Other
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994metic..29r.439a&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 29, no. 4, p. 439
Other
4
Barium Compounds, Chemical Composition, Chondrites, Meteoritic Composition, Sulfates, Chemical Analysis, Inclusions, Meteoritic Microstructures, Mineralogy, Trace Elements, Weathering
Scientific paper
Acfer 086 (CV3) was recovered from the Sahara in 1989. A thin section was studied for weathering products. During routine microprobe analysis a phase was found containing Ba and S in approximate 1:1 atomic ratio. The only other element detected at more than trace level was Fe (less than 2%), possibly from surrounding Fe-rich phases. It is concluded that the only likely mineral with this chemistry is barytes, BaSO4. The barytes occurs as isolated, 1-10-micron, irregularly shaped grains. It is present exclusively in inclusions, both metal/C-rich and chondrules and chondrule fragments. None were observed in the matrix. At its highest the barytes density reached greater than 50 grains in an area measuring 300 x 200 microns. At present, whether the barytes is terrestrial or meteoritic remains unclear. Reasons for both cases are given and discussed. While it is an intriguing possibility that the barytes in Acfer 086 may be a primary meteoritic mineral, and considerable evidence would support this view, it must be treated with great caution. Although texturally it is unlike a secondary phase and there are difficulties with the introduction of barytes by groundwater, this cannot be dismissed. The high and variable Ba contents of the Acfer/El Djouf Saharan CR chondrites are strong evidence for the formation of secondary barytes during residence on the desert floor. If terrestrial, the presence and distribution pattern of barytes in Acfer 086 has potentially important consequences for chemical and isotopic analyses of many elements in both bulk and inclusions of meteorite finds from the deserts of the world.
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