Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1773546 | Icarus | 2013 | 4 Pages |
Abstract
We have searched for the presence of simple P and S-bearing molecules in Titan’s atmosphere, by looking for the characteristic signatures of phosphine and hydrogen sulfide in infrared spectra obtained by Cassini CIRS. As a result we have placed the first upper limits on the stratospheric abundances, which are 1 ppb (PH3) and 330 ppb (H2S), at the 2-σ significance level.
► We have searched in Cassini CIRS infrared spectra for signatures of PH3 and H2S. ► We find no evidence for either gas in the stratosphere at 0.3 mbar. ► 2-σ upper limits on abundance are 1 ppb (PH3) and 330 ppb (H2S). ► These gases may still be present at lower levels, released from clathrate hydrates.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Conor A. Nixon, Nicholas A. Teanby, Patrick G.J. Irwin, Sarah M. Hörst,