In situ LA-ICPMS Isotopic and Geochronological Studies on Carbonatites and Phoscorites from the Guli Massif, Maymecha-Kotuy, Polar Siberia
- Authors: Ghobadi M.1,2, Gerdes A.2, Kogarko L.3, Hoefer H.2, Brey G.2
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Affiliations:
- Activation Laboratories, Ltd., Ancaster
- Institute of Geoscience
- Vernadsky Institute of Geochemistry and Analytical Chemistry
- Issue: Vol 56, No 8 (2018)
- Pages: 766-783
- Section: Article
- URL: https://journals.rcsi.science/0016-7029/article/view/156014
- DOI: https://doi.org/10.1134/S0016702918080049
- ID: 156014
Cite item
Abstract
In this study we present a fresh isotopic data, as well as U–Pb ages from different REE-minerals in carbonatites and phoscorites of Guli massif using in situ LA-ICPMS technique. The analyses were conducted on apatites and perovskites from calcio-carbonatite and phoscorite units, as well as on pyrochlores and baddeleyites from the carbonatites. The 87Sr/86Sr ratios obtained from apatites and perovskites from the phoscorites are 0.70308–0.70314 and 0.70306–0.70313, respectively; and 0.70310–0.70325 and 0.70314–0.70327, for the pyrochlores and apatites from the carbonatites, respectively.
Furthermore, the in situ laser ablation analyses of apatites and perovskites from the phoscorite yield εNd from 3.6 (±1) to 5.1 (±0.5) and from 3.8 (±0.5) to 4.9 (±0.5), respectively; εNd of apatites, perovskites and pyrochlores from carbonatite ranges from 3.2 (±0.7) to 4.9 (±0.9), 3.9 (±0.6) to 4.5 (±0.8) and 3.2 (±0.4) to 4.4 (±0.8), respectively. Laser ablation analyses of baddeleyites yielded an eHf(t)d of +8.5 (± 0.18); prior to this study Hf isotopic characteristic of Guli massif was not known. Our new in situ εNd, 87Sr/86Sr and eHf data on minerals in the Guli carbonatites imply a depleted source with a long time integrated high Lu/Hf, Sm/Nd, Sr/Rb ratios.
In situ U–Pb age determination was performed on perovskites from the carbonatites and phoscorites and also on pyrochlores and baddeleyites from carbonatites. The co-existing pyrochlores, perovskites and baddeleyites in carbonatites yielded ages of 252.3 ± 1.9, 252.5 ± 1.5 and 250.8 ± 1.4 Ma, respectively. The perovskites from the phoscorites yielded an age of 253.8 ± 1.9 Ma. The obtained age for Guli carbonatites and phoscorites lies within the range of ages previously reported for the Siberian Flood Basalts and suggest essentially synchronous emplacement with the Permian-Triassic boundary.
About the authors
Mahdi Ghobadi
Activation Laboratories, Ltd., Ancaster; Institute of Geoscience
Email: Kogarko@geokhi.ru
Canada, Ontario; Frankfurt am Main
Axel Gerdes
Institute of Geoscience
Email: Kogarko@geokhi.ru
Germany, Frankfurt am Main
Lia Kogarko
Vernadsky Institute of Geochemistry and Analytical Chemistry
Author for correspondence.
Email: Kogarko@geokhi.ru
Russian Federation, Moscow
Heidi Hoefer
Institute of Geoscience
Email: Kogarko@geokhi.ru
Germany, Frankfurt am Main
Gerhard Brey
Institute of Geoscience
Email: Kogarko@geokhi.ru
Germany, Frankfurt am Main
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