were targeted. No active release was detected, and we infer 2r upper limits across the disk of the planet of 1.1 ppb, 0.7 ppb and 1.3 ppb for SO 2 ; SO and H 2 S, respectively. Our
... respectively. Our derived upper limit for SO 2 is comparable to previously reported limits, whereas for H 2 S we set a more stringent upper limit than previously measured, and we establish a limit for SO. Among the targeted molecules, SO 2 is the strongest indicator for volcanic outgassing. Assuming a photochemical lifetime of 2 years for SO 2 , our upper limit of 1.1 ppb implies an outgassing rate less than 55 metric tons/day. This rate limits the daily amount of degassing magma to less than 12,000 m 3 . Our sensitivity is sufficient to detect a volcanic release on Mars that is 4% the SO 2 released continuously from Kilauea volcano in Hawaii or 5% that of the Masaya volcano in Nicaragua. The non-detection of the sulfur compounds in the atmosphere of Mars indicates the absence of major volcanic outgassing. Published by Elsevier Inc. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).