Recent discoveries suggest that liquid water may still exist within Mars' crust, defying earlier assumptions.
NASA's InSight mission explored the Martian subsurface using geophysical measurements to collect seismic data.
Analysis of the seismic data uncovered compelling evidence of water-saturated fractures within the mid-crust, located 11 to 20 kilometers below the surface.
Parameters of the model applied featured a Bayesian inversion model combined with rock physics theories to analyze seismic velocities and bulk density within the Martian crust.
The presence of liquid water enriches understanding of Mars climate history and serves as clues to the planet's evolutionary journey.
The discovery of liquid water on Mars--even deep underground--opens new possibilities in the search for extraterrestrial life.
Geophysical techniques used could be adapted for other planetary bodies, broadening search for life and habitable conditions beyond Earth.
International collaboration is essential to unraveling the mysteries of our solar system.
Analysis of past missions, like InSight, helps create a more comprehensive picture of Mars' geological history and its potential for supporting life.
Mars emerges as a more dynamic and potentially life-sustaining environment, bringing humanity closer to solving the mysteries of the Red Planet.