Chondrule and chondrite formation: Major unresolved issues

Details Chondrule and chondrite formation: Major unresolved issues Chondrule and chondrite formation: Major unresolved issues

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994metic..29..553w&link_type=abstract

Meteoritics (ISSN 0026-1114), vol. 29, no. 4, p. 553

Computer Science

Chondrites, Chondrule, Geochronology, Inclusions, Parameterization, Temperature Effects, Chemical Composition, Cooling, Mineralogy, Particle Size Distribution, Volatility

Scientific paper

There is widespread (though not universal) agreement on only a few aspects of chondrule formation: they were created as dispersed igneous droplets in the nebula, and cooled on a timescale of order 1 hr; some if not all incorporated an earlier generation of mineral grains. Beyond this, many of the parameters and processes that affected their formation are disputed. The present paper attempts to identify the most important unresolved issues, name the several positions that have been taken on them, and suggest tests that might resolve the problem.

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