EGU24-18542, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-18542
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Continuous 3D modelling over deep time – the SCION Earth Evolution Model

Benjamin Mills1, Dongyu Zheng2, Khushboo Gurung1, Andrew Merdith3, Alexander Krause1, Zhen Xu1, Fred Bowyer1, and Stephen Hunter1
Benjamin Mills et al.
  • 1University of Leeds, United Kingdom of Great Britain – England, Scotland, Wales (b.mills@leeds.ac.uk)
  • 2Chengdu University of Technology, Chengdu, China (dzheng9295@126.com)
  • 3University of Adelaide, Adelaide, Australia (andrew.merdith@adelaide.edu.au)

Earth system models for deep time have typically been unable to represent geological timespans in 3D because climate and ocean circulation plays a key role in global biogeochemistry and generating a 3D physical climate simulation is extremely computationally expensive. This means that Earth System Modelling for periods of over 1 Myr has been exclusively carried out in nondimensional box models, which leads to oversimplification of spatially heterogeneous processes like continental weathering and marine carbon burial. This simplification may be a key reason why so many climate questions over deep time remain unresolved. The SCION (Spatial Continuous IntegratiON) project aims to produce a 3D and self-consistent climate and biogeochemical system that can be run over billion-year timeframes. To do this, it employs a physical climate emulator which is developed using a Deep Learning method trained on hundreds of General Circulation Model runs over different paleogeographies and CO2 levels. The SCION development project – SIM-EARTH – also includes a new process-based reconstruction of paleotopography using the GPlates kinematic plate model, development of a long-term dynamic global vegetation module and ocean biogeochemical module, and databasing projects to establish 3D datasets for marine and terrestrial palaeontology and geochemistry that can be compared to model outputs at the local scale to test hypotheses. We hope that new model frameworks like this can help us better understand the evolution of Earth’s surface conditions over time, assess the contribution of the biosphere to global environmental change, and help determine what fundamental characteristics are required for a planet to be habitable for complex life.

How to cite: Mills, B., Zheng, D., Gurung, K., Merdith, A., Krause, A., Xu, Z., Bowyer, F., and Hunter, S.: Continuous 3D modelling over deep time – the SCION Earth Evolution Model, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-18542, https://doi.org/10.5194/egusphere-egu24-18542, 2024.