Petrogenesis of the 1.85 Ga Sonakhan mafic dyke swarm, Bastar Craton, India

J. G. Shellnutt, K. R. Hari, A. C.Y. Liao, S. W. Denyszyn, N. Vishwakarma, S. D. Deshmukh

研究成果: 雜誌貢獻期刊論文同行評審

9 引文 斯高帕斯(Scopus)


The NNW trending tholeiitic Sonakhan mafic dyke swarm of the Northern Bastar Craton is comprised of basalt to basaltic andesite (SiO 2 = 46.3 wt% to 55.3 wt%; Mg# = 37 to 70) dykes. A single basaltic dyke yielded a weighted-mean 207 Pb/ 206 Pb baddeleyite age of 1851.1 ± 2.6 Ma. The Sr and Nd isotopes ( 87 Sr/ 86 Sr i = 0.70396 to 0.70855; ε Nd (t) = −5.7 to +2.0) are variable which is a consequence of crustal contamination. Trace element modeling suggests the dykes were likely derived by partial melting of a spinel-bearing mantle source. The Sonakhan dykes are 30 million years younger than the 1.88 Ga Bastar-Cuddapah dykes (Bastanar-Hampi swarm) of the southern and central Bastar Craton indicating they represent a distinct period of magmatism. However, much like the 1.88 Ga dykes, the Sonakhan dykes appear to be correlative with dykes from the Yilgarn Craton (Yalgoo dyke = 1854 ± 5 Ma) of Western Australia. The temporal and compositional similarity of the Sonakhan dykes with the Yalgoo dyke is evidence that they are petrologically related and may represent different branches of the same dyke swarm. The existence of two distinct Paleoproterozoic dyke swarms in the Bastar Craton that each have a correlative unit in the Yilgarn Craton is supportive of a link between India and Australia before 1.9 Ga. Moreover, it suggests that the break-up of India and Western Australia was protracted and lasted for at least 30 million years.

頁(從 - 到)88-101
出版狀態已發佈 - 2019 六月 1

ASJC Scopus subject areas

  • 地質學
  • 地球化學與岩石學


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