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Flash heating is required to minimize sodium losses from chondrulesChondrules were formed by high-temperature melting events, but do not always show Na depletion compared to CI chondrites, though extensive Na loss has been found in previous isothermal experiments. While Na loss can be prevented by high partial pressure of Na in the nebula, many people favor a flash-heating mechanism to reduce the Na loss from chondrule melts. To examine the validity of the flash-heating hypothesis, we have conducted a series of flash-heating experiments and observed Na loss rate under different conditions. Our results support the flash heating as a plausible heating mechanism to form chondrules.
Document ID
19950012922
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Yu, Y.
(Rutgers Univ. Piscataway, NJ, United States)
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
95N19337
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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