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- Saturn\u2019s moon Enceladus has a salty, global subsurface ocean<\/strong> similar to Earth\u2019s oceans. Is it habitable? Could there actually be life there?<\/li>\n
- Enceladus\u2019 ocean is likely stable enough to support life,<\/strong> a new analysis of Cassini data showed.<\/li>\n
- Scientists measured heat flow at the moon\u2019s north pole<\/strong> for the 1st time. This heat loss at both poles is evidence that the ocean is stable over long geological time periods.<\/li>\n<\/ul>\n
Millions come to EarthSky for night sky news and trusted science.<\/strong>
Your donation keeps us free and accessible for all.<\/p>\nA stable, habitable ocean on Enceladus?<\/h3>\n
Scientists have found yet more evidence that the subsurface ocean on Saturn\u2019s moon Enceladus might be habitable. Researchers from the University of Oxford, Southwest Research Institute (SwRI) in Texas and the Planetary Science Institute (PSI) in Arizona said on November 10, 2025, that they have confirmed heat flow at the moon\u2019s north pole, not just the south pole as first thought. This indicates that Enceladus is generating a lot more heat inside than previously known. This suggests the ocean has been stable over the long term geologically. It\u2019s an exciting new finding hinting at how this alien ocean just might be home for some form of life<\/em>.<\/p>\n
The researchers used data from the now-finished Cassini mission for their new study.<\/p>\n
Previously, scientists thought heat was escaping into space only from Enceladus\u2019 south pole. That is where the huge water vapor plumes erupt from long cracks in the icy surface called tiger stripes. NASA\u2019s Cassini spacecraft previously flew through the plumes and sampled them to analyze their composition.<\/p>\n
The intriguing new peer-reviewed results were published in Science Advances<\/em> on November 7, 2025.<\/p>\n
Heat loss at Enceladus\u2019 north pole<\/h3>\n
Scientists have thought that the north pole on Enceladus was much less geologically active than its south pole. That made sense, since it\u2019s at the south pole where the tiger stripes and plumes are located. And scientists had only measured heat loss at the south pole.<\/p>\n
But now, it seems there might be some geological activity at the north pole after all. The researchers compared Cassini observations of the north polar region in deep winter (in 2005) and summer (in 2015). They then measured how much energy Enceladus loses from its \u201cwarm\u201d subsurface ocean (32 degrees Fahrenheit or 0 degrees Celsius) as heat travels through the icy outer shell to the surface (\u2013370 degrees F, or -223 degrees C) and then radiates into space.<\/p>\n
Lead author Georgina Miles at the Southwest Research Institute (SwRI) and a visiting scientist at the Department of Physics, University of Oxford, said:<\/p>\n
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Eking out the subtle surface temperature variations caused by Enceladus\u2019 conductive heat flow from its daily and seasonal temperature changes was a challenge, and was only made possible by Cassini\u2019s extended missions.<\/p>\n<\/blockquote>\n
![\"Cutaway](\"https:\/\/earthsky.org\/upl\/2025\/11\/Enceladus-heat-transfer-infographic-University-of-Oxford-November-10-2025.jpg\")
View larger. | This infographic depicts heat transfer from Enceladus\u2019 subsurface ocean, at both the north and south poles. This balance shows the ocean is stable over the long term and increases the chances of it being habitable. Image via University of Oxford\/ NASA\/ JPL-CalTech\/ Space Science Institute (PIA19656 and PIA11141).<\/figcaption><\/figure>\n ![\"Grayish](\"https:\/\/earthsky.org\/upl\/2020\/09\/Enceladus-north-pole-Cassini-Nov-27-2016-800x800.jpg\")
View larger. | A visible-light image of Enceladus\u2019 north pole, taken by Cassini on November 27, 2016. The terrain is much more cratered than in the south, but the infrared images \u2013 and the cracks in the surface seen here \u2013 show there has been at least some geological activity in the region. Image via NASA\/ JPL-Caltech.<\/figcaption><\/figure>\n North pole warmer than expected<\/h3>\n
