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Lab Simulations Show Trapped Vapor Cracks Ice to Propel Cryovolcanism on Europa and Enceladus

By overturning earlier models of ice sealing, the study offers radar-based methods for mapping ancient eruptions on icy moons.

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An artist's impression of NASA's Cassini flying through Enceladus' plumes.
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Overview

  • Researchers from the University of Sheffield, the Open University and the Czech Academy of Sciences used the 'George' chamber to replicate vacuum-like conditions on Europa and Enceladus.
  • They found that under near-zero pressure water boils and freezes simultaneously, creating a thin, porous ice crust.
  • Trapped vapor beneath this crust repeatedly builds pressure, cracks the ice and drives liquid water to seep onto the surface in cycles.
  • The results, published in Earth and Planetary Science Letters, challenge earlier studies that predicted a thick ice layer would seal off subsurface water and halt cryovolcanic processes.
  • The team is now exploring radar detection of vapor-induced surface irregularities as a method to locate ancient cryovolcanic sites on icy moons.