Earth Syst. Dynam., 11, 291–299, 2020 https://doi.org/10.5194/esd-11-291-2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. Back to the future II: tidal evolution of four supercontinent scenarios Hannah S. Davies1,2, J. A. Mattias Green3, and Joao C. Duarte1,2,4 1Instituto Dom Luiz (IDL), Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016, Lisbon, Portugal 2Departamento de Geologia, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016, Lisbon, Portugal 3School of Ocean Sciences, Bangor University, Askew St, Menai Bridge LL59 5AB, UK 4School of Earth, Atmosphere and Environment, Monash University, Melbourne, VIC 3800, Australia Correspondence: Hannah S. Davies (
[email protected]) Received: 7 October 2019 – Discussion started: 25 October 2019 Revised: 3 February 2020 – Accepted: 8 February 2020 – Published: 20 March 2020 Abstract. The Earth is currently 180 Myr into a supercontinent cycle that began with the break-up of Pangaea and which will end around 200–250 Myr (million years) in the future, as the next supercontinent forms. As the continents move around the planet they change the geometry of ocean basins, and thereby modify their resonant properties. In doing so, oceans move through tidal resonance, causing the global tides to be profoundly affected. Here, we use a dedicated and established global tidal model to simulate the evolution of tides during four future supercontinent scenarios. We show that the number of tidal resonances on Earth varies between one and five in a supercontinent cycle and that they last for no longer than 20 Myr.