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Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988metic..23...49p&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 23, March 1988, p. 49-57.
Other
21
Chemical Composition, Grain Size, Metal Compounds, Meteoritic Composition, Mineralogy, Rare Gases, Australia, Basalt, Igneous Rocks, Pyroxenes, Meteorites, Camel Donga, Eucrites, Metal, Composition, Chemistry, Iron, Mineralogy, Rare Gases, Comparisons, Origin, Formation, Lithology, Inaa, Reduction, Homogeneity, Distribution, Sulfides, Heating, Procedure, Sem, Laboratory Studies, Samples, Meteorite, Petrography, Photomicrographs, Refractory Material, Lithophiles, Sulfur, Electron Microscopy, Johnstown, Neutr
Scientific paper
The Camel Donga eucrite is unique since it contains about 2 percent metallic iron. Chemical composition, mineralogy, and noble-gas contents of Camel Donga are, however, indistinguishable from other eucrites. The bulk iron content and the composition of the metal show that the camel Donga metal was formed by reduction of FeO and FeS, probably through loss of S2 and SO2. Since coarse- and fine-grained lithologies are affected, it is likely that the reduction occurred after brecciation. The inhomogeneous distribution of metal suggests that reduction is limited to areas where sulfides were present. The fact that major parts of the meteorite still contain sulfides, in many cases associated with metal, indicates that the reduction process did not go to completion. A comparatively short heating period is suggested, perhaps in an ejecta blanket.
Dreibus Gerlind
Palme Herbert
Spettel Bernhard
Weber Harald
Wlotzka Frank
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