Petrology, U-Pb titanite dating and Sr-Nd isotope geochemistry of a shoshonitic lamprophyre dyke near the Western Dharwar Craton-Southern Granulite Terrane contact, southern India: Implications for long-lived enriched mantle, widespread Tonian-Cryogenian rifting, and Rodinia configuration

被引:0
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作者
Raghuvanshi, Sneha [1 ]
Rao, N. V. Chalapathi [1 ]
Talukdar, D. [1 ,2 ]
Belyatsky, B. [3 ]
Prabhat, P. [4 ]
Rahaman, Waliur [4 ]
Lehmann, B. [5 ]
Meert, J. G. [6 ]
机构
[1] Banaras Hindu Univ, Inst Sci, Dept Geol, Mantle Petrol Lab, Varanasi 221005, India
[2] Geol Survey India, HR SIMS lab, 40 Dharitri Bldg,Sect V,Salt Lake, Kolkata 700091, Haryana, India
[3] Russian Acad Sci, Karpinsky Geol Inst VSEGEI, St Petersburg 199034, Russia
[4] Natl Ctr Polar & Ocean Res, Minist Earth Sci, Headland Sada, Mormugao 403804, Goa, India
[5] Tech Univ Clausthal, Mineral Resources, Adolph Roemer Str 2A, D-38678 Clausthal Zellerfeld, Germany
[6] Univ Florida, Dept Geol Sci, Gainesville, FL USA
关键词
Neoproterozoic lamprophyre; U -Pb SHRIMP dating; Western Dharwar Craton; India; Rodinia; CALC-ALKALINE LAMPROPHYRES; WAJRAKARUR KIMBERLITE FIELD; TAMIL-NADU; LITHOSPHERIC MANTLE; ZR/HF FRACTIONATION; CRUSTAL EVOLUTION; TRACE-ELEMENTS; CARBONATITE METASOMATISM; ZIRCON GEOCHRONOLOGY; POLYGENETIC TITANITE;
D O I
10.1016/j.precamres.2023.107241
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We present petrology, U-Pb titanite geochronology, bulk-rock and Sr-Nd geochemistry of an undeformed and unmetamorphosed shoshonitic lamprophyre (spessartite) from the Mysuru area (Halaguru-Harohalli alkaline province) located approximately 80 km north of the tectonic contact between the Western Dharwar Craton and the Southern Granulite Terrane, southern India, to understand its origin and to evaluate its geodynamic sig-nificance. The lamprophyre shows a typical porphyritic-panidiomorphic texture with amphibole phenocrysts. Clinopyroxene occurs only as xenocrysts with feldspar, apatite, titanite and titano-magnetite confined to the groundmass. Amphibole mineral composition classifies them as pargasite and tremolite, and the groundmass is essentially constituted of alkali feldspar. High whole-rock Mg# (56-65), Ni + Cr (245 to 730 ppm), a lack of correlation between SiO2 and Rb/Sr as well as epsilon Nd(i) indicates that crustal contamination experienced by the lamprophyre magma is limited. U-Pb titanite (n = 18) SHRIMP-II dating yielded a Neoproterozoic Tera-Wasserburg concordia age of 820 +/- 15 Ma (MSWD = 5.9). Whole-rock derived 87Sr/86Sr(i) (0.70425-0.70530) and epsilon Nd(i) (-6.3 to-4.3) suggest origin of the lamprophyre from an enriched lithospheric mantle source. Pale-oproterozoic depleted-mantle model ages of ca. 1.8 Ga suggest the existence of a long-lived enriched mantle which correspond to the timing (ca.1.9-1.7 Ga) of widespread mafic dyke swarms' emplacement in the Dharmapuri-Agali-Tiruvannamalai domain in the Salem block at the northernmost portion of the Southern Granulite Terrane. The Tonian emplacement age of the studied lamprophyre is synchronous with several co-spatial Neoproterozoic (i) alkaline complexes +/- carbonatite +/- lamprophyre from the northern part of the Southern Granulite Terrane, and (ii) other mafic alkaline dykes of the Halaguru-Harohalli alkaline province from the southern part of the Eastern Dharwar Craton. Our results highlight the importance of this lamprophyre dyke, present close to the'Fermor Line' as well as near the boundary between Eastern and Western Dharwar Cratons, which provides a rare opportunity to understand its spatio-temporal link with alkaline dykes of the Southern Granulite Terrain. Our findings also help understand the role of repeated large-scale rifting, associated with the Rodinia break-up, leading to the generation of a wide spectrum of Tonian-Cryogenian alkaline magmas in southern Indian Shield. The new age data also have implications for the configuration of India's paleoposition during the Neoproterozoic and support the idea that South China Block-India were located on the periphery of Rodinia or were already detached from the supercontinent.
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