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From meteorites to evolution and habitability of planets

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

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


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.

Titel:From meteorites to evolution and habitability of planets
AutorenInstitution oder E-Mail-AdresseAutoren-ORCID
Dehant, V.Royal Observatory of Belgium, Brussels, BelgiumNICHT SPEZIFIZIERT
Breuer, D.doris.breuer@dlr.deNICHT SPEZIFIZIERT
Claeys, P.Vrije Universiteit Brussel, Brussels, BelgiumNICHT SPEZIFIZIERT
Debaille, V.Université Libre de Bruxelles, Brussels, BelgiumNICHT SPEZIFIZIERT
De Keyser , J.Belgian Institute for Space Aeronomy, Brussels, BelgiumNICHT SPEZIFIZIERT
Javaux, E.Université de Liège, 4000 Liège 1, BelgiqueNICHT SPEZIFIZIERT
Goderis, S.Vrije Universiteit Brussel, Brussels, BelgiumNICHT SPEZIFIZIERT
Karatekin, O.Royal Observatory of Belgium, 3 avenue Circulaire, Brussels, B-1180, BelgiumNICHT SPEZIFIZIERT
Spohn, T.Tilman.Spohn@dlr.deNICHT SPEZIFIZIERT
Vandaele, A.C.Belgian Institute for Space Aeronomy, Brussels, BelgiumNICHT SPEZIFIZIERT
Vanhaecke, F.Universiteit Gent, Brussels, BelgiumNICHT SPEZIFIZIERT
Van Hoolst, T.Royal Observatory of Belgium, Brussels, BelgiumNICHT SPEZIFIZIERT
Wilquet, V.Belgian Institute for Space Aeronomy, Brussels, BelgiumNICHT SPEZIFIZIERT
Erschienen in:Planetary and Space Science
Referierte Publikation:Ja
In Open Access:Nein
In ISI Web of Science:Ja
DOI :10.1016/j.pss.2012.05.018
Seitenbereich:Seiten 3-17
Stichwörter:Terrestrial planets; Habitability; Meteorites
HGF - Forschungsbereich:Verkehr und Weltraum (alt)
HGF - Programm:Weltraum (alt)
HGF - Programmthema:W EW - Erforschung des Weltraums
DLR - Schwerpunkt:Weltraum
DLR - Forschungsgebiet:W EW - Erforschung des Weltraums
DLR - Teilgebiet (Projekt, Vorhaben):W - Vorhaben Exploration des Sonnensystems (alt)
Standort: Berlin-Adlershof
Institute & Einrichtungen:Institut für Planetenforschung > Planetenphysik
Institut für Planetenforschung
Hinterlegt von: Noack, Lena
Hinterlegt am:19 Sep 2012 08:26
Letzte Änderung:11 Dez 2017 10:42

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