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New Study Links Ancient Martian Valleys to Rain and Snow

Digital modeling and rover data suggest precipitation, rather than ice melt, shaped Mars' valleys during its Noachian epoch.

An artist's depiction of water rushing into Mars' Jezero Crater (Credit: NASA/JPL-Caltech)
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Overview

  • Researchers used digital simulations to compare precipitation and ice-melt scenarios for Mars' ancient valley networks.
  • The precipitation model aligned more closely with observed valley head elevations, suggesting widespread rain and snow billions of years ago.
  • NASA's Perseverance rover found evidence in Jezero Crater, such as large boulders, that indicates meters-deep flowing water shaped the landscape.
  • The study, published in the Journal of Geophysical Research: Planets, highlights similarities between Mars' wet past and early Earth’s environment.
  • Questions remain about how Mars sustained warm, wet conditions under a faint young Sun, leaving the climate debate unresolved.