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Petrogenesis of melt rocks, Manicouagan impact structure, QuebecIt is suggested, on the basis of previous theoretical studies of shock waves, that the Manicouagan melt formed in 1 or 2 s in a 5-km-radius hemisphere near the point of impact. The melt and the less shocked debris surrounding it flowed downward and outward for a few minutes until the melt formed a lining of a 5- to 8-km deep, 15- to 22-km-radius cavity. Extremely turbulent flow thoroughly homogenized the melt and promoted the incorporation and progressive digestion of debris that had been finely fragmented (but not melted) to grain sizes of less than one mm by the passage of the shock waves. The equilibration of clasts and melt, plagioclase nucleation, and readjustment of the crater floor are discussed.
Document ID
19780057184
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Simonds, C. H.
(Northrop Services, Inc. Houston, Tex., United States)
Floran, R. J.
(Oak Ridge National Laboratory Oak Ridge, Tenn., United States)
Mcgee, P. E.
(Lockheed Electronics Co., Inc. Houston, Tex., United States)
Phinney, W. C.
(Northrop Services, Inc. Houston, TX, United States)
Warner, J. L.
(NASA Johnson Space Center Houston, Tex., United States)
Date Acquired
August 9, 2013
Publication Date
June 10, 1978
Publication Information
Publication: Journal of Geophysical Research
Volume: 83
Subject Category
Lunar And Planetary Exploration
Accession Number
78A41093
Funding Number(s)
CONTRACT_GRANT: NSG-7068
CONTRACT_GRANT: NSR-09-051-001
Distribution Limits
Public
Copyright
Other

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