RHENIUM OXIDE, POTASSIUM PERRHENATE, IRON AND ALUMINUM HYDROXYCHLORIDES, BARITE, AND CELESTINE IN LUNAR REGOLITH

dc.contributor.author	Mokhov A.V.
dc.contributor.author	Bogatikov O.A.
dc.contributor.author	Kartashov P.M.
dc.contributor.author	Gorshkov A.I.
dc.contributor.author	Koporulina E.V.
dc.contributor.author	Magazina L.O.
dc.contributor.author	Ashikhmina N.A.
dc.date.accessioned	2024-11-09T08:38:20Z
dc.date.available	2024-11-09T08:38:20Z
dc.date.issued	2006
dc.identifier	https://www.elibrary.ru/item.asp?id=13529043
dc.identifier.citation	Doklady Earth Sciences, 2006, 407, 3, 460-464
dc.identifier.issn	1028-334X
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/46442
dc.description.abstract	The continuing study of lunar regolith with a JSM-5610LV low-vacuum electron microscope equipped with EDS JED-2300 JEOL (Japan) made it possible to detect several oxygen-bearing phases and associated native metal in one case. These findings are of special genetic interest. The case in point is an intergrowth of native rhenium with rhenium oxide, oxides of rhenium and potassium, hydroxides of iron and aluminum, and sulfates of barium and strontium.
dc.title	RHENIUM OXIDE, POTASSIUM PERRHENATE, IRON AND ALUMINUM HYDROXYCHLORIDES, BARITE, AND CELESTINE IN LUNAR REGOLITH
dc.type	Статья
dc.identifier.doi	10.1134/S1028334X06030251

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