On presolar meteoritic sulphides

Details On presolar meteoritic sulphides On presolar meteoritic sulphides

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.265..427c&link_type=abstract

Nature, vol. 265, Feb. 3, 1977, p. 427, 428. Research supported by the University College, Science Research Council, of England,

Computer Science

14

Meteoritic Composition, Sulfides, Supernova Remnants, Mineralogy, Refractory Materials, Titanium Compounds

Scientific paper

Questions concerning the survival of supernovae condensates with unique signatures are considered. The conduction of a search among the ubiquitous sulfides present in meteorites is proposed. Particular attention in this search is to be given to sulfides of titanium. It is thought that many sulfides, especially of titanium, will not be expected in solar condensation sequences but are expected to dominate certain key zones of supernovae expansion. In the case of titanium, it seems likely that the refractory oxides made in the solar sequence will not be reduced later by hydrogen sulfide.

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