Computer Science
Scientific paper
Jan 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996eiaf.conf...37w&link_type=abstract
Workshop on Evolution of Igneous Asteroids: Focus on Vesta and the HED Meterorites, p. 37
Computer Science
Meteoritic Composition, Pyroxenes, Isotope Ratios, Cosmochemistry, Textures, Meteoroids, Grain Size, Chromites
Scientific paper
Among several eucrites we have been studying by our usual methods, two stand out as extraordinary cumulates: Asuka 881394, a volatile-depleted cumulate eucrite, and EET 87548, an extraordinarily pyroxene- and chromite-rich cumulate eucrite. The medium-grained granular texture of Asuka 881394 is possibly altered from the original igneous texture, and difficult to categorize in terms of cumulate vs. noncumulate origin. Based on low incompatible-element contents and (+) Eu anomaly (Sm = 0.29 micro gram per gram, Eu - 0.27 micro gram/g [I]) and high mg# (56.6 mol%), we infer it is a cumulate. Even so, its extremely low concentrations of volatile elements seem remarkable. The Ga/Al ratio (0.010 x CI) is also exceptionally low. This sample tends to blur the distinction between eucrites and angrites. However, many significant differences vs. angrites remain. For example, the Fe/Mn ratio (34) is typical for eucrites, and only 0.4 times the lowest Fe/Mn among angrites.
Kallemeyn Gregory W.
Kaneda Kazuhisa
Warren Harry P.
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