The chemistry of habitable oceans in the Solar system

Liquid water exists on the Earth and several other planetary bodies in our solar system. The chemical character of these aqueous reservoirs is central to evaluating their habitability. Here, we synthesize the chemical features of water reservoirs and their biological implications on the modern Earth. We then outline constraints on the evolutionary history of Earth's ocean chemistry and discuss its interplay with the biosphere. Furthermore, we examine the inferred chemical environments of water bodies on early Mars, dwarf planet Ceres, Jupiter's moon Europa and Saturn's moons Enceladus and Titan. We conclude by outlining priority questions for future planetary habitability studies.

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Publication Details

Journal
Nature Communications
Published
2026-06-29
DOI
https://doi.org/10.1038/s41467-026-74955-4
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.00

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article

The chemistry of habitable oceans in the Solar system

Pengcheng Ju, Nicholas J. Tosca, Andrew H. Knoll, David C. Catling et al.
Nature Communications
Astro and Planetary Science
article

The chemistry of habitable oceans in the Solar system

Pengcheng Ju, Nicholas J. Tosca, Andrew H. Knoll, David C. Catling, Li Liao, Yuke Zhu, Fang Huang, Christopher R. Glein, Eva E. Stüeken, Maggie C. Y. Lau, Peter W. Crockford, Lu Pan, Jihua Hao, Yafang Song, Chao He, J.U. Mondal, Anya Huo, Jie Li
article en

Abstract

Liquid water exists on the Earth and several other planetary bodies in our solar system. The chemical character of these aqueous reservoirs is central to evaluating their habitability. Here, we synthesize the chemical features of water reservoirs and their biological implications on the modern Earth. We then outline constraints on the evolutionary history of Earth's ocean chemistry and discuss its interplay with the biosphere. Furthermore, we examine the inferred chemical environments of water bodies on early Mars, dwarf planet Ceres, Jupiter's moon Europa and Saturn's moons Enceladus and Titan. We conclude by outlining priority questions for future planetary habitability studies.

Nature CommunicationsVol. 17(1)
Anhui Jianzhu University (CN), University of Science and Technology of China (CN), Southwest Research Institute (US), Harvard University (US), Polar Research Institute of China (CN), University of St Andrews (GB), University of Washington (US), University of Cambridge (GB), Institute of Deep-Sea Science and Engineering (CN), Earth and Space Research (US), Carleton University (CA)
National Natural Science Foundation of China
Life below water
Openalex Percentile: Top 8%
Astro and Planetary Science
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