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Interaction of peridotite with Ca-rich carbonatite melt at 3.1 and 6.5 GPa : Implication for merwinite formation in upper mantle, and for the metasomatic origin of sublithospheric diamonds with Ca-rich suite of inclusions. / Sharygin, Igor S.; Shatskiy, Anton; Litasov, Konstantin D. et al.

In: Contributions to Mineralogy and Petrology, Vol. 173, No. 3, 22, 01.03.2018.

Research output: Contribution to journal › Article › peer-review

Harvard

Sharygin, IS, Shatskiy, A, Litasov, KD, Golovin, AV, Ohtani, E & Pokhilenko, NP 2018, 'Interaction of peridotite with Ca-rich carbonatite melt at 3.1 and 6.5 GPa: Implication for merwinite formation in upper mantle, and for the metasomatic origin of sublithospheric diamonds with Ca-rich suite of inclusions', Contributions to Mineralogy and Petrology, vol. 173, no. 3, 22. https://doi.org/10.1007/s00410-017-1432-3

APA

Sharygin, I. S., Shatskiy, A., Litasov, K. D., Golovin, A. V., Ohtani, E., & Pokhilenko, N. P. (2018). Interaction of peridotite with Ca-rich carbonatite melt at 3.1 and 6.5 GPa: Implication for merwinite formation in upper mantle, and for the metasomatic origin of sublithospheric diamonds with Ca-rich suite of inclusions. Contributions to Mineralogy and Petrology, 173(3), [22]. https://doi.org/10.1007/s00410-017-1432-3

Vancouver

Sharygin IS, Shatskiy A, Litasov KD, Golovin AV, Ohtani E, Pokhilenko NP. Interaction of peridotite with Ca-rich carbonatite melt at 3.1 and 6.5 GPa: Implication for merwinite formation in upper mantle, and for the metasomatic origin of sublithospheric diamonds with Ca-rich suite of inclusions. Contributions to Mineralogy and Petrology. 2018 Mar 1;173(3):22. doi: 10.1007/s00410-017-1432-3

Author

Sharygin, Igor S. ; Shatskiy, Anton ; Litasov, Konstantin D. et al. / Interaction of peridotite with Ca-rich carbonatite melt at 3.1 and 6.5 GPa : Implication for merwinite formation in upper mantle, and for the metasomatic origin of sublithospheric diamonds with Ca-rich suite of inclusions. In: Contributions to Mineralogy and Petrology. 2018 ; Vol. 173, No. 3.

BibTeX

@article{33fa3de458064e008749ca1f698cf670,
title = "Interaction of peridotite with Ca-rich carbonatite melt at 3.1 and 6.5 GPa: Implication for merwinite formation in upper mantle, and for the metasomatic origin of sublithospheric diamonds with Ca-rich suite of inclusions",
abstract = "We performed an experimental study, designed to reproduce the formation of an unusual merwinite + olivine-bearing mantle assemblage recently described as a part of a Ca-rich suite of inclusions in sublithospheric diamonds, through the interaction of peridotite with an alkali-rich Ca-carbonatite melt, derived from deeply subducted oceanic crust. In the first set of experiments, we studied the reaction between powdered Mg-silicates, olivine and orthopyroxene, and a model Ca-carbonate melt (molar Na:K:Ca = 1:1:2), in a homogeneous mixture, at 3.1 and 6.5 GPa. In these equilibration experiments, we observed the formation of a merwinite + olivine-bearing assemblage at 3.1 GPa and 1200 °C and at 6.5 GPa and 1300–1400 °C. The melts coexisting with this assemblage have a low Si and high Ca content (Ca# = molar 100 × Ca/(Ca + Mg) > 0.57). In the second set of experiments, we investigated reaction rims produced by interaction of the same Ca-carbonate melt (molar Na:K:Ca = 1:1:2) with Mg-silicate, olivine and orthopyroxene, single crystals at 3.1 GPa and 1300 °C and at 6.5 GPa and 1400 °C. The interaction of the Ca-carbonate melt with olivine leads to merwinite formation through the expected reaction: 2Mg2SiO4 (olivine) + 6CaCO3 (liquid) = Ca3MgSi2O8 (merwinite) + 3CaMg(CO3)2 (liquid). Thus, our experiments confirm the idea that merwinite in the upper mantle may originate via interaction of peridotite with Ca-rich carbonatite melt, and that diamonds hosting merwinite may have a metasomatic origin. It is remarkable that the interaction of the Ca-carbonate melt with orthopyroxene crystals does not produce merwinite both at 3.1 and 6.5 GPa. This indicates that olivine grain boundaries are preferable for merwinite formation in the upper mantle.",
keywords = "Carbonatite melt, Diamond, Mantle, Merwinite, Subduction, HIGH-PRESSURE, UDACHNAYA-EAST KIMBERLITE, DEEP MANTLE, ECLOGITE, EARTHS INTERIOR, CONTINENTAL LITHOSPHERIC MANTLE, TRANSPORT, EXTRACTION, TRANSITION ZONE, PHASE-RELATIONS",
author = "Sharygin, {Igor S.} and Anton Shatskiy and Litasov, {Konstantin D.} and Golovin, {Alexander V.} and Eiji Ohtani and Pokhilenko, {Nikolay P.}",
year = "2018",
month = mar,
day = "1",
doi = "10.1007/s00410-017-1432-3",
language = "English",
volume = "173",
journal = "Contributions to Mineralogy and Petrology",
issn = "0010-7999",
publisher = "Springer Nature",
number = "3",

}

RIS

TY - JOUR

T1 - Interaction of peridotite with Ca-rich carbonatite melt at 3.1 and 6.5 GPa

T2 - Implication for merwinite formation in upper mantle, and for the metasomatic origin of sublithospheric diamonds with Ca-rich suite of inclusions

AU - Sharygin, Igor S.

