Water and the Interior Structure of Terrestrial Planets and Icy Bodies

Julien Monteux (1) , G. J Golabek , D. C Rubie , G. Tobie (2) , E. D Young

1 LMV - Laboratoire Magmas et Volcans
2 LPG - Laboratoire de Planétologie et Géodynamique [UMR 6112]

Water content and the internal evolution of terrestrial planets and icy bodies are closely linked. The distribution of water in planetary systems is controlled by the temperature structure in the protoplanetary disk and dynamics and migration of planetesimals and planetary embryos. This results in the formation of planetesimals and planetary embryos with a great variety of compositions, water contents and degrees of oxidation. The internal evolution and especially the formation time of

Domaines: Géophysique [physics.geo-ph]

Julien Monteux, G. J Golabek, D. C Rubie, G. Tobie, E. D Young. Water and the Interior Structure of Terrestrial Planets and Icy Bodies. Space Science Reviews, 2018, 214 (1), ⟨10.1007/s11214-018-0473-x⟩. ⟨hal-01907486⟩