Tectonic evolution of the Eastern Ghats Belt, India

We present possible tectonic models for two crustal domains of the Proterozoic Eastern Ghats Belt, India based on recent petrological, geophysical and geochronological data. Although both the domains presently expose deep crustal sections, they evolved in two distinct time segments of the Precambrian through accretion–collision processes. This is why we argue that no unique model can explain the complexities of the belt. The southern part of the belt evolved through subduction-dominated accretionary processes encompassing India, east Antarctica, Australia and Laurentia as part of supercontinent Columbia during the span of ca. 1.90–1.60 Ga. To the contrary, the central domain witnessed a prolonged accretion–collision history initiated at ca. 1.50 Ga and culminated at ca. 0.90 Ga with the formation of supercontinent Rodinia. The latter united cratonic India with east Antarctica as a separate continent Enderbia that existed until about ca. 0.50 Ga. The pre-1.50 Ga history of this domain is ambiguous at the present state of knowledge. The northern domain has a much younger (ca. 0.90–0.50 Ga) tectonothermal history which is unrelated to either of the studied domains. The present models explain the reported petrotectonic processes including the ultra high temperature metamorphism in both the domains. The episodic growth of the Eastern Ghats Belt matches with Proterozoic supercontinent cycles.

► Eastern Ghats Belt of India contains distinct crustal domains.
► Tectonic developments of these domains are time-specific.
► We evaluate tectonic histories of two such domains.
► The southern domains evolved during ca. 1.90–1.60 Ga during accretionary orogeny encompassing Columbia.
► The central domain shows ca. 1.50–0.90 Ga accretion–collision history involving Rodinia.