AU - Shatskiy, Anton

AU - Litasov, Konstantin D.

AU - Golovin, Alexander V.

AU - Ohtani, Eiji

AU - Pokhilenko, Nikolay P.

PY - 2018/3/1

Y1 - 2018/3/1

N2 - We performed an experimental study, designed to reproduce the formation of an unusual merwinite + olivine-bearing mantle assemblage recently described as a part of a Ca-rich suite of inclusions in sublithospheric diamonds, through the interaction of peridotite with an alkali-rich Ca-carbonatite melt, derived from deeply subducted oceanic crust. In the first set of experiments, we studied the reaction between powdered Mg-silicates, olivine and orthopyroxene, and a model Ca-carbonate melt (molar Na:K:Ca = 1:1:2), in a homogeneous mixture, at 3.1 and 6.5 GPa. In these equilibration experiments, we observed the formation of a merwinite + olivine-bearing assemblage at 3.1 GPa and 1200 °C and at 6.5 GPa and 1300–1400 °C. The melts coexisting with this assemblage have a low Si and high Ca content (Ca# = molar 100 × Ca/(Ca + Mg) > 0.57). In the second set of experiments, we investigated reaction rims produced by interaction of the same Ca-carbonate melt (molar Na:K:Ca = 1:1:2) with Mg-silicate, olivine and orthopyroxene, single crystals at 3.1 GPa and 1300 °C and at 6.5 GPa and 1400 °C. The interaction of the Ca-carbonate melt with olivine leads to merwinite formation through the expected reaction: 2Mg2SiO4 (olivine) + 6CaCO3 (liquid) = Ca3MgSi2O8 (merwinite) + 3CaMg(CO3)2 (liquid). Thus, our experiments confirm the idea that merwinite in the upper mantle may originate via interaction of peridotite with Ca-rich carbonatite melt, and that diamonds hosting merwinite may have a metasomatic origin. It is remarkable that the interaction of the Ca-carbonate melt with orthopyroxene crystals does not produce merwinite both at 3.1 and 6.5 GPa. This indicates that olivine grain boundaries are preferable for merwinite formation in the upper mantle.

AB - We performed an experimental study, designed to reproduce the formation of an unusual merwinite + olivine-bearing mantle assemblage recently described as a part of a Ca-rich suite of inclusions in sublithospheric diamonds, through the interaction of peridotite with an alkali-rich Ca-carbonatite melt, derived from deeply subducted oceanic crust. In the first set of experiments, we studied the reaction between powdered Mg-silicates, olivine and orthopyroxene, and a model Ca-carbonate melt (molar Na:K:Ca = 1:1:2), in a homogeneous mixture, at 3.1 and 6.5 GPa. In these equilibration experiments, we observed the formation of a merwinite + olivine-bearing assemblage at 3.1 GPa and 1200 °C and at 6.5 GPa and 1300–1400 °C. The melts coexisting with this assemblage have a low Si and high Ca content (Ca# = molar 100 × Ca/(Ca + Mg) > 0.57). In the second set of experiments, we investigated reaction rims produced by interaction of the same Ca-carbonate melt (molar Na:K:Ca = 1:1:2) with Mg-silicate, olivine and orthopyroxene, single crystals at 3.1 GPa and 1300 °C and at 6.5 GPa and 1400 °C. The interaction of the Ca-carbonate melt with olivine leads to merwinite formation through the expected reaction: 2Mg2SiO4 (olivine) + 6CaCO3 (liquid) = Ca3MgSi2O8 (merwinite) + 3CaMg(CO3)2 (liquid). Thus, our experiments confirm the idea that merwinite in the upper mantle may originate via interaction of peridotite with Ca-rich carbonatite melt, and that diamonds hosting merwinite may have a metasomatic origin. It is remarkable that the interaction of the Ca-carbonate melt with orthopyroxene crystals does not produce merwinite both at 3.1 and 6.5 GPa. This indicates that olivine grain boundaries are preferable for merwinite formation in the upper mantle.

KW - Carbonatite melt

KW - Diamond

KW - Mantle

KW - Merwinite

KW - Subduction

KW - HIGH-PRESSURE

KW - UDACHNAYA-EAST KIMBERLITE

KW - DEEP MANTLE

KW - ECLOGITE

KW - EARTHS INTERIOR

KW - CONTINENTAL LITHOSPHERIC MANTLE

KW - TRANSPORT

KW - EXTRACTION

KW - TRANSITION ZONE

KW - PHASE-RELATIONS

UR - http://www.scopus.com/inward/record.url?scp=85042443458&partnerID=8YFLogxK

U2 - 10.1007/s00410-017-1432-3

DO - 10.1007/s00410-017-1432-3

M3 - Article

AN - SCOPUS:85042443458

VL - 173

JO - Contributions to Mineralogy and Petrology

JF - Contributions to Mineralogy and Petrology

SN - 0010-7999

IS - 3

M1 - 22

ER -

ID: 10422101