NASA NTRS · 19810054012
Graphite-magnetite aggregates in ordinary chondritic meteorites
Abstract
The graphite-magnetite component has been found (1) as abundant isolated inclusions in eight ordinary-chondritic, regolith breccias; (2) as the sole matrix in a new kind of unequilibrated chondrite that forms clasts in these regolith breccias; and (3) together with a Huss matrix in six unequilibrated ordinary chondrites. It is suggested that the component was formed by low-temperature, gas-solid reactions before the accretion of the meteorite, and that the isolated inclusions of graphite-magnetite in regolith breccias were derived from bodies composed of the new kind of chondrite that has graphite-magnetite as its sole matrix.
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Scott, E. R. D., Taylor, G. J., Rubin, A. E., Keil, K., Okada, A.. 1981-06-18. Graphite-magnetite aggregates in ordinary chondritic meteorites. https://ntrs.nasa.gov/citations/19810054012
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