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Geochemical investigations to explain iodine-overabundances in Antarctic meteorites

Journal Article · · Geochim. Cosmochim. Acta; (United States)

Iodine, bromine, and chlorine concentrations were determined in different Antarctic meteorite specimens with isotope dilution mass spectrometry. In all Antarctic meteorites I-overabundances have been analyzed compared with the concentrations for non-Antarctic meteorites of the same class. Half of the Antarctic specimens show especially high concentrations of more than 1 ..mu..g/g. By analyzing different types of Antarctic rocks, a significant decrease of the I concentration-but not of the Br and Cl concentration-was determined from the surfaces to the centers of the rocks. This shows that atmospheric I compounds interact with the surfaces of Antarctic rocks and, therefore, with those of Antarctic meteorites as well. Analyses of atmospheric halogens show that the gaseous compound CH/sub 3/I is probably responsible for the I-overabundance in Antarctic meteorites and rocks. Chloride and bromide are found in particles derived from sea-spray in Antarctic aerosols. Deposition of halogens in Antarctic snow near the coast shows I/Cl ratios 10-190 higher than the average value for sea water. The corresponding Br/Cl ratios are in the same range as sea water. On the basis of these results and of other reported data the authors construct a preliminary hypothesis for a geochemical I cycle in Antarctica, taking into consideration long-distance and short-distance transportation of different I compounds from the coast to inland Antarctica.

Research Organization:
Universitaetsstrasse, Regensburg (West Germany)
OSTI ID:
5100007
Journal Information:
Geochim. Cosmochim. Acta; (United States), Journal Name: Geochim. Cosmochim. Acta; (United States) Vol. 51:9; ISSN GCACA
Country of Publication:
United States
Language:
English