|
Título:
|
Paleo-heat flows, radioactive heat generation, and the coolingand deformation history of Mercury
|
|
Autores:
|
Ruiz Pérez, Javier ;
López, Valle ;
Egea González, Isabel
|
|
Tipo de documento:
|
texto impreso
|
|
Editorial:
|
Elsevier Science B.V., Amsterdam, 2013-07
|
|
Dimensiones:
|
application/pdf
|
|
Nota general:
|
info:eu-repo/semantics/openAccess
|
|
Idiomas:
|
|
|
Palabras clave:
|
Estado = Publicado
,
Materia = Ciencias: Geología: Geodinámica
,
Tipo = Artículo
|
|
Resumen:
|
Estimates of lithospheric strength for Mercury, based on the depth of thrust faults associated with large lobate scarps (which were most probably formed previously to similar to 3 Ga) or on the effective elastic thickness of the lithosphere supporting a broad rise in the northern smooth plains (whose formation is poorly constrained, but posterior to 3.8 Ga), serve as a basis for the calculation of paleo-heat flows, referred to the time when these structures were formed. The so-obtained paleo-heat flows can give information on the Urey ratio (Ur), the ratio between the total radioactive heat production and the total surface heat loss. By imposing the condition Ur
|
|
En línea:
|
https://eprints.ucm.es/id/eprint/31393/1/45-Mercurio.pdf
|
