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Heat from Saturn’s moon Enceladus reveals a stable, active ocean with potential for life.
Heat escaping from Enceladus, Saturn’s moon, indicates a stable subsurface ocean and ongoing geological activity, driven by tidal forces from Saturn.
Data from NASA’s Cassini mission show heat emission not only at the south pole—where plumes of water vapor and organic material erupt—but also from the north pole, suggesting a uniformly heated ocean.
This stability over long timescales, along with hydrothermal activity and chemical energy sources, makes Enceladus a leading candidate in the search for extraterrestrial life.
Future missions by NASA and the European Space Agency aim to study the plumes directly.
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El calor de la luna de Saturno, Encélado, revela un océano estable y activo con potencial para la vida.