Abstract
Practically all of the examined spherules extracted in 1948–1949 from soil at the crater field of the 1947 Sikhote Alin meteorite shower are ablation spherules produced during this meteorite fall. The spherules can classified into two textural types: (i) fine-grained, which consist of Ni-bearing magnetite (3–6 wt % NiO) dendrites, sometimes with minor amounts of interstitial P- and Fe-rich material, and (ii) coarse-grained, which also consist of Ni-bearing magnetite dendrites or grains, sometimes with wuestite, an interstitial material, which resembles that in type (i) or has a silicate composition. The texture, mineralogy, and chemistry (presence of P and Si) of these spherules differ from those of iron cosmic spherules (type I) that occur in the background flux of micrometeorites. The spherules are thought to were produced by the ablation of meteoritic material at elevations of about 12 km (in the region where disintegration starts) and below, at maximum temperatures of 1600–2180°C and oxygen fugacity of 10−14 to 10−1 atm. Conceivably, the ablated material was enriched in silicates compared to the fallen material.
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Original Russian Text © D.D. Badyukov, J. Raitala, 2012, published in Petrologiya, 2012, Vol. 20, No. 6, pp. 574–582.
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Badyukov, D.D., Raitala, J. Ablation spherules in the Sikhote Alin meteorite and their genesis. Petrology 20, 520–528 (2012). https://doi.org/10.1134/S086959111206001X
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DOI: https://doi.org/10.1134/S086959111206001X