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Heat flow and crustal thermal structure in the Late Archaean Closepet Granite batholith, south India.

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Title: Heat flow and crustal thermal structure in the Late Archaean Closepet Granite batholith, south India.
Authors: Roy, Sukanta1 (AUTHOR) sukantaroy@yahoo.com, Ray, Labani1 (AUTHOR) labani_ngri@rediffmail.com, Bhattacharya, Anurup1 (AUTHOR) srinivasanmalathi@rediffmail.com, R., Srinivasan1 (AUTHOR)
Source: International Journal of Earth Sciences. Apr2008, Vol. 97 Issue 2, p245-256. 12p. 3 Black and White Photographs, 2 Charts, 1 Graph.
Abstract: The Late Archaean Closepet Granite batholith in south India is exposed at different crustal levels grading from greenschist facies in the north through amphibolite and granulite facies in the south along a ~ 400 km long segment in the Dharwar craton. Two areas, Pavagada and Magadi, located in the Main Mass of the batholith, best represent the granitoid of the greenschist and amphibolite facies crustal levels respectively. Heat flow estimates of 38 mW m–2 from Pavagada and 25 mW m–2 from Magadi have been obtained through measurements in deep (430 and 445 m) and carefully sited boreholes. Measurements made in four boreholes of opportunity in Pavagada area yield a mean heat flow of 39 ± 4 (s.d.) mW m–2, which is in good agreement with the estimate from deep borehole. The study, therefore, demonstrates a clear-cut heat flow variation concomitant with the crustal levels exposed in the two areas. The mean heat production estimates for the greenschist facies and amphibolite facies layers constituting the Main Mass of the batholith are 2.9 and 1.8 lWm–3, respectively. The enhanced heat flow in the Pavagada area is consistent with the occurrence of a radioelement-enriched 2-km-thick greenschist facies layer granitoid overlying the granitoid of the amphibolite facies layer which is twice as thick as represented in the Magadi area. The crustal heat production models indicate similar mantle heat flow estimates in the range 12–14 mW m–2, consistent with the other parts of the greenstone-granite-gneiss terrain of the Dharwar craton. [ABSTRACT FROM AUTHOR]
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Abstract:The Late Archaean Closepet Granite batholith in south India is exposed at different crustal levels grading from greenschist facies in the north through amphibolite and granulite facies in the south along a ~ 400 km long segment in the Dharwar craton. Two areas, Pavagada and Magadi, located in the Main Mass of the batholith, best represent the granitoid of the greenschist and amphibolite facies crustal levels respectively. Heat flow estimates of 38 mW m–2 from Pavagada and 25 mW m–2 from Magadi have been obtained through measurements in deep (430 and 445 m) and carefully sited boreholes. Measurements made in four boreholes of opportunity in Pavagada area yield a mean heat flow of 39 ± 4 (s.d.) mW m–2, which is in good agreement with the estimate from deep borehole. The study, therefore, demonstrates a clear-cut heat flow variation concomitant with the crustal levels exposed in the two areas. The mean heat production estimates for the greenschist facies and amphibolite facies layers constituting the Main Mass of the batholith are 2.9 and 1.8 lWm–3, respectively. The enhanced heat flow in the Pavagada area is consistent with the occurrence of a radioelement-enriched 2-km-thick greenschist facies layer granitoid overlying the granitoid of the amphibolite facies layer which is twice as thick as represented in the Magadi area. The crustal heat production models indicate similar mantle heat flow estimates in the range 12–14 mW m–2, consistent with the other parts of the greenstone-granite-gneiss terrain of the Dharwar craton. [ABSTRACT FROM AUTHOR]
ISSN:14373254
DOI:10.1007/s00531-007-0239-2