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The depth of subsurface liquid water on Mars as predicted from 3D thermal evolution models

Plesa, Ana-Catalina and Breuer, Doris and Stamenkovic, V. (2018) The depth of subsurface liquid water on Mars as predicted from 3D thermal evolution models. 2nd GeoPlaNet Thematic School - Fluid-Rock Interactions in the Solar System, Nantes, France.

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Item URL in elib:https://elib.dlr.de/125273/
Document Type:Conference or Workshop Item (Poster)
Title:The depth of subsurface liquid water on Mars as predicted from 3D thermal evolution models
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Plesa, Ana-CatalinaAna.Plesa (at) dlr.dehttps://orcid.org/0000-0003-3366-7621
Breuer, DorisDoris.Breuer (at) dlr.dehttps://orcid.org/0000-0001-9019-5304
Stamenkovic, V.MIT – Earth, Atmospheric and Planetary Sciences, 77 Massachusetts Avenue, Cambridge, MA 02139, USAUNSPECIFIED
Date:2018
Refereed publication:No
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:Mars, Subsurface Liquid Water, Thermal Evolution, Interior Dynamics, Habitability
Event Title:2nd GeoPlaNet Thematic School - Fluid-Rock Interactions in the Solar System
Event Location:Nantes, France
Event Type:international Conference
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Science and Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Erforschung des Weltraums
DLR - Research theme (Project):R - Vorhaben Planetary Evolution and Life, R - Vorhaben Exploration des Sonnensystems
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Deposited By: Plesa, Dr. Ana-Catalina
Deposited On:18 Dec 2018 09:34
Last Modified:18 Dec 2018 09:34

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