Experimental simulations of sulfide formation in the solar nebula.

Details Experimental simulations of sulfide formation in the solar nebula. Experimental simulations of sulfide formation in the solar nebula.

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997sci...277..358l&link_type=abstract

Science, Vol. 277, No. 5324, p. 358 - 360

Mathematics

Logic

33

Solar Nebula: Laboratory Simulations

Scientific paper

Sulfurization of meteoritic metal in H2S-H2 gas produced three different sulfides: monosulfide solid solution [(Fe,Ni)1-xS], pentlandite [(Fe,Ni)9-xS8], and a phosphorus-rich sulfide. The composition of the remnant metal was unchanged. These results are contrary to theoretical predictions that sulfide formation in the solar nebula produced troilite (FeS) and enriched the remaining metal in nickel. The experimental sulfides are chemically and morphologically similar to sulfide grains in the matrix of the Alais (class Cl) carbonaceous chondrite, suggesting that these meteoritic sulfides may be condensates from the solar nebula.

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