Evaluación termodinámica del modelo concrítico de los planetas terrestres

dc.contributor.author	Casanova, I.
dc.contributor.author	Portela, J. C
dc.date.accessioned	2016-10-10T12:22:25Z
dc.date.available	2016-10-10T12:22:25Z
dc.date.issued	1996
dc.description.abstract	A new algorithm for the estimation of minera! phase chemistry condensed from a gas of solar composition has been elaborated. Extension of this method to low temperatures provides a very good match with bulk Earth composition, suggesting that equilibrium condensation may be a valid approach for estimating bulk chemistries of terrestrial-like planets	en_US
dc.identifier.uri	http://hdl.handle.net/10272/12741
dc.language.iso	spa	en_US
dc.publisher	Sociedad Geológica de España	en_US
dc.rights	Atribución-NoComercial-SinDerivadas 3.0 España	*
dc.rights.accessRights	open access	en_US
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/3.0/es/	*
dc.subject.other	Condensación	en_US
dc.subject.other	Condrito	en_US
dc.title	Evaluación termodinámica del modelo concrítico de los planetas terrestres	en_US
dc.title	Thermodynamic evaluation of the chondritic model for the terrestrial planets	eng
dc.type	journal article	en_US
dspace.entity.type	Publication

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