Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
4729918 | Journal of African Earth Sciences | 2006 | 10 Pages |
Abstract
The Neoproterozoic crust of the Tibesti massif was stabilized by magmatism that included subduction-generated batholithic suites and post-orogenic granite plutons. All of the magmatism occurred in a period of about 20 million years centered around 550 Ma, and nearly all of the granites have initial 87Sr/86Sr ratios of about 0.706. The Wadi Yebigue pluton has U–Pb zircon ages of 563 Ma and 558 Ma on two different phases and εNd at 550 Ma from −0.5 to −2.2. These isotopic data and the geologic history of the massif suggest that granites in the Tibesti massif developed during and shortly after closure of a short-lived ocean basin that developed by fragmentation of pre-existing continental crust of the Saharan region.
Related Topics
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Earth and Planetary Sciences
Geology
Authors
Ismail B. Suayah, Jonathan S. Miller, Brent V. Miller, Tovah M. Bayer, John J.W. Rogers,