Improving on Titan's stratospheric trace gaseous composition of and searching for new molecules using CIRS spectra

Details Improving on Titan's stratospheric trace gaseous composition of and searching for new molecules using CIRS spectra Improving on Titan's stratospheric trace gaseous composition of and searching for new molecules using CIRS spectra

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1440b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1440

Physics

Scientific paper

Titan is one of the most interesting objects in the Solar System considering its large size and its dense nitrogenous atmosphere rich in organics. Indeed, the Cassini-Huygens mission has reported many Earthlike characteristics of Saturn largest moon verifying the Voyager 1 results 30 years ago. In this work, focusing on Titan's stratosphere, we will report the mixing ratios of traces gases in respect to previous studies and we will search for new molecules.

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