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New Radiolytic Habitable Zone Validates Potential for Underground Life on Mars and Icy Moons

This paradigm shift directs future missions to probe beneath icy crusts or dusty Martian ice for chemical-energy signatures rather than relying on surface biosignatures

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Overview

  • Researchers at NYU Abu Dhabi introduce the Radiolytic Habitable Zone to encompass subsurface water environments energized by cosmic rays across the solar system.
  • Advanced simulations rank Saturn’s moon Enceladus as the top candidate for radiolysis-supported metabolism, followed by Mars and then Jupiter’s moon Europa based on relative energy yields.
  • Cosmic-ray interactions with underground water or ice drive radiolysis, releasing electrons that could power microbial life in cold, dark niches.
  • The framework overturns the longstanding view that extraterrestrial life requires sunlight or geothermal heat by highlighting chemical-energy sources beneath planetary surfaces.
  • Investigators urge future exploration missions to carry subsurface probes with sensors designed to detect radiolytic chemical energy instead of focusing solely on surface biosignatures.