Articles | Volume 19, issue 14
https://doi.org/10.5194/gmd-19-6909-2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/gmd-19-6909-2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
A global high-resolution hydrological model to simulate the dynamics of surface liquid reservoirs: application on Mars
Alexandre Gauvain
CORRESPONDING AUTHOR
Laboratoire de Météorologie Dynamique, CNRS, Sorbonne Université, Paris, France
François Forget
Laboratoire de Météorologie Dynamique, CNRS, Sorbonne Université, Paris, France
Martin Turbet
Laboratoire de Météorologie Dynamique, CNRS, Sorbonne Université, Paris, France
Laboratoire d'Astrophysique de Bordeaux, Université de Bordeaux, Bordeaux, France
Jean-Baptiste Clément
Laboratoire de Météorologie Dynamique, CNRS, Sorbonne Université, Paris, France
Lucas Lange
Laboratoire de Météorologie Dynamique, CNRS, Sorbonne Université, Paris, France
Romain Vandemeulebrouck
Laboratoire de Météorologie Dynamique, CNRS, Sorbonne Université, Paris, France
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Editorial statement
Observational evidence suggests that the planet Mars had, at some stage in its history, signifcant surface water. This paper presents a global computational hydrological model of Mars capable of representing that water in various configurations. This provides one component for a future computational model of Mars' ancient climate and offers a route towards greater understanding of the role that water played in the formation of the planet's surface.
Observational evidence suggests that the planet Mars had, at some stage in its history,...
Short summary
In this paper, we present a global high-resolution hydrological model to investigate how water may have once flowed and accumulated on Mars. Using detailed topography, the model tracks how lakes and seas form, grow, merge, overflow, and dry out over time. It reveals how a vast northern ocean could emerge from smaller bodies of water. This approach links surface landforms to past climates, offering new perspectives on Mars' watery history and its potential habitability.
In this paper, we present a global high-resolution hydrological model to investigate how water...