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From meteorites to evolution and habitability of planets

Dehant, V. and Breuer, D. and Claeys, P. and Debaille, V. and De Keyser, J. and Javaux, E. and Goderis, S. and Karatekin, O. and Spohn, Tilman and Vandaele, A.C. and Vanhaecke, F. and Van Hoolst, T. and Wilquet, V. (2012) From meteorites to evolution and habitability of planets. Planetary and Space Science, 72 (1), pp. 3-17. Elsevier. DOI: 10.1016/j.pss.2012.05.018 ISSN 0032-0633

Full text not available from this repository.

Official URL: http://www.sciencedirect.com/science/article/pii/S0032063312001316

Abstract

The evolution of planets is driven by the composition, structure, and thermal state of their internal core, mantle, lithosphere, and crust, and by interactions with a possible ocean and/or atmosphere. A planet’s history is a long chronology of events with possibly a sequence of apocalyptic events in which asteroids, comets and their meteorite offspring play an important role. Large meteorite impacts on the young Earth could have contributed to the conditions for life to appear, and similarly large meteorite impacts could also create the conditions to erase life or drastically decrease biodiversity on the surface of the planet. Meteorites also contain valuable information to understand the evolution of a planet through their gas inclusion, their composition, and their cosmogenic isotopes. This paper addresses the evolution of the terrestrial bodies of our Solar System, in particular through all phenomena related to meteorites and what we can learn from them. This includes our present understanding of planet formation, their interior, their atmosphere, and the effects and relations of meteorites with respect to these reservoirs. It brings further insight into the origin and sustainability of life on planets, including Earth. Particular attention is devoted to Earth and Mars, as well as to planets and satellites possessing an atmosphere (Earth, Mars, Venus, and Titan) or a subsurface ocean (e.g., Europa), because those are the best candidates for hosting life. Though the conditions on the planets Earth, Mars, and Venus were probably similar soon after their formation, their histories have diverged about 4 billion years ago. The search for traces of life on early Earth serves as a case study to refine techniques/environments allowing the detection of potential habitats and possible life on other planets. A strong emphasis is placed on impact processes, an obvious shaper of planetary evolution, and on meteorites that document early Solar System evolution and witness the geological processes taking place on other planetary bodies. ► Definition of habitability related to geophysical reservoirs and planetary evolution. ► Influence of sun and impacts on atmospheres evolution and planets habitats. ► Preservation and sustainability is important for life and biosignature preservation.

Item URL in elib:https://elib.dlr.de/77065/
Document Type:Article
Title:From meteorites to evolution and habitability of planets
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Dehant, V.Royal Observatory of Belgium, Brussels, BelgiumUNSPECIFIED
Breuer, D.doris.breuer (at) dlr.deUNSPECIFIED
Claeys, P.Vrije Universiteit Brussel, Brussels, BelgiumUNSPECIFIED
Debaille, V.Université Libre de Bruxelles, Brussels, BelgiumUNSPECIFIED
De Keyser, J.Belgian Institute for Space Aeronomy, Brussels, BelgiumUNSPECIFIED
Javaux, E.Université de Liège, 4000 Liège 1, BelgiqueUNSPECIFIED
Goderis, S.Vrije Universiteit Brussel, Brussels, BelgiumUNSPECIFIED
Karatekin, O.Royal Observatory of Belgium, 3 avenue Circulaire, Brussels, B-1180, BelgiumUNSPECIFIED
Spohn, TilmanTilman.Spohn (at) dlr.deUNSPECIFIED
Vandaele, A.C.Belgian Institute for Space Aeronomy, Brussels, BelgiumUNSPECIFIED
Vanhaecke, F.Universiteit Gent, Brussels, BelgiumUNSPECIFIED
Van Hoolst, T.Royal Observatory of Belgium, Brussels, BelgiumUNSPECIFIED
Wilquet, V.Belgian Institute for Space Aeronomy, Brussels, BelgiumUNSPECIFIED
Date:2012
Journal or Publication Title:Planetary and Space Science
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:72
DOI :10.1016/j.pss.2012.05.018
Page Range:pp. 3-17
Publisher:Elsevier
ISSN:0032-0633
Status:Published
Keywords:Terrestrial planets; Habitability; Meteorites
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben Exploration des Sonnensystems (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Institute of Planetary Research
Deposited By: Noack, Lena
Deposited On:19 Sep 2012 08:26
Last Modified:01 Dec 2018 19:48

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