An insight to the initiation of Cretaceous sedimentation in Northeast Indian Craton

2020 ◽  
Vol 5 (4) ◽  
pp. 457-471
Author(s):  
Rohini Das ◽  
Apoorve Bhardwaj ◽  
Sampita Das Mitra ◽  
Tapan Pal ◽  
Bashab N. Mahanta
Keyword(s):  
2014 ◽  
Vol 88 (s2) ◽  
pp. 1481-1482 ◽  
Author(s):  
Suman Sahu SHREERAM ◽  
Singh SAHENDRA ◽  
Sankar Satapathy JYOTI
Keyword(s):  

2015 ◽  
Vol 43 (1) ◽  
pp. 207-221 ◽  
Author(s):  
Kaushik Das ◽  
Partha Pratim Chakraborty ◽  
Yasutaka Hayasaka ◽  
Masahiro Kayama ◽  
Subhojit Saha ◽  
...  

2018 ◽  
Vol 127 (3) ◽  
Author(s):  
Shailendra Singh ◽  
Ved P Maurya ◽  
Roshan K Singh ◽  
Shalivahan Srivastava ◽  
Anurag Tripathi ◽  
...  

2014 ◽  
Vol 612-613 ◽  
pp. 128-133 ◽  
Author(s):  
Shalivahan ◽  
Bimalendu B. Bhattacharya ◽  
N.V. Chalapathi Rao ◽  
V.P. Maurya
Keyword(s):  

1987 ◽  
Vol 24 (10) ◽  
pp. 1985-1993 ◽  
Author(s):  
Ajoy K. Baksi ◽  
D. A. Archibald ◽  
S. N. Sarkar ◽  
A. K. Saha

40Ar–39Ar incremental heating studies on mineral separates from three sets of rocks in the Singbhum craton in eastern India have helped unravel the thermochronometric history of the terrane and explain an earlier discrepancy between Sm–Nd (~3800 Ma) and Rb–Sr (~3100 Ma) whole-rock ages for the Older Metamorphic Tonalitic Gneiss (OMTG). High precision plateau ages for hornblende separates from the Older Metamorphic Group of rocks (OMG) suggest that this unit is older than 3300 Ma and that enclaves of both the OMTG and OMG within the batholithic complex cooled to ~500 °C at 3300 ± 15 Ma following engulfment in magma, forming the Singbhum Granite (SG). Results from a biotite separate from the OMTG imply that slow cooling continued to a temperature of ~300 °C at ~3160 Ma. Study of a feldspar separate from the Singbhum Granite, suggests final cooling (uplift?) through the ~150 °C isotherm ~660 Ma ago.We suggest that an earlier Rb–Sr whole-rock age of 3130 ± 85 Ma on the OMTG did not yield the crystallisation age, but rather the time of cooling to strontium retention temperature for the biotite in these rocks. We also demonstrate that for hornblende and mica from Archean rocks, 40Ar–39Ar incremental heating experiments can yield very high precision plateau ages (e.g., ± 2 to ± 5 Ma at 3300 Ma). In practice, however, we suggest this technique can separate events in the early Archean spaced ~30 Ma apart.


2020 ◽  
Vol 157 (2) ◽  
pp. 340-350
Author(s):  
Tanzil Deshmukh ◽  
N. Prabhakar

AbstractThe Central Indian Tectonic Zone demarcates the zone of amalgamation between the North Indian Craton and the South Indian Craton. Presently, the major controversies in the existing tectonic models of the Central Indian Tectonic Zone revolve around the direction of subduction and the precise timing of accretion between the North Indian Craton and the South Indian Craton. A new model for the tectonic evolution of the Central Indian Tectonic Zone is postulated in this contribution, based on recent geological and geophysical evidence, combined with previously documented tectonic configurations. The present study employs the slab break-off hypothesis and subsequent polarity reversal to explain the tectonic processes involved in the evolution of the Central Indian Tectonic Zone. We propose that the subduction initiated (c. 2.5 Ga) in a S-directed system producing island-arc sequences on the South Indian Craton. The southward subduction regime culminated with slab break-off underneath the South Indian Craton between c. 1.65 Ga and 1.55 Ga, which subsequently induced subduction polarity reversal and set the course for N-directed subduction (<1.55 Ga). The final closure along the Central Indian Tectonic Zone is governed by the collisional regime during the Sausar Orogeny (1.0–0.9 Ga).


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