JavaScript is disabled for your browser. Some features of this site may not work without it.
| dc.contributor.author | Smrekar, Suzanne E. | |
| dc.contributor.author | Andrews-Hanna, Jeffrey C. | |
| dc.contributor.author | Breuer, Doris | |
| dc.contributor.author | Byrne, Paul | |
| dc.contributor.author | Buczkowski, Debra L. | |
| dc.contributor.author | Campbell, Bruce A. | |
| dc.contributor.author | Davaille, A. | |
| dc.contributor.author | Dyar, M. Darby (Melinda Darby) | |
| dc.contributor.author | Di Achille, G. | |
| dc.contributor.author | Fassett, Caleb | |
| dc.contributor.author | Gilmore, Martha S. | |
| dc.contributor.author | Grimm, Robert E. | |
| dc.contributor.author | Helbert, Jorn | |
| dc.contributor.author | Hensley, Scott | |
| dc.contributor.author | Herrick, Robert R. | |
| dc.contributor.author | Iess, Luciano | |
| dc.contributor.author | Jozwiak, Lauren | |
| dc.contributor.author | Katiaria, Tiffany | |
| dc.contributor.author | Mastrogiuseppe, Marco | |
| dc.contributor.author | Mazarico, Erwan | |
| dc.contributor.author | Mueller, Nils | |
| dc.contributor.author | Nunes, Daniel | |
| dc.contributor.author | O'Rourke, Joseph | |
| dc.contributor.author | McGovern, Patrick J. (Geophysicist) | |
| dc.contributor.author | Raguso, Maria | |
| dc.contributor.author | Stock, Joann | |
| dc.contributor.author | Tsang, Constantine | |
| dc.contributor.author | Widemann, Thomas | |
| dc.contributor.author | Whitten, Jennifer | |
| dc.contributor.author | Widemann, Thomas | |
| dc.contributor.author | Zebker, Howard | |
| dc.coverage.spatial | Venus | |
| dc.date.accessioned | 2020-09-23T18:33:03Z | |
| dc.date.available | 2020-09-23T18:33:03Z | |
| dc.date.issued | 2020 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.11753/1695 | |
| dc.description.abstract | Although supremely unhospitable to life today, Venus’s geodynamic similarities to Earth provide the ultimate control case for understanding rocky planet evolution and habitability. It very likely had past long-term surface water, as well as a dynamo. Tectonism and volcanism, with associated outgassing, likely persist today. A majority of rocky Earth-sized exoplanets lie in the high insolation “Venus-zone”. The ultimate question is are any of them habitable? | en |
| dc.description.statementofresponsibility | Primary author: Suzanne Smrekar Jet Propulsion Laboratory/California Institute of Technology, Pasadena CA ; Co-authors: Jeff Andrews-Hanna (U.AZ), Doris Breuer (DLR Berlin), Paul Byrne (NCSU), Debra Buczkowski (JHU/APL), Bruce Campbell (Nat. Air Space Museum), A. Davaille (CNRS/U. Paris-Saclay), Darby Dyar (Mt. Holyoke/PSI), G. Di Achille (INAF/Astro Obs. Teramo), Caleb Fassett (Marshall), Martha Gilmore (Wesleyan), Robert Grimm (SWRI), Jorn Helbert (DLR Berlin), Scott Hensley (JPL), Robert Herrick (U. Alaska), Luciano Iess (U.Roma), Lauren Jozwiak (JHU/APL), Tiffany Katiaria (JPL), Marco Mastrogiuseppe (U. Roma), Erwan Mazarico (Goddard), Nils Mueller (DLR Berlin), Daniel Nunes (JPL), Joseph O'Rourke (ASU); Patrick McGovern (LPI), Maria Raguso (Caltech), Joann Stock (Caltech), Constantine Tsang (SwRI), Thomas Widemann (Obs. Paris), Jennifer Whitten (Tulane), Thomas Widemann (LESIA), Howard Zebker (Stanford) | |
| dc.format.extent | 7 pages | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.relation.ispartofseries | LPI contribution ; no. 2444 | |
| dc.subject | Venus (Planet)--Exploration | en |
| dc.title | Habitability, Geodynamics, and the Case for Venus | en |
| dc.type | Working Paper | en |
Files in this item
This item appears in the following Collection(s)
-
LPI Contributions
Documents the scientific research, meetings, and outreach products from the LPI.