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Cassini Data Reveal Enceladus Is Venting Heat From Both Poles, Bolstering Case for a Long-Lived Ocean

The global heat-loss estimate of about 54 gigawatts closely matches tidal heating predictions.

Overview

  • A reanalysis of Cassini's Composite Infrared Spectrometer data detected the north pole about 7 K warmer than seasonal models, indicating significant internal heat flow.
  • Comparing winter 2005 and summer 2015 observations, researchers inferred a conductive heat loss of roughly 35 GW from the surface, with a moonwide total near 54 GW when the south-pole output is included.
  • The measured heat-loss budget aligns with tidal heating from Saturn's gravity, supporting the persistence of Enceladus's subsurface ocean over geological timescales.
  • Thermal data yield new ice-thickness estimates of about 20–23 km at the north pole and a global average of 25–28 km, informing designs for future landers or probes.
  • Scientists highlight the unknown age of the ocean as the key open question for habitability studies, with authors Georgina Miles and Carly Howett underscoring the need for targeted missions.