The Liquidus Temperature for Methanol-Water Mixtures at High Pressure and Low Temperature, With Application to Titan

Author:

Dougherty A. J.1ORCID,Bartholet Z. T.1,Chumsky R. J.1,Delano K. C.12ORCID,Huang X.1,Morris D. K.13

Affiliation:

1. Department of Physics; Lafayette College; Easton, PA USA

2. Now at Department of Physics; University of Texas at San Antonio; San Antonio, TX USA

3. Division of Geological and Planetary Sciences; California Institute of Technology; Pasadena, CA USA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference53 articles.

1. Titan's obliquity as evidence of a subsurface ocean?;Baland;Astronomy & Astrophysics,2011

2. Analytic theory of Titan's Schumann resonance: Constraints on ionospheric conductivity and buried water ocean;Beghin;Icarus,2012

3. The second most abundant ice species towards the high-mass protostars RAFGL7009S and W 33A;Dartois;Astronomy & Astrophysics,1999

4. Cryolava flow destabilization of crustal methane clathrate hydrate on Titan;Davies;Icarus,2016

5. Atmospheric control of the cooling rate of impact melts and cryolavas on Titan's surface;Davies;Icarus,2010

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