Origin & Evolution of Life

Ionic Liquid Biospheres

By Keith Cowing
Status Report
astro-ph.EP
March 6, 2026
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Ionic Liquid Biospheres
Chemical structures of selected ILs and DES. (a) Anions common to planetary environments could lead to abiotic formation of ILs and DES, including, e.g., NO3 , HSO4 , Cl, ClO4, HCOO, CH3COO, FeCl4, and CO32−. In principle, any positively charged nitrogen-containing organic molecule could act as the cation in a “planetary” ionic liquid pair; (b) selected industrial synthetic ionic liquids not expected to be present in planetary settings; (c) the known natural ionic liquid formed between two ant species as a venom counteragent; (d) examples of selected natural deep eutectic solvents (NADES) mixtures made by desert plants and fly larvae. Note that NADES mixtures can be very diverse in their chemical composition and molar ratios of individual components, differing significantly even between closely related species. — astro-ph.EP

Liquid is a fundamental requirement for life as we understand it, but whether that liquid has to be water is not known.

We propose the hypothesis that ionic liquids (ILs) and deep eutectic solvents (DES) constitute a class of non-aqueous planetary liquids capable of persisting on a wide range of bodies where stable liquid water cannot exist.

This hypothesis is motivated by key physical properties of ILs and DES. Many exhibit vapor pressures orders of magnitude lower than that of water and remain liquid across exceptionally wide temperature ranges, from cryogenic to well above terrestrial temperatures. These properties permit stable liquids to exist where liquid water would rapidly evaporate or freeze and outside of bulk phases as persistent microscale reservoirs-such as thin films and pore-filling droplets.

In other words, ILs and DES can persist in environments without requiring oceans, thick atmospheres, or narrowly regulated climate conditions. We further hypothesize that ILs and DES could act as solvents for non-Earth-like life. Our hypothesis ex-tends to the idea that ILs and DES could enable prebiotic chemistry by providing long-lived, protective liquid environments for complex organic molecules on bodies such as comets and asteroids, where liquid water is absent.

Based on the occurrence of DES-like mixtures as protective intracellular liquids in desiccation-tolerant plants, we propose that ILs and DES might be solvents that life elsewhere purposefully evolves. We review protein and other biomolecule studies in ILs and DES and outline planetary environments in which ILs and DES might occur by discussing available anions and cations.

We present strategies to advance the IL/DES solvent hypothesis using laboratory studies, computational chemistry, planetary missions, analysis of existing spectroscopic datasets, and modeling of liquid microniches and chemical survival on small bodies.

Sara Seager, William Bains, Iaroslav Iakubivskyi, Rachana Agrawal, John Jenkins, Pranav Shinde, Janusz J. Petkowski

Comments: Published in Life, section Astrobiology
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2603.02776 [astro-ph.EP] (or arXiv:2603.02776v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2603.02776
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Journal reference: Life 2026, 16(3), 408
Related DOI:
https://doi.org/10.3390/life16030408
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Submission history
From: Janusz Petkowski
[v1] Tue, 3 Mar 2026 09:16:52 UTC (669 KB)
https://arxiv.org/abs/2603.02776
Astrobiology,

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