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The proposed existence of magnetic lineations in the Terra Cimmeria and Terra Sirenum regions of Mars was initially explained by Earth-like sea-floor spreading. Here we argue instead that these lineations could have been formed at a convergent p[...]texto impreso
Ruiz Pérez, Javier ; Williams, Jean-Pierre ; Dohm, James M. ; Fernández, Carlos ; López, Valle | Rosen Pub. Group | 2009Heat flow calculations based on geological and/or geophysical indicators can help to constrain the thickness, and potentially the geochemical stratification, of the martian crust. Here we analyze the Warrego rise region, part of the ancient moun[...]texto impreso
Fairén, Alberto G. ; Dohm, James M. ; Baker, Victor R. ; Pablo Hernández, Miguel Ángel de ; Ruiz Pérez, Javier ; Ferris, Justin C. ; Anderson, Robert C. | Rosen Pub. Group | 2003Throughout the recorded history of Mars, liquid water has distinctly shaped its landscape, including the prominent circum-Chryse and the northwestern slope valleys outflow channel systems, and the extremely flat northern plains topography at the[...]texto impreso
The Raz Fossae, a pair of ? 15-km wide trough en echelon interpreted as grabens, can be used to propose an estimation of the depth to the brittle–ductile transition on Triton. This estimation may in turn give an idea of the thermal state of Trit[...]texto impreso
Two opposing models to explain the geological features observed on Europa’s surface have been proposed. The thin-shell model states that the ice shell is only a few kilometers thick, transfers heat by conduction only, and can become locally thin[...]texto impreso
Fernández, Carlos ; Anguita, Francisco ; Ruiz Pérez, Javier ; Romeo Briones, Ignacio ; Martín Herrero, Álvaro Ignacio ; Rodríguez, Alberto ; Pimentel, Carlos | Rosen Pub. Group | 2009This work shows the results of a detailed structural analysis of the deformation belts of Lavinia Planitia. Ridge belts and graben and groove belts can be observed at the studied area, while wrinkle ridges and large individual grooves predominat[...]texto impreso
The present-day thermal state of the martian interior is a very important issue for understanding the 22 internal evolution of the planet. Here, in order to obtain an improved upper limit for the heat flow at 23 the north polar region, we use th[...]texto impreso
Large areas of strongly magnetized crust are located in Terra Cimmeria and Terra Sirenum, in the southern highlands of Mars, the older terrains on the planet. The typical depth to the base of the magnetized layer, deduced from the magnetic spect[...]
