A. Herrero-Gil (et al.)- Large thrust faults on Mars are caused by lithospheric planetary contraction. The geometry of these faults … Más
Etiqueta: Martínez Parro-L.
From hot to cold? – Hydrothermal activities as a source for icy-debris flows on Dryas Mons, Terra Sirenum, Mars
M. Voelker (et al.)- During an extensive grid-mapping campaign on Mars’ southern hemisphere, we have detected so-called sheet flow deposits, … Más
Comments on “Using the viscoelastic relaxation of large impact craters to study the thermal history of Mars” (Karimi et al., 2016, Icarus 272, 102–113) and “Studying lower crustal flow beneath mead basin: Implications for the thermal history and rheology of Venus” (Karimi and Dombard, 2017, Icarus 282, 34–39)
Javier Ruiz (et al.)- Two recent papers, by Karimi et al. (2016, Icarus 272, 102–113) and Karimi and Dombard (2017, Icarus … Más
The thermal structure and mechanical behavior of the Martian lithosphere
Alberto Jiménez-Díaz (et al.)- In depth knowledge of the thermal and rheological properties of the crust and mantle of Mars … Más
Regional heat flow and subsurface temperature patterns at Elysium Planitia and Oxia Planum areas, Mars
Isabel Egea-Gonzalez (et al.)- Elysium Planitia and Oxia Planum are plains located near the Martian dichotomy. Lately, both regions have been extensively … Más
Evidence of thrust faulting and widespread contraction of Ceres
Javier Ruiz (et al.)- The surface of the dwarf planet Ceres is considered to be dominated by geological processes typical … Más
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