Extreme ecosystem instability suppressed tropical dinosaur dominance for 30 million years

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Extreme ecosystem instability suppressed tropical dinosaur dominance for 30 million years. / Whiteside, J.H.; Lindström, S.; Irmis, R.B.; Glasspool, I.J.; Schaller, M.F.; Dunlavey, M.; Nesbitt, S.J.; Smith, N.D.; Turner, A.H.

In: Proceedings of the National Academy of Sciences of the United States of America, Vol. 112, No. 26, 2015.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Whiteside, JH, Lindström, S, Irmis, RB, Glasspool, IJ, Schaller, MF, Dunlavey, M, Nesbitt, SJ, Smith, ND & Turner, AH 2015, 'Extreme ecosystem instability suppressed tropical dinosaur dominance for 30 million years', Proceedings of the National Academy of Sciences of the United States of America, vol. 112, no. 26. https://doi.org/10.1073/pnas.1505252112

APA

Whiteside, J. H., Lindström, S., Irmis, R. B., Glasspool, I. J., Schaller, M. F., Dunlavey, M., Nesbitt, S. J., Smith, N. D., & Turner, A. H. (2015). Extreme ecosystem instability suppressed tropical dinosaur dominance for 30 million years. Proceedings of the National Academy of Sciences of the United States of America, 112(26). https://doi.org/10.1073/pnas.1505252112

Vancouver

Whiteside JH, Lindström S, Irmis RB, Glasspool IJ, Schaller MF, Dunlavey M et al. Extreme ecosystem instability suppressed tropical dinosaur dominance for 30 million years. Proceedings of the National Academy of Sciences of the United States of America. 2015;112(26). https://doi.org/10.1073/pnas.1505252112

Author

Whiteside, J.H. ; Lindström, S. ; Irmis, R.B. ; Glasspool, I.J. ; Schaller, M.F. ; Dunlavey, M. ; Nesbitt, S.J. ; Smith, N.D. ; Turner, A.H. / Extreme ecosystem instability suppressed tropical dinosaur dominance for 30 million years. In: Proceedings of the National Academy of Sciences of the United States of America. 2015 ; Vol. 112, No. 26.

Bibtex

@article{7b12b0cf4d384352bc33d342b4a4381c,
title = "Extreme ecosystem instability suppressed tropical dinosaur dominance for 30 million years",
abstract = "A major unresolved aspect of the rise of dinosaurs is why early dinosaurs and their relatives were rare and species-poor at low paleolatitudes throughout the Late Triassic Period, a pattern persisting 30 million years after their origin and 10–15 million years after they became abundant and speciose at higher latitudes. New palynological, wildfire, organic carbon isotope, and atmospheric pCO2 data from early dinosaur-bearing strata of low paleolatitudes in western North America show that large, high-frequency, tightly correlated variations in δ13Corg and palynomorph ecotypes occurred within a context of elevated and increasing pCO2 and pervasive wildfires. Whereas pseudosuchian archosaur-dominated communities were able to persist in these same regions under rapidly fluctuating extreme climatic conditions until the end-Triassic, large-bodied, fast-growing tachymetabolic dinosaurian herbivores requiring greater resources were unable to adapt to unstable high CO2 environmental conditions of the Late Triassic.",
author = "J.H. Whiteside and S. Lindstr{\"o}m and R.B. Irmis and I.J. Glasspool and M.F. Schaller and M. Dunlavey and S.J. Nesbitt and N.D. Smith and A.H. Turner",
year = "2015",
doi = "10.1073/pnas.1505252112",
language = "English",
volume = "112",
journal = "Proceedings of the National Academy of Sciences of the United States of America",
issn = "0027-8424",
publisher = "The National Academy of Sciences of the United States of America",
number = "26",

}

RIS

TY - JOUR

T1 - Extreme ecosystem instability suppressed tropical dinosaur dominance for 30 million years

AU - Whiteside, J.H.

AU - Lindström, S.

AU - Irmis, R.B.

AU - Glasspool, I.J.

AU - Schaller, M.F.

AU - Dunlavey, M.

AU - Nesbitt, S.J.

AU - Smith, N.D.

AU - Turner, A.H.

PY - 2015

Y1 - 2015

N2 - A major unresolved aspect of the rise of dinosaurs is why early dinosaurs and their relatives were rare and species-poor at low paleolatitudes throughout the Late Triassic Period, a pattern persisting 30 million years after their origin and 10–15 million years after they became abundant and speciose at higher latitudes. New palynological, wildfire, organic carbon isotope, and atmospheric pCO2 data from early dinosaur-bearing strata of low paleolatitudes in western North America show that large, high-frequency, tightly correlated variations in δ13Corg and palynomorph ecotypes occurred within a context of elevated and increasing pCO2 and pervasive wildfires. Whereas pseudosuchian archosaur-dominated communities were able to persist in these same regions under rapidly fluctuating extreme climatic conditions until the end-Triassic, large-bodied, fast-growing tachymetabolic dinosaurian herbivores requiring greater resources were unable to adapt to unstable high CO2 environmental conditions of the Late Triassic.

AB - A major unresolved aspect of the rise of dinosaurs is why early dinosaurs and their relatives were rare and species-poor at low paleolatitudes throughout the Late Triassic Period, a pattern persisting 30 million years after their origin and 10–15 million years after they became abundant and speciose at higher latitudes. New palynological, wildfire, organic carbon isotope, and atmospheric pCO2 data from early dinosaur-bearing strata of low paleolatitudes in western North America show that large, high-frequency, tightly correlated variations in δ13Corg and palynomorph ecotypes occurred within a context of elevated and increasing pCO2 and pervasive wildfires. Whereas pseudosuchian archosaur-dominated communities were able to persist in these same regions under rapidly fluctuating extreme climatic conditions until the end-Triassic, large-bodied, fast-growing tachymetabolic dinosaurian herbivores requiring greater resources were unable to adapt to unstable high CO2 environmental conditions of the Late Triassic.

U2 - 10.1073/pnas.1505252112

DO - 10.1073/pnas.1505252112

M3 - Journal article

VL - 112

JO - Proceedings of the National Academy of Sciences of the United States of America

JF - Proceedings of the National Academy of Sciences of the United States of America

SN - 0027-8424

IS - 26

ER -

ID: 290263595