Silicon Carbide From a Carbon Nodule in the Canyon Diablo Meteorite

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[6015] Planetary Sciences: Comets And Small Bodies / Dust, [6022] Planetary Sciences: Comets And Small Bodies / Impact Phenomena, [6240] Planetary Sciences: Solar System Objects / Meteorites And Tektites

Scientific paper

The Canyon Diablo Meteorite fell in the Arizona desert 50,000 years ago, giving rise to the well-preserved Meteor Crater. Irons of various sizes were scattered around the crater rim and on the surrounding plains. We studied a rusty specimen containing a carbon nodule. We dug out small blocks of sooty carbon by means of a sharp tungsten carbide tip. These carbon materials contain traces of silicon carbide (SiC) and diamond/lonsdaleite. We report here our findigs of two groups of SiC grains. (1) Relatively large crystals, about 80-90 microns in size. Their colors are in shades of blue, green and neutral. One of the grains are composed of a cluster of 3 crystals of the 3C polytype, whereas, 7 other individual crystals are of hexagonal structure. All crystals in this group have dark, rounded resorption rims. (2) Small crystals, about 30-50 microns in size. They are pale blue in color, and they lack dark-colored rims. These two distinct groups probably have different modes of origin. The large crystals seem to be early-formed, but had been reheated or partially melted, as indicated by the bead-like rims. The complexities displayed by these SiC crystals might have resulted from a long residence time in the meteorite while it was still in space. Their origin might be akin to that of SiC occurring in carbonaceous chondrites and interplanetary dust particles.

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