Researchers analyzing seismic data from NASA’s InSight lander have discovered evidence of a massive liquid water reservoir deep within the Martian crust. Located between 7 and 13 miles underground, the volume of water is estimated to be sufficient to cover the entire planet in a shallow ocean.
TLDR: Scientists have identified a vast reservoir of liquid water deep in the Martian mid-crust using seismic data from the InSight lander. This discovery suggests that Mars’s ancient water migrated underground rather than escaping into space, though the depth makes it currently inaccessible for human use.
Researchers at the University of California, Berkeley, have identified a vast reservoir of liquid water trapped deep within the rocky outer crust of Mars. This discovery, based on a sophisticated re-examination of data from NASA’s retired InSight lander, suggests that the Red Planet’s ancient oceans did not simply evaporate into space but may have filtered down into the subsurface over billions of years. The findings provide a new perspective on the geological evolution of Mars and its potential to harbor life.
The research team utilized seismic measurements recorded by the InSight lander’s seismometer between 2018 and 2022. During its mission, the lander recorded over 1,300 “marsquakes,” which sent vibrations through the planet’s interior. By applying rock physics models similar to those used on Earth to map underground oil fields and deep aquifers, the scientists analyzed the speed and behavior of these seismic waves. These waves travel at different velocities depending on the density, temperature, and state of the material they pass through, allowing the team to distinguish between solid rock, gas, and liquid. Specifically, the researchers looked at how the velocity of primary P-waves and secondary S-waves changed as they penetrated the crust, providing a detailed map of the planet’s internal composition.
The data indicates a layer of fractured igneous rock, likely granite or basalt, saturated with liquid water. This reservoir is located in the mid-crust, between 11.5 and 20 kilometers beneath the Martian surface. The volume of water contained within these deep pores is staggering; the researchers estimate it is enough to cover the entire planet in an ocean more than a kilometer deep. This suggests that the mid-crust contains more water than the volumes proposed to have filled hypothesized ancient Martian oceans. The presence of liquid water at these depths requires specific temperature and pressure conditions, which the study suggests are maintained by the planet’s internal heat.
For decades, planetary scientists have debated the fate of Mars’s surface water, which disappeared roughly three billion years ago. While much of the water was thought to have been lost to space after the planet lost its magnetic field, this study supports the theory that a significant portion was sequestered within the crust. On Earth, groundwater is a critical component of the hydrological cycle, and these findings suggest Mars may possess a similarly complex, albeit much deeper, system.
The depth of this reservoir presents significant challenges for future human exploration and colonization. Drilling several miles into the Martian crust exceeds current technological capabilities and would require massive energy resources. Consequently, this water is not an immediate resource for future astronauts. However, the discovery shifts the focus of the search for life. On Earth, deep subsurface environments often harbor microbial life where water and chemical energy sources are present, suggesting that the Martian mid-crust could be a long-term habitable zone.
Future missions may focus on identifying specific regions where the crustal structure allows for easier access or investigating the chemical composition of the minerals surrounding the water. Understanding the distribution and salinity of this water is essential for reconstructing the history of Mars and determining if the planet ever hosted life. This discovery marks a pivotal moment in planetary science, transforming the image of Mars from a desiccated desert into a world with a hidden, watery interior. Scientists are now considering how this subsurface water might interact with the surface through volcanic activity or tectonic shifts, potentially creating transient habitable environments.

