Fluid Flow In Ceres Due To Core Heating

editorAstrobiology6 hours ago3 Views

Fluid Flow In Ceres Due To Core Heating
This illustration depicts the interior of dwarf planet Ceres, including the transfer of water and gases from the rocky core to a reservoir of salty water as a consequence of internal heating. NASA ID: PIA26570 larger image

A couple examples of molecules carrying chemical energy – carbon dioxide and methane – are included in the illustration.

Research published in Science Advances on Aug. 20, 2025 (Ceres May Have Had Long-Standing Energy to Fuel Habitability), relies on data from NASA’s Dawn mission to find that chemical energy inside Ceres may have lasted long enough to fuel microbial metabolisms.

Although there is no evidence that microorganisms ever existed on Ceres, the finding supports theories that this intriguing dwarf planet, which is the largest body in the main asteroid belt between Mars and Jupiter, may have once had conditions suitable to support single-celled lifeforms.

Core metamorphism controls the dynamic habitability of mid-sized ocean worlds—The case of Ceres, Science Advances (open access)

Astrobiology, Astrogeology, Astrochemistry,

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) 🖖🏻

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