Igneous rock from Severnyi Kolchim (H3) chondrite: Nebular origin

Details Igneous rock from Severnyi Kolchim (H3) chondrite: Nebular origin Igneous rock from Severnyi Kolchim (H3) chondrite: Nebular origin

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24.1055n&link_type=abstract

In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z p 1055-1056 (SEE N94-20636 05-91

Computer Science

Carbonaceous Chondrites, Chondrites, Chondrule, Igneous Rocks, Meteoritic Composition, Fragments, Rocks, Textures

Scientific paper

The discovery of lithic fragments with compositions and textures similar to igneous differentiates in unequilibrated ordinary chondrites (UOC's) and carbonaceous chondrites (CC's) has been interpreted as to suggest that planetary bodies existed before chondrites were formed. As a consequence, chondrites (except, perhaps CI chondrites) cannot be considered primitive assemblages of unprocessed nebular matter. We report about our study of an igneous clast from the Severnyi Kolchim (H3) chondrite. The results of the study are incompatible with an igneous origin of the clast but are in favor of a nebular origin similar to that of chondrules.

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