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Flash melting of chondrule precursors in excess of 1600 C. Series 1: Type 2 (B1) chondrule composition experimentsSeveral questions in chondrule production remain an enigma despite years of experiments. What were the melting temperatures experienced by chondrules? What were the physical characteristics of chondrule precursors? How and why did volatile elements (i.e. Na) found within chondrules survive the formation process? We present the initial results of a series of experiments designed to investigate the above questions by using flash melting to duplicate the melting stage of chondrule formation.
Document ID
19940007705
Document Type
Conference Paper
Authors
Connolly, Harold C., Jr. (Rutgers Univ. New Brunswick, NJ, United States)
Hewins, Roger H. (Rutgers Univ. New Brunswick, NJ, United States)
Lofgren, Gary E. (NASA Lyndon B. Johnson Space Center Houston, TX., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Lunar and Planetary Inst., Twenty-fourth Lunar and Planetary Science Conference. Part 1: A-F
Subject Category
ASTROPHYSICS
Funding Number(s)
CONTRACT_GRANT: NGT-50836
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19940007055Analytic PrimarySixth Annual Workshop on Space Operations Applications and Research (SOAR 1992), volume 219940007543Analytic PrimaryTwenty-fourth Lunar and Planetary Science Conference. Part 1: A-F