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Cosmic Rays Can Sustain Subsurface Life in New Radiolytic Habitable Zone

Scientists have introduced the Radiolytic Habitable Zone to guide missions toward underground water on Mars or icy moons in search of life.

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Overview

  • High-energy cosmic rays break apart subsurface water or ice through radiolysis, releasing electrons that could power microbial metabolism in dark, cold environments.
  • The Radiolytic Habitable Zone concept extends habitability criteria beyond surface liquid water by focusing on underground reservoirs energized by cosmic radiation.
  • Computer simulations show Saturn’s moon Enceladus offers the greatest radiolytic energy potential, with Mars ranked second and Jupiter’s moon Europa third.
  • Publication in the International Journal of Astrobiology cements radiolysis by cosmic rays as a viable energy mechanism and challenges the need for sunlight or geothermal heat.
  • Researchers recommend that future missions carry instruments capable of detecting chemical energy signatures produced by cosmic-ray interactions beneath planetary surfaces.