Implications of the Newark Supergroup-based astrochronology and geomagnetic polarity time scale (Newark-APTS) for the tempo and mode of the early diversification of the Dinosauria
Olsen
Paul E.
author
Columbia University. Earth and Environmental Sciences
Kent
Dennis V.
author
Columbia University. Lamont-Doherty Earth Observatory
Whiteside
Jessica H.
author
Columbia University. Lamont-Doherty Earth Observatory
originator
text
Articles
2011
English
The Newark-APTS established a high-resolution framework for the Late Triassic and Early Jurassic. Palaeomagnetic polarity correlations to marine sections show that stage-level correlations of continental sequences were off by as much as 10 million years. New U–Pb ages show the new correlations and the Newark basin astrochronology to be accurate. Correlation of Newark-APTS to the Chinle Formation/Dockum Group, Glen Canyon Group, Fleming Fjord Formation and Ischigualasto Formation led to the following conclusions: (1) there are no unequivocal Carnian-age dinosaurs; (2) the Norian Age was characterised by a slowly increasing saurischian diversity but no unequivocal ornithischians; (3) there was profound Norian and Rhaetian continental provinciality; (4) the classic Chinle-, Germanic- and Los Colorados-type assemblages may have persisted to the close of the Rhaetian; (5) the distinct genus-level biotic transition traditionally correlated with the marine Carnian–Norian is in fact mid-Norian in age and within published error of the Manicouagan impact; (6) the end-Triassic marine and continental extinctions as seen in eastern North America were contemporaneous; and (7) compared to Triassic communities, Hettangian and Sinemurian age terrestrial communities were nearly globally homogenous and of low diversity. Consequently, the complex emerging picture of dinosaur diversification demands biostratigraphically-independent geochronologies in each of the faunally-important regions.
Geology
Paleontology
Earth and Environmental Science Transactions of the Royal Society of Edinburgh
101
3-4
201
229
2011-05
http://dx.doi.org/10.1017/S1755691011020032
http://hdl.handle.net/10022/AC:P:12397
NNC
NNC
2012-01-30 14:39:15 -0500
2013-02-11 15:39:10 -0500
6394
eng