ORIGIN OF ULTRAMAFIC-HOSTED VEIN MAGNESITE DEPOSITS

dc.contributor.author	Abu-Jaber N.S.
dc.contributor.author	Kimberley M.M.
dc.date.accessioned	2020-11-09T07:44:47Z
dc.date.available	2020-11-09T07:44:47Z
dc.date.issued	1992
dc.identifier	https://elibrary.ru/item.asp?id=31594230
dc.identifier.citation	Ore Geology Reviews, 1992, , 3, 155-191
dc.identifier.issn	0169-1368
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/18714
dc.description.abstract	Large deposits of magnesite (MgCO3) occur either as carbonated ultramafic rocks or as sedimentary beds. The origins of both sedimentary and ultramafic-hosted deposits remain controversial, as does the relationship between them. Ultramafic-hosted deposits are reviewed herein, with an emphasis on veins rather than massive bodies. Magnesium apparently has been supplied to magnesite veins by their ultramafic host. Uncertainties concerning ultramafic-hosted deposits include the source, state, and mode of transportation of carbon, the cause of its precipitation, and the mineralogy of the initial precipitate.
dc.title	ORIGIN OF ULTRAMAFIC-HOSTED VEIN MAGNESITE DEPOSITS
dc.type	Статья

Files in this item

Files	Size	Format	View
There are no files associated with this item.