Oxidized conditions in iron meteorite parent bodies
Magmatic iron meteorites are thought to originate from the cores of differentiated planetary embryos, but it is unclear where they formed in the circumstellar disk. Oxygen fugacity (fO2) is thought to have varied radially across the disk, affecting planetary accretion and core formation. Metal-silic...
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| Format: | Journal article |
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Nature Publishing Group
2018
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