25.01.2015 Views

IASPEI - Picture Gallery

IASPEI - Picture Gallery

IASPEI - Picture Gallery

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy<br />

(S) - <strong>IASPEI</strong> - International Association of Seismology and Physics of the Earth's<br />

Interior<br />

JSS013 Oral Presentation 2228<br />

Lithospheric structure and its relationship to diamond fertility of Dharwar<br />

and Bastar cratons of the indian shield - a gravity perspective<br />

Dr. Bijendra Singh<br />

National Geophysical Research Institute, Hyderabad Scientist <strong>IASPEI</strong><br />

V. M. Tiwari, S. K. Verma<br />

One of the unique features of the Indian shield is that it consists of number of Cratonic blocks bounded<br />

by mobile belts. The lithospheric structures across these terrains are not well resolved due to scanty of<br />

data. We have carried out gravity modeling along two long profiles cutting across the Indian shield to<br />

understand the lithospheric configuration below the Dharwar and Bastar Cratons. Modeling is<br />

constrained by the available geophysical results from deep seismic sounding, receiver function analysis,<br />

seismic tomography and magnetotelluric methods. After accounting for the anomalies due to known<br />

geological structures in the crust, long wavelength gravity response is interpreted in terms of variation<br />

in the thickness of the lithosphere.Modeling results suggest that the lithosphere below the western<br />

Dharwar Craton has got a maximum thickness of about 220-230 Km that reduces towards Eastern<br />

Dharwar Craton to about 150 Km. Under the Godavari rift, it further reduces to about 100-120 Km.<br />

North of Godavari in the Bastar Craton: the thickness again increases northward to about 200 Km.<br />

Interestingly, the study of 1.1 Ga mantle xenoliths from kimberlite of Dharwar Craton also provide<br />

similar depths. The lithospheric model thus obtained has significant implications on the geodynamic<br />

evolution of Dharwar and Bastar Cratons and Diamond fertility of Kimberlite fields north and south<br />

ofGodavari rift.It is suggested that the Godavari rift represents the zone of suturing between Dharwar<br />

and Bastar Cratons during Archean period. The continent-continent collision of Dharwar and Bastar<br />

Cratons along Godavari suture zone (GSZ) gave rise to number of parallel fracture zones both north and<br />

south of the suture.The diamond fertility in Dharwar and Bastar Cratons are also governed by the GSZ<br />

below which the two Cratonic blocks show minimum thickness that is not conducive for diamond<br />

generation and stability. This is well reflected in the diamond barren kimberlite clusters belonging to<br />

Tokapal kimberlite field lying in the north and Narayanpet kimberlite field (NKF) lying to the south of<br />

GSZ. Kimberlite clusters further away from GZS are likely to be diamond fertile as they sample a thicker<br />

lithosphere providing necessary conditions for diamond generation and stability. Geochemical studies of<br />

mantle xenolith also reveal that these are derived from a 220-240 km thick lithosphere from less than<br />

160 km lithosphere for the NKF. It is inferred that the Dharwar Craton in Peninsular India has not been<br />

subjected to any major destabilization during the past one billion years.<br />

Keywords: kimberlite, cratons, gravitymodeling

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!