Subsurface Water on Mars

An artist illustration of the InSight lander on Mars. InSight, short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, is designed to give the Red Planet its first thorough check-up since it formed 4.5 billion years ago. Credit: NASA/JPL-Caltech

Physics connects seismic data to properties of rocks and sediments.

A new analysis of seismic data from NASA’s Mars InSight mission has uncovered a couple of big surprises.

The first surprise: the top 300 meters (1000 feet) of the subsurface beneath the landing site near the Martian equator contains little or no ice.

“We find that Mars’ crust is weak and porous. The sediments are not well-cemented. And there’s no ice or not much ice filling the pore spaces,” said geophysicist Vashan Wright of Scripps Institution of Oceanography at the University of California San Diego. 

Wright and three co-authors published their analysis on August 9, 2022, in the journal Geophysical Research Letters.“These findings don’t preclude that there could be grains of ice or small balls of ice that are not cementing other minerals together,” said Wright. “The question is how likely is ice to be present in that form?”

The second surprise contradicts a leading theory about what happened to the water on Mars. It is believed the red planet may have harbored oceans of water early in its history. Many experts suspected that much of that water became part of the minerals that make up underground cement.  READ MORE...