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Concerning the meteoritic origin of the Puchezh-Katunki craterCriticism of the works of Vardaniants (1961) and Goretskii (1962) regarding the origin of the Puchezh-Katunki crater, and development of a new hypothesis regarding this disturbance. Although Vardaniants defines the Puchezh-Katunki disturbance as a structure of explosive nature and assumes that the explosion originated as a consequence of accumulation of gases in the crystalline basement of the Russian platform, he lacks evidence to qualify this explosion as coming from a depth. Goretskii's tectonic-injection hypothesis attributes the formation of the disturbance to penetration of an intrusion of basic and ultrabasic rocks into the Paleozoic rocks of the platform. It is shown that, even if the intrusion were spread somewhere at depth, it could not account for the extent of the deformation in the disturbance. It is suggested that this disturbance is of meteoritic origin, since the structure and morphology of the region are similar to the sloping conical surface produced by an explosive meteor crater. The energy, mass, and size of the asteroid which could cause such a disturbance are estimated, and it is shown that the probability of the occurrence of an impact of this size is finite over geological time.
Document ID
19740031033
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Firsov, L.
Kieffer, S. W.
(Akademiia Nauk SSSR Institut Geologii i Geofiziki, Novosibirsk, Ussr)
Date Acquired
August 7, 2013
Publication Date
September 30, 1973
Publication Information
Publication: Meteoritics
Volume: 8
Subject Category
Space Sciences
Accession Number
74A13783
Funding Number(s)
CONTRACT_GRANT: NGL-05-002-003
Distribution Limits
Public
Copyright
Other

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