FORMISANO, MichelangeloMichelangeloFORMISANOFederico, CostanzoCostanzoFedericoCastillo-Rogez, JulieJulieCastillo-RogezDE SANCTIS, MARIA CRISTINAMARIA CRISTINADE SANCTISMagni, GianfrancoGianfrancoMagni2024-05-302024-05-302019http://hdl.handle.net/20.500.12386/35169In this work we demonstrated that the thermal convection probably is not likely in the Ceres' crust. In fact, it is possible only for a narrow set of thermophysical parameters. This result implies that: I) dome formation (like Ahuna Mons) is probably due to the diapirism rather than thermal convection; II) deep brine reservoir are possible until now.ELETTRONICOenConference abstracthttps://www.epsc-dps2019.eu/2019EPSC...13.1632FFIS/05 - ASTRONOMIA E ASTROFISICA