Researchers modeled the expected surface temperatures during the polar night and compared them with infrared observations from the Cassini Composite InfraRed Spectrometer (CIRS). And \u2013 surprise \u2013 they found the surface at the north pole was about 7 Kelvin warmer than expected. According to the researchers, only heat leaking from the ocean below could explain that.<\/p>\n
The researchers measured the heat flow at 46 \u00b1 4 milliwatts per square meter. That\u2019s equivalent to 2\/3 of the heat loss (per unit area) through Earth\u2019s continental crusts. This is a total heat loss of 35 gigawatts for all of Enceladus. That equals 66 million solar panels (with an output of 530 watts) or 10,500 wind turbines (with an output of 3.4 megawatts).<\/p>\n
The results also show the ice shell thickness at the north pole to be about 12-19 miles (20-30 km). This is consistent with previous models.<\/p>\n
Interestingly, another team of researchers said in 2020 that they found evidence for plumes at Enceladus\u2019 north pole, as well. They are thought to be smaller and weaker than the ones at the south pole. But if confirmed, they would fit with the new evidence for heat leaking from the ocean at the north pole, through cracks in the ice crust.<\/p>\n
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NEW: Latest findings from NASA\u2019s Cassini mission show that Enceladus \u2013 one of Saturn\u2019s moons and a top contender for extra-terrestrial life \u2013 is losing heat from both poles, suggesting it could stay stable enough for life to form.Read more ??<\/p>\n
\u2014 University of Oxford (@ox.ac.uk) 2025-11-10T16:10:19.457171907Z<\/p>\n<\/blockquote>\n
Evidence for a stable ocean on Enceladus<\/h3>\n
The researchers then combined the heat loss at both poles for a total of about 54 gigawatts. Notably, that is close to what models predicted for heat input from tidal forces in the ocean. Why is that significant? It means there is a balance between heat production and heat loss. That would allow the subsurface ocean to remain stable for a long time.<\/p>\n
The tidal heating \u2013 caused by Saturn\u2019s gravity tugging on Enceladus \u2013 would maintain this balance. This is important. If the ocean doesn\u2019t gain enough energy, it would eventually freeze solid. If there\u2019s too much energy, however, then that could alter the chemistry of the ocean, perhaps making it less habitable.<\/p>\n
![\"Smiling](\"https:\/\/earthsky.org\/upl\/2025\/11\/Georgina-Miles-Southwest-Research-Institute.jpeg\")
Georgina Miles at the Southwest Research Institute (SwRI) is the lead author of the new study about heat loss and the habitability of Enceladus\u2019 subsurface ocean. Image via ResearchGate.<\/figcaption><\/figure>\n Enceladus: An abode of life?<\/h3>\n
The evidence has mounted in recent years that Enceladus\u2019 ocean is potentially habitable. Cassini found all of the necessary ingredients in the water vapor plumes, including complex organics and phosphorous. The ocean is also salty, but not too<\/em> salty. There is also evidence for hydrothermal activity \u2013 hydrothermal vents \u2013 on the ocean floor, much like in Earth\u2019s oceans.<\/p>\n
But more study is needed, including from future missions going back to Enceladus. And as with Cassini, it can take many years to go through all of the data. As Miles noted:<\/p>\n
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Our study highlights the need for long-term missions to ocean worlds that may harbor life, and the fact the data might not reveal all its secrets until decades after it has been obtained.<\/p>\n<\/blockquote>\n
Bottom line: The subsurface ocean on Enceladus is stable enough for life, a new study of data from the Cassini mission suggests. Heat flow at both poles provides the clues.<\/p>\n
Source: Endogenic heat at Enceladus\u2019 north pole<\/p>\n
Via University of Oxford<\/p>\n
Read more: Do the organics in Enceladus\u2019 ocean point to habitability?<\/p>\n
Read more: Enceladus\u2019 ocean even more habitable than thought<\/p>\n
<\/div>\n
\n - Enceladus\u2019 ocean is likely stable enough to support life,<\/strong> a new analysis of Cassini data showed.<\/li>\n