EGU25-13954, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-13954
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
“Short” or “Long” Hettangian? Astronomical chronometry on the duration of lower Jurassic Hettangian stage and the recovery dynamics following the end – Triassic mass extinction. 
Amanda Perera1, Micha Ruhl1, Weimu Xu2, Ricardo L. Silva3, Rob Raine4, and Robbie Goodhue5
Amanda Perera et al.
  • 1Department of Geology, School of Natural Sciences, & SFI Research Centre in Applied Geosciences (iCRAG), Trinity College Dublin, The University of Dublin, Dublin, Ireland (Micha.Ruhl@tcd.ie)
  • 2School of Earth Sciences, & SFI Research Centre in Applied Geosciences (iCRAG), University College Dublin, Dublin, Ireland (weimu.xu1@ucd.ie)
  • 3Clayton H. Riddell Faculty of Environment, Earth and Resources, University of Manitoba, Winnipeg, Manitoba, Canada
  • 4Geological Survey of Northern Ireland, Adelaide House, 39-49 Adelaide Street, Belfast, BT24 8FD, Northern Ireland, United Kingdom
  • 5Department of Geology, School of Natural Sciences, Trinity College Dublin, The University of Dublin, Dublin, Ireland

The end-Triassic mass extinction (ETME) and global climatic perturbation coincide with the onset of Central Atlantic Magmatic Province (CAMP) emplacement. The associated perturbation to the global carbon cycle is reflected by a ~ 3 – 6 ‰ negative carbon isotope excursion (CIE) coinciding with the ETME. The magnitude and duration of the negative CIE are however poorly constrained. Furthermore, the Early Jurassic Hettangian stage, marking the initial recovery phase following the end-Triassic mass extinction, has been the subject of significant debate over its precise timing and duration. Estimated Hettangian stage durations derived from cyclostratigraphic and U-Pb geochronological analyses vary between a ‘short Hettangian’ of 1.8 – 2.5 Myr, and a ‘long Hettangian’ of 3.9 – 4.4 Myr. Poor time constraints for the Triassic–Jurassic interval impact understanding of the timing and rate of biogeochemical cycling, environmental and biological recovery after the end-Triassic mass extinction, and global climatic perturbation.

We here conducted carbon isotopic and cyclostratigraphic analysis of the well-preserved, biostratigraphically complete, and expanded Hettangian succession in the Carnduff-2 core of the Larne Basin (Northern Ireland), nearby the Waterloo Bay outcrop. The studied sedimentary succession (~120 m in core) stratigraphically spans the upper Rhaetian (upper Triassic), including the end-Triassic mass extinction, Hettangian, and lower Sinemurian (lower Jurassic), and consists of predominantly mudstone, with varying degrees of limestone and silt throughout the succession. Cyclostratigraphic analyses of elemental and carbonate concentration data show a hierarchy of dominant frequencies, interpreted to reflect long and short eccentricity, obliquity, and precession. These observations suggest a total duration of ~2.2 Myr for the Hettangian Stage with a sedimentation rate of ~ 4.1 cm/kyr, confirming the ‘short-Hettangian’ hypothesis. The negative carbon isotope excursion (CIE) duration, which coincides with the ETME, is estimated at ~290 kyr. The first occurrence of the Jurassic ammonite Psiloceras tillmanni, marking the onset of Hettangian biotic recovery after the ETME across the British Isles, ~320 kyr after the end-Triassic negative CIE, suggesting a prolonged period of biotic demise in response to CAMP induced climatic and environmental upheaval at this time.

Key Words: end-Triassic mass extinction, Early Jurassic, Hettangian stage, Milankovitch cycles

 

How to cite: Perera, A., Ruhl, M., Xu, W., Silva, R. L., Raine, R., and Goodhue, R.: “Short” or “Long” Hettangian? Astronomical chronometry on the duration of lower Jurassic Hettangian stage and the recovery dynamics following the end – Triassic mass extinction. , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13954, https://doi.org/10.5194/egusphere-egu25-13954, 2025.