- 1Earth Surface Science Institute, School of Earth and Environment, University of Leeds, Leeds, United Kingdom (S.Hunter@leeds.ac.uk)
- 2Tectonics and Earth Systems Group, School of Physics, Chemistry and Earth Sciences, The University of Adelaide, Adelaide, Australia
The late Neoproterozoic Era saw deep glaciation and possible rises in atmospheric and marine oxygen levels. It has been suggested that these environmental changes could be the consequence of supercontinent breakup and amplified continental weathering rates, which could have drawn down CO2 and liberated nutrients. But this idea has not been tested using recent paleogeographic reconstructions and paleoclimate modelling. Here we present a suite of HadCM3L climate model simulations covering the late Neoproterozoic Era, specifically the descent into the Sturtian glaciation (800 – 715 Ma), based upon a new full-plate model and palaeogeographic framework. We outline the modelling strategy which includes representation of continental-scale icesheets and investigate the sensitivity of the climate to changing palaeogeography. To assess the implications for the carbon cycle, the resulting suite of climatologies are incorporated into the SCION climate-chemical model to produce a self-consistent reconstruction of biogeochemistry (including chemical weathering and atmospheric O2 and CO2) and climate.
How to cite: Hunter, S., Mills, B., Merdith, A., and Haywood, A.: Climate Modelling of the late Neoproterozoic Era., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8991, https://doi.org/10.5194/egusphere-egu25-8991, 2025.