| Literature DB >> 27337974 |
V Dehant1, D Asael2, R M Baland3, B K Baludikay2, J Beghin2, J Belza4,5, M Beuthe3, D Breuer6, S Chernonozhkin5, Ph Claeys4, Y Cornet2, L Cornet2, A Coyette3, V Debaille7, C Delvigne7, M H Deproost3, N De WInter4, C Duchemin7, F El Atrassi7, C François2, J De Keyser8, C Gillmann3, E Gloesener3, S Goderis4, Y Hidaka7, D Höning6, M Huber4, G Hublet7, E J Javaux2, Ö Karatekin3, J Kodolanyi4, L Lobo Revilla5, L Maes8, R Maggiolo4, N Mattielli7, M Maurice6, S McKibbin4, A Morschhauser6, W Neumann6, L Noack3, L B S Pham3, L Pittarello4, A C Plesa6, A Rivoldini3, S Robert8, P Rosenblatt3, T Spohn6, J -Y Storme2, N Tosi6, A Trinh3, M Valdes7, A C Vandaele8, F Vanhaecke5, T Van Hoolst3, N Van Roosbroek7, V Wilquet8, M Yseboodt3.
Abstract
The Interuniversity Attraction Pole (IAP) 'PLANET TOPERS' (Planets: Tracing the Transfer, Origin, Preservation, and Evolution of their Reservoirs) addresses the fundamental understanding of the thermal and compositional evolution of the different reservoirs of planetary bodies (core, mantle, crust, atmosphere, hydrosphere, cryosphere, and space) considering interactions and feedback mechanisms. Here we present the first results after 2 years of project work.Entities:
Keywords: Atmosphere evolution; Habitability; Impacts; Interior evolution; Mantle overturn; Planet evolution
Mesh：
Year: 2016 PMID： 27337974 DOI： 10.1007/s11084-016-9488-z
Source DB: PubMed Journal: Orig Life Evol Biosph ISSN： 0169-6149 Impact factor: 1.950