A Dual Origin for the Deuterium Enrichment in the Atmosphere of Titan

Details A Dual Origin for the Deuterium Enrichment in the Atmosphere of Titan A Dual Origin for the Deuterium Enrichment in the Atmosphere of Titan

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1691c&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

The recent determination of D/H derived from Cassini/CIRS spectra
indicates values of the order on 1.32 + 0.15-0.11 ×
10-4. The D/H enhancement would then result from consequent
isotopic fractionation; we reinvestigate this scenario.

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