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Sulfur, carbon and oxygen isotopic compositions of Newania carbonatites of India: implications for the mantle source characteristics

Banerjee, A and Satish Kumar, M and Chakrabarti, R (2021) Sulfur, carbon and oxygen isotopic compositions of Newania carbonatites of India: implications for the mantle source characteristics. In: Journal of Mineralogical and Petrological Sciences, 116 (3). pp. 121-128.

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Official URL: https://doi.org/10.2465/jmps.201130e

Abstract

This study presents first report of the sulfur isotopic compositions of carbonatites from the Mesoproterozoic Newania complex of India along with their stable C and O isotope ratios. The δ34SV-CDT (-1.4 to 2o) and �33S (-0.001 to -0.13o) values of these carbonatite samples (n = 7) overlap with the S isotope compositions of Earth's mantle. Additionally, the δ13CV-PDB and δ18OV-SMOW values of these carbonatites also show overlapping compositions to that of Earth's mantle. Based on these mantle-like stable isotopic compositions of carbonatites along with their higher crystallization temperature (~ 600 °C) compared to a hydrothermal fluid (<250 °C), we suggest that the sulfide minerals in these carbonatites were formed under a magmatic condition. The mantle like signatures in the δ34S, δ13C- δ18O, and 87Sr/86 Sr values of these carbonatites rule out possible crustal contamination. Coexistence of the sulfide phase (pyrrhotite) with magnesite in these carbonatites suggests that the sulfide phase has formed early during the crystallization of carbonatite magmas under reducing conditions. Overall restricted variability in the δ34S values of these samples further rules out any isotopic fractionation due to the change in the redox condition of the magma and reflect the isotopic composition of the parental melts of the Newania carbonatite complex. A compilation of δ34S of carbonatites from Newania and other complexes worldwide indicates limited variability in the isotopic composition for carbonatites older than 400 Ma, which broadly overlaps with Earth's asthenospheric mantle composition. This contrasts with the larger variability in δ34S observed in carbonatites younger than 400 Ma. Such observation could suggest an overall lower oxidation state of carbonatite magmas emplaced prior to 400 Ma. © 2021. All Rights Reserved.

Item Type: Journal Article
Publication: Journal of Mineralogical and Petrological Sciences
Publisher: Tohoku University
Additional Information: The copyright for this article belongs to Authors
Department/Centre: Division of Mechanical Sciences > Centre for Earth Sciences
Date Deposited: 28 Nov 2021 09:44
Last Modified: 28 Nov 2021 09:44
URI: http://eprints.iisc.ac.in/id/eprint/69993

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