Revised age constraints for Late Cretaceous to early Paleocene terrestrial strata from the Dawson Creek section, Big Bend National Park, west Texas

Caitlin E. Leslie, Daniel J. Peppe, Thomas E. Williamson, Matthew Heizler, Mike Jackson, Stacy C. Atchley, Lee Nordt, Barbara Standhardt

Research output: Contribution to journalArticlepeer-review

17 Scopus citations


We analyzed samples for paleomagnetism, 40Ar/39Ar detrital sanidine ages, and mammalian fauna to produce a precise chronostratigraphic framework for the Upper Cretaceous to Lower Paleocene Dawson Creek section of Big Bend National Park, west Texas. Prior to this work, the absolute ages and durations of the Upper Cretaceous Aguja and Javelina Formations and Paleocene Black Peaks Formation were relatively poorly constrained. The documented polarity zones can be correlated to C32n-C31n, C29r, and C27r of the geomagnetic polarity time scale, with three hiatuses spanning more than 1.5 m.y. each. Rock magnetic analyses indicate that the dominant magnetic carrier in the Aguja and Black Peaks Formations is titanomagnetite, while the Javelina Formation has varying magnetic carriers, including hematite, magnetite, and maghemite. An overprint interval surrounding the Cretaceous-Paleogene boundary suggests the primary magnetic carrier, titanohematite, was likely reset by burial and/or overlying basaltic flows. These are the first independent age constraints for the Cretaceous-Paleocene strata at the Dawson Creek section that determine the age and duration of deposition of each formation in the section, as well as the age and duration of multiple unconformities through the succession. As a result, these age constraints can be used to reassess biostratigraphic and isotopic correlations between the Big Bend area and other Cretaceous-Paleogene basins across North America. Based on this new data set, we reassign the age of the mammalian fauna found in the Black Peaks Formation from the Puercan to the Torrejonian North American Land Mammal age. Our age constraints show that the dinosaur fauna in the Javelina Formation in the Dawson Creek area is latest Maastrichtian and restricted to chron C29r. Thus, the Javelina dinosaur fauna is correlative to the Hell Creek Formation dinosaur fauna from the Northern Great Plains, indicating differences between the faunas are not due to differences in age, and providing support for the hypothesis of provinciality and endemism in dinosaur communities in the late Maastrichtian. Further, the age constraints indicate that the previously documented mid-Maastrichtian and late Maastrichtian greenhouse events were rapid ( < 200 k.y.) and correlate closely with climate events documented in the marine record.

Original languageEnglish (US)
Pages (from-to)1143-1163
Number of pages21
JournalBulletin of the Geological Society of America
Issue number7-8
StatePublished - Jul 1 2018

Bibliographical note

Funding Information:
This work was conducted in Big Bend National Park on research permit BIBE-2014-SCI-005 to Leslie. This work was supported by the Society for Sedimentary Geology (SEPM), National Science Foundation grants EAR-132552, 0207750, and 1325544, the American Chemical Society Petroleum Research Fund (PRF#52822-DN18), Baylor University Department of Geosciences' Dixon Fund, and the Institute for Rock Magnetism. The Institute for Rock Magnetism is supported by the Instruments and Facilities program of the National Science Foundation, and by the University of Minnesota. We thank two anonymous reviewers for their helpful comments and B. Pratt and B. Singer for editorial assistance. Thanks go to A. Ramsey for assistance with sample collec tion and section measuring, L. Peters for assistance with sanidine separation, J. Schiebout and S. Ting of Louisiana State University (LSU) and M. Brown and C. Sagebiel of Texas Memorial Museum (TMM) for providing access and loan of fossil specimens, and J. Feinberg for helpful discussions

Publisher Copyright:
© 2018 The Authors.


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