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Solid-gas-equilibria in geo- and cosmochemistry; 2, Cosmochemistry

W. Schroen
Solid-gas-equilibria in geo- and cosmochemistry; 2, Cosmochemistry
European Journal of Mineralogy (December 1989) 1 (6): 765-782

Abstract

On the basis of thermodynamic trend analysis of gaseous F and Cl compounds of various elements and systematic dominance analysis, conclusions are drawn concerning the mass transfer necessary for the formation of meteorites in the early stages of the solar system, which may contribute to the explanation of metal silicate fractionation prior to the accretion of dust.


ISSN: 0935-1221
Serial Title: European Journal of Mineralogy
Serial Volume: 1
Serial Issue: 6
Title: Solid-gas-equilibria in geo- and cosmochemistry; 2, Cosmochemistry
Author(s): Schroen, W.
Affiliation: Univ. Jena, Dep. Chem., Jena, Federal Republic of Germany
Pages: 765-782
Published: 198912
Text Language: English
Summary Language: German
Publisher: Schweizerbart'sche Verlagsbuchhandlung (Naegele u. Obermiller), Stuttgart, Federal Republic of Germany
References: 43
Accession Number: 1992-062991
Categories: Petrology of meteorites and tektites
Document Type: Serial
Bibliographic Level: Analytic
Illustration Description: 8 tables
Country of Publication: Germany
Secondary Affiliation: GeoRef, Copyright 2017, American Geosciences Institute. Reference includes data from Mineralogical Abstracts, United KingdomTwickenhamUKUnited Kingdom
Update Code: 1992
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