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Chondrules as condensation productsThe formation of meteoritic chondrules via condensation from the primordial solar nebula is discussed. Chondrule formation in regions where the gas/dust ratio was enhanced, and where transient high energy events heated the gas and temporarily vaporized the dust, is advocated. The observed diversity of chondrule types can be understood as resulting from local variations in the initial gas/dust proportions and other parameters.
Document ID
19780035889
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Wood, J. A. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Mcsween, H. Y., Jr. (Harvard College Observatory and Smithsonian Astrophysical Observatory, Center for Astrophysics, Cambridge Mass., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1977
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: International Colloquium
Location: Lyons
Country: France
Start Date: August 17, 1976
End Date: August 20, 1976
Accession Number
78A19798
Funding Number(s)
CONTRACT_GRANT: NSG-7132
Distribution Limits
Public
Copyright
Other

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