ORIGIN OF FE-RICH LHERZOLITES AND WEHRLITES FROM TOK, SE SIBERIA BY REACTIVE MELT PERCOLATION IN REFRACTORY MANTLE PERIDOTITES

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dc.contributor.author Ionov D.A.
dc.contributor.author Chanefo I.
dc.contributor.author Bodinier J.L.
dc.date.accessioned 2023-12-03T03:59:59Z
dc.date.available 2023-12-03T03:59:59Z
dc.date.issued 2005
dc.identifier https://www.elibrary.ru/item.asp?id=14744376
dc.identifier.citation Contributions to Mineralogy and Petrology, 2005, 150, 3, 335-353
dc.identifier.issn 0010-7999
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/42128
dc.description.abstract Lherzolite–wehrlite (LW) series xenoliths from the quaternary Tok volcanic field in the southeastern Siberian craton are distinguished from the more common lherzolite–harzburgite (LH) series by (a) low Mg numbers (0.84–0.89) at high modal olivine (66–84%) and (b) widespread replacement of orthopyroxene (0–12%) and spinel by clinopyroxene (7–22%). The LW series peridotites are typically enriched in Ca, Fe, Mn and Ti, and depleted in Si, Ni and Cr relative to refractory LH series rocks (Mg number ≥0.89), which are metasomatised partial melting residues. Numerical modelling of Fe–Mg solid/liquid exchange during melt percolation demonstrates that LW series rocks can form by reaction of host refractory peridotites with evolved (Mg numbers 0.6–0.7), silica-undersaturated silicate melts at high melt/rock ratios, which replace orthopyroxene with clinopyroxene and decrease Mg numbers. This process is most likely related to underplating and fractionation of basaltic magma in the shallow mantle, which also produced olivine–clinopyroxene cumulates found among the Tok xenoliths.
dc.subject Siberia
dc.subject Lithospheric mantle
dc.subject Peridotite
dc.subject Wehrlite
dc.subject Reactive melt percolation
dc.title ORIGIN OF FE-RICH LHERZOLITES AND WEHRLITES FROM TOK, SE SIBERIA BY REACTIVE MELT PERCOLATION IN REFRACTORY MANTLE PERIDOTITES
dc.type Статья
dc.identifier.doi 10.1007/s00410-005-0026-7


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