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Ruiz Pérez, Javier ; Jiménez Díaz, Alberto ; Parro, Laura M. ; Egea González, Isabel ; Mansilla, Federico | Elsevier | 2019-04Two recent papers, by Karimi et al. (2016, Icarus 272, 102–113) and Karimi and Dombard (2017, Icarus 282, 34–39), tried to deduce paleo-heat flows for, respectively, Mars and Venus from modeling the viscoelastic relaxation of large impact crater[...]texto impreso
Ruiz Pérez, Javier ; Jiménez Díaz, Alberto ; Parro, Laura M. ; Mansilla, Federico ; Egea González, Isabel ; Küppers, Michael | Nature Research | 2019-07-01The surface of the dwarf planet Ceres is considered to be dominated by geological processes typical of small bodies or medium-sized icy bodies, such as impact cratering; there are also features of putative cryovolcanic origin as well as those re[...]texto impreso
Parro, Laura M. ; Jiménez Díaz, Alberto ; Mansilla, Federico ; Ruiz Pérez, Javier | Nature Publishing Group | 2017-04-03Until the acquisition of in-situ measurements, the study of the present-day heat flow of Mars must rely on indirect methods, mainly based on the relation between the thermal state of the lithosphere and its mechanical strength, or on theoretical[...]texto impreso
Egea-González, Isabel ; Jiménez Díaz, Alberto ; Parro, Laura M. ; Mansilla, Federico ; Holmes, James A. ; Lewis, Stephen R. ; Patel, Manish R. ; Ruiz Pérez, Javier | Elsevier | 2019Elysium Planitia and Oxia Planum are plains located near the Martian dichotomy. Lately, both regions have been extensively analyzed due to the major role that they play in the InSight and ExoMars missions. InSight landed in Elysium Planitia and [...]
