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Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes. / Karputin, I. S.; Agashev, Aleksey M.; Agasheva, E. V. et al.

In: Doklady Earth Sciences, Vol. 522, No. 1, 16, 15.04.2025.

Research output: Contribution to journalArticlepeer-review

Harvard

Karputin, IS, Agashev, AM, Agasheva, EV, Serov, IV & Pokhilenko, NP 2025, 'Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes', Doklady Earth Sciences, vol. 522, no. 1, 16. https://doi.org/10.1134/S1028334X24605868

APA

Karputin, I. S., Agashev, A. M., Agasheva, E. V., Serov, I. V., & Pokhilenko, N. P. (2025). Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes. Doklady Earth Sciences, 522(1), [16]. https://doi.org/10.1134/S1028334X24605868

Vancouver

Karputin IS, Agashev AM, Agasheva EV, Serov IV, Pokhilenko NP. Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes. Doklady Earth Sciences. 2025 Apr 15;522(1):16. doi: 10.1134/S1028334X24605868

Author

Karputin, I. S. ; Agashev, Aleksey M. ; Agasheva, E. V. et al. / Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes. In: Doklady Earth Sciences. 2025 ; Vol. 522, No. 1.

BibTeX

@article{7ceb7d0b65e94b8fbc0ba9c1f5100eb2,
title = "Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes",
abstract = "Abstract: The results of study of the chemical composition of “depleted” garnets from xenoliths of lherzolites from the Mir and V. Grib highly diamondiferous kimberlite pipes are presented. The garnets from the xenoliths of the Mir pipe are characterized by a relatively large size (3–15 mm) and a hook-shaped or elongated grain morphology. The garnets from the V. Grib pipe are rounder, and their size ranges from 1 to 4 mm. Based on the content of CaO and Cr2O3, the garnets belong to the lherzolite paragenesis. The garnets of the studied xenoliths have low contents of incompatible elements and are characterized by fractionated rare earth element (REE) patterns with a strong decrease from heavy to light REEs (LREEs). The LREE contents are ten or more times lower in comparison with chondrite. The Y and Zr contents form a trend from “depleted” peridotites to “metasomatized” lherzolites, which can be observed in both within a single xenolith and within a single grain. In contrast to metasomatized garnets with an increasing from core to rim Y and Zr content, the peripheral parts of the depleted garnets are depleted in Y, Zr, Ti, and LREEs in comparison with the central parts. These peculiarities of the chemical composition and morphology of garnets indicate their restite origin as a result of partial melting. It is shown for the first time that the upper horizons of the lithospheric mantle preserve restite lherzolites, the garnets in which were unaffected by metasomatic processes.",
keywords = "kimberlite pipe, lherzolite, lithospheric mantle, mantle metasomatism, pyrope, rare earth elements",
author = "Karputin, {I. S.} and Agashev, {Aleksey M.} and Agasheva, {E. V.} and Serov, {I. V.} and Pokhilenko, {N. P.}",
note = "All analytical works were supported by the Russian Science Foundation, project no. 20-77-10018. Sampling of xenoliths was supported by state contract no. 122041400157-9 of the Institute of Geology and Mineralogy, Siberian Branch, Russian Academy of Sciences (Novosibirsk, Russia). Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes / I. S. Karputin, A. M. Agashev, E. V. Agasheva [et al.] // Doklady Earth Sciences. – 2025. – Vol. 522, No. 1. – P. 1-7. – DOI 10.1134/S1028334X24605868.",
year = "2025",
month = apr,
day = "15",
doi = "10.1134/S1028334X24605868",
language = "English",
volume = "522",
journal = "Doklady Earth Sciences",
issn = "1028-334X",
publisher = "Pleiades Publishing",
number = "1",

}

RIS

TY - JOUR

T1 - Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes

AU - Karputin, I. S.

AU - Agashev, Aleksey M.

AU - Agasheva, E. V.

AU - Serov, I. V.

AU - Pokhilenko, N. P.

