Research output: Contribution to journal › Article › peer-review
A Find of Coesite in Diamond-Bearing Kyanite Eclogite from the Udachnaya Kimberlite Pipe, Siberian Craton. / Mikhailenko, D. S.; Korsakov, A. V.; Rezvukhina, O. V. et al.
In: Doklady Earth Sciences, Vol. 487, No. 2, 01.08.2019, p. 925-928.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - A Find of Coesite in Diamond-Bearing Kyanite Eclogite from the Udachnaya Kimberlite Pipe, Siberian Craton
AU - Mikhailenko, D. S.
AU - Korsakov, A. V.
AU - Rezvukhina, O. V.
AU - Golovin, A. V.
AU - Sobolev, N. V.
N1 - Publisher Copyright: © 2019, Pleiades Publishing, Ltd. Copyright: Copyright 2019 Elsevier B.V., All rights reserved.
PY - 2019/8/1
Y1 - 2019/8/1
N2 - Abstract: A find of coesite in a kyanite graphite–diamond-bearing eclogite xenolith from the Udachnaya–Vostochnaya kimberlite pipe is described in this paper. The coesite relics were found in intensely fractured garnet indicating some influence of the kimberlite melt, which is supported by the typical secondary mineral assemblage around this inclusion. These data indicate that shallower diamond-free coesite-grade rocks (2.7 GPa) underwent metamorphism distinct from diamond-bearing coesite eclogites (≥4 GPa). The metasomatic alteration of rock as a result of the C–O–H fluid-rock interaction during diamond crystallization may be another possible reason for the absence of coesite in diamond-bearing xenoliths.
AB - Abstract: A find of coesite in a kyanite graphite–diamond-bearing eclogite xenolith from the Udachnaya–Vostochnaya kimberlite pipe is described in this paper. The coesite relics were found in intensely fractured garnet indicating some influence of the kimberlite melt, which is supported by the typical secondary mineral assemblage around this inclusion. These data indicate that shallower diamond-free coesite-grade rocks (2.7 GPa) underwent metamorphism distinct from diamond-bearing coesite eclogites (≥4 GPa). The metasomatic alteration of rock as a result of the C–O–H fluid-rock interaction during diamond crystallization may be another possible reason for the absence of coesite in diamond-bearing xenoliths.
KW - XENOLITH
KW - GARNET
UR - http://www.scopus.com/inward/record.url?scp=85073075408&partnerID=8YFLogxK
U2 - 10.1134/S1028334X19080087
DO - 10.1134/S1028334X19080087
M3 - Article
AN - SCOPUS:85073075408
VL - 487
SP - 925
EP - 928
JO - Doklady Earth Sciences
JF - Doklady Earth Sciences
SN - 1028-334X
IS - 2
ER -
ID: 21856163