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Journal of African earth sciences v.139, 2018년, pp.403 - 420   SCIE
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Paleomagnetism of the Cretaceous Galula Formation and implications for vertebrate evolution

Widlansky, Sarah J. (Department of Earth Sciences, University of New Hampshire, Durham, NH, 03824, USA ) ; Clyde, William C. (Department of Earth Sciences, University of New Hampshire, Durham, NH, 03824, USA ) ; O'Connor, Patrick M. (Department of Biomedical Sciences, Ohio University Heritage College of Osteopathic Medicine, 228 Irvine Hall, Athens, OH, 45701, USA ) ; Roberts, Eric M. (Department of Geosciences, James Cook University, Townsville, Queensland, Australia ) ; Stevens, Nancy J. (Department of Biomedical Sciences, Ohio University Heritage College of Osteopathic Medicine, 228 Irvine Hall, Athens, OH, 45701, USA ) ;
  • 초록  

    Abstract This study uses magnetostratigraphy to help constrain the age of the paleontologically important Galula Formation (Rukwa Rift Basin, southwestern Tanzania). The formation preserves a Cretaceous vertebrate fauna, including saurischian dinosaurs, a putative gondwanatherian mammal, and notosuchian crocodyliforms. With better dating, the Galula Formation and its fossils help fill a temporal gap in our understanding of vertebrate evolution in continental Africa, enabling better evaluation of competing paleobiogeographic hypotheses concerning faunal exchange throughout Gondwana during the Cretaceous. Paleomagnetic samples for this study were collected from the Namba (higher in section) and Mtuka (lower in section) members of the Galula Formation and underwent stepwise thermal demagnetization. All samples displayed a strong normal magnetic polarity overprint, and maximum unblocking temperatures at approximately 690 °C. Three short reversed intervals were identified in the Namba Member, whereas the Mtuka Member lacked any clear reversals. Given the relatively limited existing age constraints, one interpretation correlates the Namba Member to Chron C32. An alternative correlation assigns reversals in the Namba Member to recently proposed short reversals near the end of the Cretaceous Normal Superchron (Chron C34), a time that is traditionally interpreted as having stable normal polarity. The lack of reversals in the Mtuka Member supports deposition within Chron C34. These data suggest that the Namba Member is no older than Late Cretaceous (Cenomanian-Campanian), with the Mtuka Member less well constrained to the middle Cretaceous (Aptian-Cenomanian). The paleomagnetic results are supported by the application of fold and reversal tests for paleomagnetic stability, and paleomagnetic poles for the Namba (246.4°/77.9°, α 95 5.9°) and Mtuka (217.1°/72.2°, α 95 11.1°) members closely matching the apparent polar wander path for Africa during the Late Cretaceous. These results confidently indicate a Late Creteceous age assignment for the Namba Member of the Galula Formation, a unit that has yielded key crocodyliform (e.g., Pakasuchus ; Rukwasuchus ) and dinosaur (e.g., Rukwatitan; Shingopana ) fossils from eastern Africa. Highlights New paleomagnetic results from the Cretaceous Galula Formation of southwest Tanzania offer additional age constraint. Namba Member consistent with deposition during the Late Cretaceous. Mtuka Member consistent with deposition in the middle Cretaceous during the Cretaceous Normal Superchron.


  • 주제어

    Paleomagnetism .   Late Cretaceous .   Africa .   Tanzania .   Rukwa Rift Basin.  

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