Ammonia, a Methane Hydrate Inhibitor - Implications for Titan's Atmospheric Methane

Details Ammonia, a Methane Hydrate Inhibitor - Implications for Titan's Atmospheric Methane Ammonia, a Methane Hydrate Inhibitor - Implications for Titan's Atmospheric Methane

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1640c&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1640

Physics

Scientific paper

As methane is dissociated in Titan's atmosphere, cryovolcanism is
required to explain its current abundance. This work provide
experimental constraints on methane hydrate stability in the system
H2O-CH4-NH3 for describing cryovolcanic processes.

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