N1 - All analytical works were supported by the Russian Science Foundation, project no. 20-77-10018. Sampling of xenoliths was supported by state contract no. 122041400157-9 of the Institute of Geology and Mineralogy, Siberian Branch, Russian Academy of Sciences (Novosibirsk, Russia). Residual Origin of Garnets and Their Host Lherzolites from the Mir and V. Grib Kimberlite Pipes / I. S. Karputin, A. M. Agashev, E. V. Agasheva [et al.] // Doklady Earth Sciences. – 2025. – Vol. 522, No. 1. – P. 1-7. – DOI 10.1134/S1028334X24605868.

PY - 2025/4/15

Y1 - 2025/4/15

N2 - Abstract: The results of study of the chemical composition of “depleted” garnets from xenoliths of lherzolites from the Mir and V. Grib highly diamondiferous kimberlite pipes are presented. The garnets from the xenoliths of the Mir pipe are characterized by a relatively large size (3–15 mm) and a hook-shaped or elongated grain morphology. The garnets from the V. Grib pipe are rounder, and their size ranges from 1 to 4 mm. Based on the content of CaO and Cr2O3, the garnets belong to the lherzolite paragenesis. The garnets of the studied xenoliths have low contents of incompatible elements and are characterized by fractionated rare earth element (REE) patterns with a strong decrease from heavy to light REEs (LREEs). The LREE contents are ten or more times lower in comparison with chondrite. The Y and Zr contents form a trend from “depleted” peridotites to “metasomatized” lherzolites, which can be observed in both within a single xenolith and within a single grain. In contrast to metasomatized garnets with an increasing from core to rim Y and Zr content, the peripheral parts of the depleted garnets are depleted in Y, Zr, Ti, and LREEs in comparison with the central parts. These peculiarities of the chemical composition and morphology of garnets indicate their restite origin as a result of partial melting. It is shown for the first time that the upper horizons of the lithospheric mantle preserve restite lherzolites, the garnets in which were unaffected by metasomatic processes.

AB - Abstract: The results of study of the chemical composition of “depleted” garnets from xenoliths of lherzolites from the Mir and V. Grib highly diamondiferous kimberlite pipes are presented. The garnets from the xenoliths of the Mir pipe are characterized by a relatively large size (3–15 mm) and a hook-shaped or elongated grain morphology. The garnets from the V. Grib pipe are rounder, and their size ranges from 1 to 4 mm. Based on the content of CaO and Cr2O3, the garnets belong to the lherzolite paragenesis. The garnets of the studied xenoliths have low contents of incompatible elements and are characterized by fractionated rare earth element (REE) patterns with a strong decrease from heavy to light REEs (LREEs). The LREE contents are ten or more times lower in comparison with chondrite. The Y and Zr contents form a trend from “depleted” peridotites to “metasomatized” lherzolites, which can be observed in both within a single xenolith and within a single grain. In contrast to metasomatized garnets with an increasing from core to rim Y and Zr content, the peripheral parts of the depleted garnets are depleted in Y, Zr, Ti, and LREEs in comparison with the central parts. These peculiarities of the chemical composition and morphology of garnets indicate their restite origin as a result of partial melting. It is shown for the first time that the upper horizons of the lithospheric mantle preserve restite lherzolites, the garnets in which were unaffected by metasomatic processes.

KW - kimberlite pipe

KW - lherzolite

KW - lithospheric mantle

KW - mantle metasomatism

KW - pyrope

KW - rare earth elements

UR - https://www.mendeley.com/catalogue/0f2b00b8-92d6-3842-8e73-b36483fe5ef7/

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-105005160926&origin=inward&txGid=e9d0fc19d1d7a8e6bc18f48f58d4678b

UR - https://www.elibrary.ru/item.asp?id=80631705

U2 - 10.1134/S1028334X24605868

DO - 10.1134/S1028334X24605868

M3 - Article

VL - 522

JO - Doklady Earth Sciences

JF - Doklady Earth Sciences

SN - 1028-334X

IS - 1

M1 - 16

ER -

ID: 66751941