THERMOBAROMETRY OF ORDINARY CHONDRITES

dc.contributor.author	Zinovieva N.G.
dc.contributor.author	Pletchov P.Yu.
dc.contributor.author	Latyshev N.P.
dc.contributor.author	Granovsky L.B.
dc.date.accessioned	2024-11-02T11:07:41Z
dc.date.available	2024-11-02T11:07:41Z
dc.date.issued	2006
dc.identifier	https://www.elibrary.ru/item.asp?id=13520548
dc.identifier.citation	Doklady Earth Sciences, 2006, 409, 5, 758-761
dc.identifier.issn	1028-334X
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/46322
dc.description.abstract	Ordinary chondrites are the most abundant type of meteorites. However, their genetic interpretation, accepted in modern literature and based on independent investigations of the formation of droplike silicate chondrules and the kamacite matrix, is obviously inconsistent with results of their petrographic and experimental studies, indicating the joint formation of the chondrules and chondrite matrix as a result of the development of iron–silicate immiscibility, which defined their compositional relationships according to Prior’s rules.
dc.title	THERMOBAROMETRY OF ORDINARY CHONDRITES
dc.type	Статья
dc.identifier.doi	10.1134/S1028334X06050187

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