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Certain peculiarities in the distribution of mercury in meteorites
Authors:N.A. Ozerova  L.G. Kvasha  G.A. Bulkin  N.Kh. Aidinian
Affiliation:Institute of Geology of Ore Deposits, Petrography, Mineralogy and Geochemistry of the Academy of Sciences of the U.S.S.R., MoscowU.S.S.R.;Committee on Meteorites of the Academy of Sciences of the U.S.S.R., MoscowU.S.S.R.;All-Union Geological Scientific Research Institute, LeningradU.S.S.R.;Institute of Geology of Ore Deposits, Petrography, Mineralogy and Geochemistry of the Academy of Sciences of the U.S.S.R., MoscowU.S.S.R.
Abstract:This paper presents chemical analyses of mercury in 123 specimens of 58 meteorites. A statistical comparison is made of the mercury content in meteorites (using all available data) as a function of their composition and texture.The average mercury abundance in stony meteorites is estimated as 6.6 ppm. Stony and iron meteorites differ significantly in mercury content. Among stones, chondrites and achondrites show significant differences in the mercury content. In ordinary cbondrites, mineralogy and texture do not seem to have a significant influence on the distribution of mercury, judging from the available number of analyses. Carbonaceous chondrites, in which we found up to 500 ppm mercury, stand out among all other varieties of chondrites. Iron meteorites fall at the other extreme, having the lowest mercury concentrations (generally 0-0x ppm). In specimens of several meteorite classes, troilite is a good mercury concentrator, having a consistently higher mercury content than the meteorite as a whole. Nonetheless, troilite generally accounts for less than one-half the total mercury content of the meteorite.
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