| 2003 Seattle Annual Meeting (November 2–5, 2003) | |
| Paper No. 222-3 | |
| Presentation Time: 8:00 AM-12:00 PM | ||
PRELIMINARY PALEOMAGNETIC DATA FROM RAJAHSTAN: IMPLICATIONS FOR RODINIA PALEOGEOGRAPHY | ||
|
REDFIELD, T.F.1, TORSVIK, T.H.1, ASHWAL, L.2, WEBB, S.2, and PANDIT, M.3, (1) Geodynamics, Royal Geol Survey of the Kingdom of Norway, Leiv Eirikssons vei 39, Trondheim, 7491, tim.redfield@ngu.no, (2) School of Geosciences, Univ of the Witwatersrand, Private Bag 3 Wits 2050, 1 Jan Smuts Avenue, Johannesburg, (3) Department of Geology, Universityof Rajasthan, Jaipur, 302-004 The Neoproterozoic Mt. Abu granitic pluton of southern Rajahstan, India, is crosscut by steeply-dipping, sub-parallel mafic dikes. Paleomagnetic measurements from the dikes have identified a steeply dipping high temperature component of magnetization. Both pluton and dikes are poorly dated but the age of magnetization probably ranges between 800 and 900 Ma; we await 40Ar/39Ar mica and U/Pb zircon ages to fully interpret the paleomagnetic data. Previous palaeomagnetic data from the 750 Ma Malani rhyolites (NW Rajahstan) yielded intermediate northerly latitudes for India during the Neoproterozoic, and India along with Madagascar and the Seychelles were separated from East Antarctica and Australia at this time. The presumably older palaeomagnetic data from the Mt. Abu dikes suggest that India occupied high northerly latitudes between 800-900 Ma (65-87oN) and subsequently drifted rapidly southward to reach subtropical latitudes at c. 750 Ma. This demonstrate that the Rodinia was not a static and equatorially cantered Supercontinent during the Neoproterozoic and break-up probably commenced at around 850 Ma.
| ||
|
2003 Seattle Annual Meeting (November 2–5, 2003)
| ||
| Session No. 222 Precambrian Geology (Posters) Washington State Convention and Trade Center: Hall 4-F 8:00 AM-12:00 PM, Wednesday, November 5, 2003 Geological Society of America Abstracts with Programs, Vol. 35, No. 6, September 2003, p. 505 | ||
© Copyright 2003 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions. | ||