Water, Life, and Planetary Geodynamical Evolution |
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| Authors: | P van Thienen K Benzerara D Breuer C Gillmann S Labrosse P Lognonné T Spohn |
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| Institution: | (1) Faculty of Geosciences, Utrecht University, P.O. Box 80.021, 3508 TA Utrecht, The Netherlands;(2) Institut de Minéralogie et de Physique des Milieux Condensés, UMR 7590 and Institut de Physique du Globe de Paris, 140 Rue de Lourmel, 75015 Paris, France;(3) German Aerospace Center (DLR), Rutherfordstrasse 2, 12489 Berlin, Germany;(4) équipe études spatiales et planétologie, Institut de Physique du Globe de Paris, 4 Avenue de Neptune, 94107 Saint-Maur-des-Fossés, France;(5) Laboratoire des sciences de la Terre, école Normale Supérieure de Lyon, 46 Allée d’Italie, 69364 Lyon Cedex 07, France;(6) German Aerospace Center (DLR), Rutherfordstrasse 2, 12489 Berlin, Germany |
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| Abstract: | In our search for life on other planets over the past decades, we have come to understand that the solid terrestrial planets
provide much more than merely a substrate on which life may develop. Large-scale exchange of heat and volatile species between
planetary interiors and hydrospheres/atmospheres, as well as the presence of a magnetic field, are important factors contributing
to the habitability of a planet. This chapter reviews these processes, their mutual interactions, and the role life plays
in regulating or modulating them. |
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| Keywords: | Mantle dynamics Habitability Magnetic field Volatiles Thermal evolution |
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