EGU2020-5821
https://doi.org/10.5194/egusphere-egu2020-5821
EGU General Assembly 2020
© Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License.
The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation
- 1NASA, Goddard Institute for Space Studies, New York, United States of America (michael.j.way@nasa.gov)
- 2Goddard Space Flight Center Sellers Exoplanet Environments Collaboration, USA
- 3Theoretical Astrophysics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden
- 4Instituto Dom Luiz (IDL), Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal
- 5Departamento de Geologia, Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal
- 6School of Earth, Atmosphere and Environment, Monash University, Melbourne, Victoria, Australia
- 7School of Ocean Sciences, Bangor University, Menai Bridge, UK
We investigate two possible deep future Earth climate scenarios using a 3-D GCM [1], 200 and 250 million years into the future when the next supercontinent phase is expect to take place. We use knowledge of the evolution of plate tectonics, solar luminosity, and rotation rate over this time period. In one scenario, a supercontinent forms at low latitudes. In the other scenario it forms at high northerly latitudes with an Antarctic subcontinent remaining at the south pole. The climates differences between these two scenarios are dramatic, with differences in mean surface temperatures approaching 4 degrees. The fractional habitability (where mean surface temperatures are between 0<T<100C year round) on land surfaces (as opposed to the ocean) is shown to differ up to 40% between the two simulations. We believe these demonstrate that the community needs to consider alternative boundary conditions when simulating Earth-like exoplanetary climates.
[1] Way et al. 2017, ApJS, 231, 21.
How to cite: Way, M., Davies, H., Duarte, J., and Green, M.: The climates of Earth's next supercontinent: effects of tectonics, rotation rate, and insolation, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-5821, https://doi.org/10.5194/egusphere-egu2020-5821, 2020
