Research output: Contribution to journal › Article › peer-review
Conditions of Formation of Layered Intrusions of the Monchegorsk Magmatic Cluster. / Semenov, V. S.; Kazanov, O. V.; Korneev, S. I.; Salnikova, E. B.; Semenov, S. V.
In: Petrology, Vol. 30, No. 4, 24.07.2022, p. 369-391.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Conditions of Formation of Layered Intrusions of the Monchegorsk Magmatic Cluster
AU - Semenov, V. S.
AU - Kazanov, O. V.
AU - Korneev, S. I.
AU - Salnikova, E. B.
AU - Semenov, S. V.
N1 - Publisher Copyright: © 2022, Pleiades Publishing, Ltd.
PY - 2022/7/24
Y1 - 2022/7/24
N2 - The paper presents geochronological data and results of petrological modeling of the Monchegorsk and Monchetundra layered massifs. The U-Pb ID-TIMS zircon dating of norite from the marginal zone of Mt. Nittis yielded 2506 ± 7 Ma, which coincides with previous data on similar rocks from other areas. Based on the comparison of sections of the Monchegorsk and Kivakka massifs, the pre-erosion thickness of the Monchegorsk massif is estimated as 3700 m. Calculations using rocks of the marginal zone of the Monchegorsk intrusion at a pressure of 6.5–5.5 kbar showed that the melt in equilibrium with Ol contained SiO2 ≤ 55 wt %, TiO2 ≤ 0.50 wt %, and MgO ≤14 wt %. The temperature of the primary magma could be equal to 1390°C. At a lower pressure (below 6.5 kbar), the obtained melt becomes more siliceous. In the Monchegorsk intrusion, the composition of intratelluric olivine according to this model could vary within 88–92 mol % Fo. The content of intratelluric olivine in the melt, depending on pressure, could vary from 11 to 24 vol %. Magmas that formed the Monchegorsk intrusion and the layered series of the Monchetundra intrusion (hole 742) were derived from different sources.
AB - The paper presents geochronological data and results of petrological modeling of the Monchegorsk and Monchetundra layered massifs. The U-Pb ID-TIMS zircon dating of norite from the marginal zone of Mt. Nittis yielded 2506 ± 7 Ma, which coincides with previous data on similar rocks from other areas. Based on the comparison of sections of the Monchegorsk and Kivakka massifs, the pre-erosion thickness of the Monchegorsk massif is estimated as 3700 m. Calculations using rocks of the marginal zone of the Monchegorsk intrusion at a pressure of 6.5–5.5 kbar showed that the melt in equilibrium with Ol contained SiO2 ≤ 55 wt %, TiO2 ≤ 0.50 wt %, and MgO ≤14 wt %. The temperature of the primary magma could be equal to 1390°C. At a lower pressure (below 6.5 kbar), the obtained melt becomes more siliceous. In the Monchegorsk intrusion, the composition of intratelluric olivine according to this model could vary within 88–92 mol % Fo. The content of intratelluric olivine in the melt, depending on pressure, could vary from 11 to 24 vol %. Magmas that formed the Monchegorsk intrusion and the layered series of the Monchetundra intrusion (hole 742) were derived from different sources.
KW - cumulates
KW - geochronological age
KW - magma
KW - melt
KW - micrograined rocks
KW - Monchegorsk and Monchetundra layered massifs
KW - Monchegorsk and Monchetundra layered massifs, cumulates, geochronological age, micrograined rocks, melt, magma
UR - http://www.scopus.com/inward/record.url?scp=85134624416&partnerID=8YFLogxK
UR - https://www.mendeley.com/catalogue/07b99c6e-da80-3784-b9c3-40558b4c9626/
U2 - 10.1134/s0869591122030079
DO - 10.1134/s0869591122030079
M3 - Article
AN - SCOPUS:85134624416
VL - 30
SP - 369
EP - 391
JO - Petrology
JF - Petrology
SN - 0869-5911
IS - 4
ER -
ID: 98218344