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The solubility of 40 Ar and 84 Kr in liquid hydrocarbons: Implications for Titan's geological evolution
Author(s) -
Hodyss Robert,
Choukroun Mathieu,
Sotin Christophe,
Beauchamp Patricia
Publication year - 2013
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/grl.50630
Subject(s) - titan (rocket family) , methane , outgassing , krypton , atmosphere of titan , argon , solubility , astrobiology , chemistry , physics , organic chemistry
The solubility of argon and krypton in methane and ethane has been experimentally determined at Titan‐relevant temperatures. At typical Titan surface temperature (94 K), argon and krypton solubilities are very large (47% in methane and 15% in ethane for Ar, 29% in methane and 43% in ethane for Kr), making liquid alkanes on Titan an important potential reservoir of 40 Ar and other noble gases. Large subsurface reservoirs of liquid ethane and methane could be sufficient to trap much of the argon outgassing from Titan's interior, which can help explain the discrepancy between the potential amount of 40 Ar produced inside Titan's interior and the amount observed in the atmosphere by Cassini‐Huygens. Consequently, on Titan, liquid hydrocarbons may function as a buffer in the outgassing of volatiles from the interior, and they may strongly influence the evolution of the atmosphere's composition through the release of soluble gases upon evaporation and/or intake upon condensation.