Modelling the long-term impacts of artificial warming on the Martian water cycle and surface ice distribution

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Braude, Ashwin S., Kite, Edwin S., Richardson, Mark I., Kling, Alexandre, Mischna, Michael A.
Format: Preprint
Publié: 2026
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866910037730918400
author Braude, Ashwin S.
Kite, Edwin S.
Richardson, Mark I.
Kling, Alexandre
Mischna, Michael A.
author_facet Braude, Ashwin S.
Kite, Edwin S.
Richardson, Mark I.
Kling, Alexandre
Mischna, Michael A.
contents Recent papers by Ansari et al. (2024, Science Advances 10, eadn4650) and Richardson et al. (2025, arXiv eprint 2504.01455) have suggested that global warming of the Martian surface ('terraforming') by 35 K to sustain local habitats above the melting point of water could be achieved through the injection of engineered aerosols into the Martian atmosphere. Using the MarsWRF 3D Global Climate Model, we investigate how artificial warming of Mars through engineered aerosol release would affect the planetary water cycle and the distribution of the major surface ice reservoirs. Within our model framework, every 20 K of global warming induces a tenfold increase in atmospheric water vapour content due to sublimation of H2O ice from the North Polar Cap. This increases the potency of cloud radiative feedbacks which induces nighttime warming (~5-10 K) at low latitudes, but daytime cooling (up to 40 K) in the winter midlatitudes. Water is transferred from the edge of the North Polar Cap to the South Polar Cap and there is minor destabilisation of shallow northern midlatitude subsurface ice. As a result, seasonal sublimation of H2O ice from the South Pole has an increased impact on the global water cycle. These changes persist on Mars at least decades after loading of the atmosphere with engineered aerosols ceases. Our model is limited by the gaps in our knowledge of present-day Martian weather and climate, and of the microphysics and radiative properties of candidate warming agents. Much more data is therefore needed before warming Mars could become feasible.
format Preprint
id arxiv_https___arxiv_org_abs_2603_01539
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Modelling the long-term impacts of artificial warming on the Martian water cycle and surface ice distribution
Braude, Ashwin S.
Kite, Edwin S.
Richardson, Mark I.
Kling, Alexandre
Mischna, Michael A.
Earth and Planetary Astrophysics
Atmospheric and Oceanic Physics
Geophysics
Recent papers by Ansari et al. (2024, Science Advances 10, eadn4650) and Richardson et al. (2025, arXiv eprint 2504.01455) have suggested that global warming of the Martian surface ('terraforming') by 35 K to sustain local habitats above the melting point of water could be achieved through the injection of engineered aerosols into the Martian atmosphere. Using the MarsWRF 3D Global Climate Model, we investigate how artificial warming of Mars through engineered aerosol release would affect the planetary water cycle and the distribution of the major surface ice reservoirs. Within our model framework, every 20 K of global warming induces a tenfold increase in atmospheric water vapour content due to sublimation of H2O ice from the North Polar Cap. This increases the potency of cloud radiative feedbacks which induces nighttime warming (~5-10 K) at low latitudes, but daytime cooling (up to 40 K) in the winter midlatitudes. Water is transferred from the edge of the North Polar Cap to the South Polar Cap and there is minor destabilisation of shallow northern midlatitude subsurface ice. As a result, seasonal sublimation of H2O ice from the South Pole has an increased impact on the global water cycle. These changes persist on Mars at least decades after loading of the atmosphere with engineered aerosols ceases. Our model is limited by the gaps in our knowledge of present-day Martian weather and climate, and of the microphysics and radiative properties of candidate warming agents. Much more data is therefore needed before warming Mars could become feasible.
title Modelling the long-term impacts of artificial warming on the Martian water cycle and surface ice distribution
topic Earth and Planetary Astrophysics
Atmospheric and Oceanic Physics
Geophysics
url https://arxiv.org/abs/2603.01539