Cumulate Eucrites: Volatile-Depleted Asuka 881394, Chromium-Loaded EET 87548 and Cumulate Versus Noncumulate Relationships

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Meteoritic Composition, Pyroxenes, Isotope Ratios, Cosmochemistry, Textures, Meteoroids, Grain Size, Chromites

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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.

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