Os, Re, Ir, Ru, Rh, Pd, AU in borehole samples from the Clearwater East Crater (Canada) and the Boltysh Impact Crater (Ukraine)

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Hypervelocity Impact, Meteorite Craters, Meteoritic Composition, Chondrites, Chromium, Rare Earth Elements, Canada, Boreholes, Osmium, Rhenium, Iridium, Rubidium, Rhodium, Palladium, Gold

Scientific paper

The identification of projectiles of terrestrial impact craters may be deduced from melt rock siderophile and highly siderophile element abundances and interelement ratios. High concentrations of strongly siderophile trace elements have been detected in the East Clearwater melt rocks. Chondrite-normalized ratios and the apparent presence of meteoritic Cr suggested the presence of around 7 percent of a chondritic component (nickel concentrations 5 to 10 percent CI-chondritic abundances) in the impact melt. From Boltysh, so far only eight samples have been analyzed; three contain less than 1 ng/g Ir and five contain about 0.1 ng/g Ir. Grieve et al. (1987) concluded that the impactor could have been a stony projectile if the Ni (43 micro-g/g), Cr (56 micro-g/g), and Ir enrichments are meteoritic in origin. The purpose of this study was to better characterize the meteoritic signatures of these two craters by additional analyses of highly siderophile elements (especially the less often analyzed elements Os, Rh and Ru) which can be used to distinguish between magmatic iron meteorites and nonmagmatic iron meteorites and chondrites.

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