REFINEMENT OF THE MANGAN-NEPTUNITE CRYSTAL STRUCTURE

dc.contributor.authorZolotarev Jr.A.A.
dc.contributor.authorKrivovichev S.V.
dc.contributor.authorYakovenchuk V.N.
dc.date.accessioned2026-10-19T05:21:34Z
dc.date.issued2007
dc.description.abstractThe crystal structure of mangan-neptunite, a manganese analogue of neptunite, has been refined in two space groups (Cc and C2/c). The mineral is monoclinic, with the correct space group Cc; the unit-cell dimensions are: a = 16.4821(6), b = 12.5195(4), c = 10.0292(3) Å, β = 115.474(1)°, and V = 1868.31 Å3. The crystal structure has been refined to R 1 = 0.0307 (wR 2 = 0.0901) on the basis of 4892 observed reflections with |F hkl | ≥ 4σ|F hkl |. The most plausible acentric model is caused by the Ti- and (Fe, Mn, Mg)-ordering in the structure. Ti-octahedrons are strongly distorted and consist of short bond Ti-O (1.7 Å), one long bond (2.2 Å), and four equal bonds (2.0 Å). Fe-octahedrons are regularly shaped, with all Fe-O bonds being approximately identical.
dc.identifierhttps://elibrary.ru/item.asp?id=13551781
dc.identifier.citationGeology of Ore Deposits, 2007, 49, 8, 835-838
dc.identifier.doi10.1134/S1075701507080181
dc.identifier.issn1075-7015
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/55081
dc.titleREFINEMENT OF THE MANGAN-NEPTUNITE CRYSTAL STRUCTURE
dc.typeСтатья

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