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Why should Titan’s ocean be organic rich? What thermodynamic modeling of the dewatering of undifferentiated versus differentiated moons can tell us
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| dc.contributor.author | Daswani, Mohit Melwani | |
| dc.contributor.author | Vance, Steven | |
| dc.date.accessioned | 2021-02-19T00:55:38Z | |
| dc.date.available | 2021-02-19T00:55:38Z | |
| dc.date.issued | 2019-06-24 | |
| dc.identifier.citation | 2019 Astrobiology Science Conference (AbSciCon 2019), Bellevue, Washington, June 24-28, 2019 | en_US |
| dc.identifier.clearanceno | 19-3562 | |
| dc.identifier.uri | http://hdl.handle.net/2014/51010 | |
| dc.description.sponsorship | NASA/JPL | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2019 | en_US |
| dc.title | Why should Titan’s ocean be organic rich? What thermodynamic modeling of the dewatering of undifferentiated versus differentiated moons can tell us | en_US |
| dc.type | Presentation | en_US |
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JPL TRS 1992+
JPL TRS 1992+