Enceladus has a warm heart

Until recently, active volcanism was known to exist only on two planets, Venus and Earth, and on Jupiter’s moon Io. However, it has now been confirmed that Enceladus, a moon of Saturn, also exhibits this phenomenon.
 
This satellite orbits Saturn at a distance of 238,040 km, doing so synchronously (always showing the same face) in 32.9 hours. It is nearly spherical, with a diameter of 499 km, and its icy surface displays remarkable diversity: some regions are almost smooth, devoid of geological features, while others show fracture lines from tectonic activity, and still others are dotted with impact craters. The most striking feature, however, lies at its South Pole.
 
There, scientists have identified what they’ve dubbed “tiger stripes”—grooves stretching 130 km long, 2 km wide, and 500 meters deep. From these, massive jets of water vapor, solid materials like sodium chloride crystals and ice, volatile compounds, and—surprisingly—organic material are continuously ejected into space at a rate of up to 200 kg per second. The Cassini spacecraft, which explored this moon, detected over 100 such geysers, confirming the presence of an internal heat source. The concentration of this activity at the South Pole may be due to centrifugal forces pushing denser material toward the equator and lighter material toward the poles. Some of the expelled water vapor falls back as snow, while the rest escapes, contributing to Saturn’s outermost and faintest E ring, within which Enceladus orbits.
 
This internal heat source drives volcanoes and hydrothermal vents, similar to those found on Earth’s ocean floors. Beneath its icy surface, Enceladus harbors a liquid water ocean about 30 km deep and 10 km thick, situated above its central core. Yet, there may be additional, unknown heat sources at play. For instance, Enceladus is in an orbital resonance with its neighboring moon Dione (completing two orbits around Saturn for every one of Dione’s), which helps maintain its orbital eccentricity and generates extra heat through geological activity. Between these factors, scientists are left astounded—especially upon discovering that the heat output at the South Pole reaches nearly 16 million watts, ten times higher than previously estimated, with no clear explanation yet uncovered.
 
At the surface, Enceladus is blanketed in ice, with an average temperature of -198°C. This varies by location and time, ranging from -240°C to -128°C—except, of course, in the South Pole regions where the constant geysers emerge.
 
Its atmosphere consists of water vapor (91%), nitrogen (4%), carbon dioxide (3.2%), and methane (1.7%). This composition, along with its subsurface ocean and hydrothermal activity, has sparked significant scientific interest, positioning Enceladus as one of the most promising locations in our solar system for potential life, particularly near its hydrothermal vents.
 

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