Ferrous oxide-rich asteroid achondrites
Autor: | Christopher A. Corder, Pierre Cartigny, James M.D. Day, Nelly Assayag |
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Rok vydání: | 2019 |
Předmět: |
Solar System
Materials science 010504 meteorology & atmospheric sciences Inorganic chemistry Partial melting Oxide 010502 geochemistry & geophysics 01 natural sciences Silicate Ferrous chemistry.chemical_compound chemistry Geochemistry and Petrology Asteroid Brachinite Achondrite 0105 earth and related environmental sciences |
Zdroj: | Geochimica et Cosmochimica Acta. 266:544-567 |
ISSN: | 0016-7037 |
DOI: | 10.1016/j.gca.2019.04.005 |
Popis: | Ferrous oxide (FeO)-rich asteroid achondrites can be defined as asteroid-derived samples that experienced incipient partial melting processes in the early Solar System (>4.5 Ga) leading to melt-residues and cumulate and melt rocks that have high FeO in silicate grains (molar Mg/[Mg + Fe] |
Databáze: | OpenAIRE |
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