EGU21-6498, updated on 04 Mar 2021
https://doi.org/10.5194/egusphere-egu21-6498
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Synthetic and Comparative Hydrology of Earth, Mars, and Titan

Vojtěch Cuřín1, Johanna Blöcher1, Petr Brož1,2, Yannis Markonis1, Jan Masner1, Jan Pavlík1, Anezina Solomonidou1,3, and Nikola Šeborová1
Vojtěch Cuřín et al.
  • 1Czech University of Life Sciences Prague, Faculty of Environmental Sciences, Praha, Czech Republic
  • 2Institute of Geophysics of the Czech Academy of Science, Prague, Czech Republic
  • 3California Institute of Technology (Caltech), Pasadena, CA 91125, USA

Earth, Mars, and Titan are the only known planetary bodies in our solar system where flowing liquids have shaped surface topography and formed extensive river networks. Fed by atmospheric precipitation and carved by fluvial erosion, these channels are observable in remote sensing data. They carry information about the interactions between the atmosphere, the hydro(carbon)sphere, and the lithosphere and allow for investigation of the conditions that had prevailed during their formation. Comparison of drainage basins, which developed in these profoundly different environments, could yield insights into the past and ongoing hydrological processes in addition to climatic, chemical, and topographic conditions of the planetary bodies. Increased computing capacities allow for building and utilization of a vast database of hydrological, climatological, and geological data as well as algorithmic evaluation of remote sensing products. Here, we propose a classification of basins from Earth, Mars, and Titan using several machine learning techniques based on their morphological characteristics, network properties, spatial homogeneity, cross-scale self-similarity, and visual properties. Constraints on climatic and geologic properties of the terrestrial basin classes will be identified, and the results of their morphology-climatic relationship extrapolated to Mars and Titan. To find out more, visit our project’s website https://www.schemata-project.com/.

How to cite: Cuřín, V., Blöcher, J., Brož, P., Markonis, Y., Masner, J., Pavlík, J., Solomonidou, A., and Šeborová, N.: Synthetic and Comparative Hydrology of Earth, Mars, and Titan, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-6498, https://doi.org/10.5194/egusphere-egu21-6498, 2021.

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