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NUCLEAR REACTIONS IN IRON METEORITES (in Russian)

Journal Article · · Geokhimiya (U.S.S.R.) For English translation 1956-63 see Geochemistry (USSR)
OSTI ID:4819914
Iron spallation by cosmic particles is the chief nuclear process in iron meteorites. About 10/sup 07/ g/g of cosmogenic isotopes per gram of meteorite accumulate during 4.5 x 10/sup 9/ years. The stable isotopes Ar/sup 36/, Ar/sup 38/, K/sup 40/, Sc/sup 45/, and V/sup 50/ in iron meteorites are of cosmogenic origin. Observed anomalies in the isotopic composition of argon and potassium may be explained by deep spallation reactions. For isotopes of vanadium and titanium and of other elements, the abundance of which is 10/sup -6/ to 10/sup -7/ g/g, shifts in the isotopic composition in iron meteorites relative to rocks of the earth may be expected. Equilibrium activity values were estimated for long- lived cosmogenic nuclei detected in iron meteorites. The average effective energy of nuclei formation A approximates 20 and approximates 40 was estimated. (auth)
Research Organization:
Vernadskii Inst. of Geochemistry and Analytical Chemistry, Moscow
NSA Number:
NSA-16-006886
OSTI ID:
4819914
Journal Information:
Geokhimiya (U.S.S.R.) For English translation 1956-63 see Geochemistry (USSR), Journal Name: Geokhimiya (U.S.S.R.) For English translation 1956-63 see Geochemistry (USSR) Vol. Vol: No. 11; ISSN GEOKA
Country of Publication:
Country unknown/Code not available
Language:
Russian

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