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NASA NTRS · 19870060774

Diverse eucritic pebbles in the Vaca Muerta mesosiderite

Abstract

Seven 5-cm basaltic pebbles from the Vaca Muerta mesosiderite were studied by neutron activation and electron microprobe analysis, and three additional pebbles were studied petrographically. The cumulate pebbles had low REE concentrations and high Eu/Sm ratios, indicating the absence of intercumulus liquid. Siderophile interelement ratios were similar to those found in Vaca Muerta metal except for anomalously low Ir concentrations. The presence of 20 percent impact-melt breccias among the pebbles and 35-40 percent melt breccias among the mesosiderite whole-rocks suggests that the mesosiderites were more extensively impact melted than the howardites. Three alternative models to explain this greater proportion of impact-melted material among the mesosiderites are proposed.

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BibTeXRIS

Rubin, Alan E., Jerde, Eric A.. 1987-06-01. Diverse eucritic pebbles in the Vaca Muerta mesosiderite. https://ntrs.nasa.gov/citations/19870060774

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