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Experimental constraints on models for origins of chondrules: Peak temperaturesChondrule peak temperature constraints for mathematical models pertaining to chondrule origin are discussed in this article. The peak temperatures experienced by chondrules provide a parameter that may allow discrimination between alternative heating mechanisms. Successful mechanisms must provide just enough energy to reach such temperatures and not overshoot them. In principle, determination of peak temperatures from chondrule textures and experiments that duplicate them should be very easy. However, this approach is complicated by the fact that there are several different experimental paths that reproduce chondrule properties. The key texture depends not only on the peak temperature but also on the heating time and, in the case of totally molten droplets, on interactions with other particles. Addressed here are different types of peak temperature constraints; (1) near-liquidus melting; (2) flash melting; (3) dust seeding; (4) volatile element constraints; and (5) barred olivine chondrules.
Document ID
19950012887
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hewins, R. H.
(Rutgers Univ. Piscataway, NJ, United States)
Connolly, H. C., Jr.
(Rutgers Univ. Piscataway, NJ, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1994
Publication Information
Publication: Lunar and Planetary Inst., Papers Presented to the Conference on Chondrules and the Protoplanetary Disk
Subject Category
Astrophysics
Accession Number
95N19302
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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