THE SOLIDUS OF CARBONATED, FERTILE PERIDOTITE

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dc.contributor.author Falloon T.J.
dc.contributor.author Green D.H.
dc.date.accessioned 2020-10-12T05:35:07Z
dc.date.available 2020-10-12T05:35:07Z
dc.date.issued 1989
dc.identifier https://elibrary.ru/item.asp?id=31462969
dc.identifier.citation Earth and Planetary Science Letters, 1989, , 3, 364-370
dc.identifier.issn 0012-821X
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/18020
dc.description.abstract The solidus for a fertile peridotite composition (“Hawaiian pyrolite”) in the presence of CO2 has been determined from 14 to 35 kbar. The solidus shape inP-T space is consistent with previous studies in the model system CaO—MgO—SiO2—CO2. The intersection of the decarbonation reaction Olivine + Diopside + CO2 ⇌ Orthopyroxene + Dolomite with the pyrolite solidus defines the pointI6, which is located at 20.5 kbar, 1050°C. At pressures less thanI6 the solidus is only slightly (20–50°C) below that of the volatile-absent (C—H absent) solidus but at pressures greater thanI6 the solidus curve is approximately 275°C below the volatile-absent solidus. The large depression of the solidus to lower temperatures with little change in pressure occurs at approximately 19 kbar, 1250°C. At 26 kbar the Hawaiian pyrolite-CO2 solidus is approximately 100°C higher than the solidus for Hawaiian pyrolite-H2O—CO2 confirming that the primary sodic dolomitic carbonatite melt at the latter solidus does contain some dissolved water.
dc.title THE SOLIDUS OF CARBONATED, FERTILE PERIDOTITE
dc.type Статья
dc.identifier.doi 10.1016/0012-821X(89)90153-2


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