Saturn Moon Enceladus May Harbor Stable Ocean for Life
Heat flow from Enceladus' subsurface ocean remains stable, matching tidal heating inputs and supporting the moon's potential to sustain life, researchers found.
- On November 7, 2025, the study published in Science Advances showed Oxford University, Southwest Research Institute, and Planetary Science Institute found strong heat flow at Enceladus' north pole.
- Comparing Cassini's 2005 and 2015 infrared observations showed Saturn's gravity flexes Enceladus each orbit, producing tidal heating that supplies internal heat.
- Infrared analysis yields quantitative heat-flow figures such as the north polar surface being about 7 K warmer than models predicted, measured heat flow 46 milliwatts per square meter, and conductive heat loss ~35 gigawatts.
- Matching totals show Enceladus loses 54 gigawatts total heat loss, aligning with tidal heating and supporting a stable subsurface ocean over geological timescales.
- With missions under consideration in the 2040s, ESA plans to study ice thickness, which ranges from 20 to 23 kilometers at the north pole and 25 to 28 kilometers globally, while scientists say determining how long the ocean has persisted is the next challenge.
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Study says that Encelado is emitting much more heat than would be expected if it were simply a passive body, which reinforces the possibility that he could endure life as it is known.
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Saturn’s icy moon may host a stable ocean fit for life, study finds
New findings from NASA’s Cassini mission show that Enceladus, one of Saturn’s moons and a top contender for extra-terrestrial life, is losing heat from both poles – indicating that it has the long-term stability required for life to develop. The findings have been published today (7 November) in Science Advances.
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