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Reanalysis of Magellan Data Points to Kilometer-Scale Lava Tube Beneath Venus

Researchers say higher-resolution radar from EnVision and VERITAS is needed to verify the radar-inferred cavern.

Overview

  • The peer-reviewed study in Nature Communications reexamines 1990–1992 radar images from NASA’s Magellan orbiter.
  • Scientists from the University of Trento report skylight-style collapse features in the Nyx Mons region consistent with a subsurface lava tube.
  • The inferred tunnel is estimated at roughly 1 kilometer in diameter with a roof at least 150 meters thick and an interior height near 375 meters.
  • Radar signatures indicate the detectable cavity continues at least 300 meters below the surface, with additional collapses suggesting possible channels extending about 45 kilometers, a hypothesis still unverified.
  • Venus’s extreme heat and pressure preclude optical imaging, making radar the principal tool until future missions can map and confirm any subsurface channels.