THE ORIGIN OF PLANETOCENTRIC METEORITES

dc.contributor.author	Marakushev A.A.
dc.date.accessioned	2020-12-02T10:17:16Z
dc.date.available	2020-12-02T10:17:16Z
dc.date.issued	1996
dc.identifier	https://elibrary.ru/item.asp?id=20957613
dc.identifier.citation	Vestnik Moskovskogo universiteta. Seriâ 4: Geologiâ, 1996, , 3, 3-14
dc.identifier.issn	0579-9406
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/20108
dc.description.abstract	The meteorites of the Solar System can be divided into heliocentric and planetocentric. The heliocentric meteorites originated in the asteroid belt while the origin of the planetocentric meteorites is associated with the destruction of satellites of planets. Satellites are a natural 'product' of planets which occurred by separation from the fluid casing of the planet in the form of molten fluid silicate masses under the influence of centrifugal forces. On consolidation on the surface a stressed state arose within the satellite, expressed as explosive volcanism. Some satellites disintegrated as a result of this and formed planetocentric meteorites. Planetocentric meteorites are examined with reference to the planets of the solar system.
dc.title	THE ORIGIN OF PLANETOCENTRIC METEORITES
dc.type	Статья

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