The Liquidus of H2O-NH3 up to 1.5 GPa: Implications for the Presence of a Liquid Shell in Titan's Interior

Details The Liquidus of H2O-NH3 up to 1.5 GPa: Implications for the Presence of a Liquid Shell in Titan's Interior The Liquidus of H2O-NH3 up to 1.5 GPa: Implications for the Presence of a Liquid Shell in Titan's Interior

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27..453g&link_type=abstract

Lunar and Planetary Science, volume 27, page 453

Physics

1

Ammonia-Water Liquidus, Experiments: H.P.-Bt, History: Thermal, Ocean Crystallization, Titan

Scientific paper

Thermal evolution, internal structure and atmospheric composition of Titan depend strongly on the physical and chemical properties of the NH3-H2O-CH4 system. Sapphire anvil cell experiments have been conducted in the pressure range [100 MPa - 1.5 GPa] and in the temperature range [130 - 300 K] to investigate the ammonia (15%) - water system. A liquidus of the system is proposed and its implications for the internal structure of the satellite are discussed.

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