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Meteorites and marsquakes hint at an underground ocean of liquid water on the red planet

  • In 2021-2022, scientists studied vibrations recorded by NASA's InSight lander near Mars' equator and identified a slow-wave zone located between 5.4 and 8 kilometers beneath the surface.
  • This slowdown likely resulted from liquid water in porous rocks, explaining a large volume of Mars' 'missing' water not accounted for by surface ice or atmospheric loss.
  • The inferred aquifer could hold enough liquid water to cover Mars with a global ocean between 520 and 780 meters deep, several times Antarctica's ice sheet volume.
  • Co-Author Hrvoje Tkal i explained that their research suggests a significant portion of the ancient water likely seeped into the sponge-like, porous rocks beneath the surface and remained trapped underground.
  • Additional exploration involving instruments like seismometers and drilling equipment will be essential to verify these subterranean water deposits, investigate potential signs of Martian life, and evaluate their usefulness for human missions.
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Mars Daily broke the news in Australia on Sunday, May 11, 2025.
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