Enough water to completely cover Mars may lie 11.5 to 20 kilometers below the surface, a depth warm enough for liquid water with the potential to support microbial life, according to seismic data collected by NASA’s now-retired robotic InSight lander and published in the Proceedings of the National Academy of Sciences. Measurements of seismic wave speed and gravity, combined with rock physics models, indicate the water is in fractures of igneous rocks.
Full Story: Reuters (8/12)
This water is deep but the article states that there’s more accessible water as ice at lesser depths
WASHINGTON, Aug 12 (Reuters) – An immense reservoir of liquid water may reside deep under the surface of Mars within fractured igneous rocks, holding enough to fill an ocean that would cover the entire surface of Earth’s planetary neighbor.
That is the conclusion of scientists based on seismic data obtained by NASA’s robotic InSight lander during a mission that helped decipher the interior of Mars. The water, located about 7.2 to 12.4 miles (11.5 to 20 km) below the Martian surface, potentially offers conditions favorable to sustain microbial life, either in the past or now, the researchers said.
“At these depths, the crust is warm enough for water to exist as a liquid. At more shallow depths, the water would be frozen as ice,” said planetary scientist Vashan Wright of the University of California, San Diego’s Scripps Institution of Oceanography, lead author of the study published on Monday in the journal Proceedings of the National Academy of Sciences, opens new tab.
“On Earth, we find microbial life deep underground where rocks are saturated with water and there is an energy source,” added planetary scientist and study co-author Michael Manga of the University of California, Berkeley.
The InSight lander touched down in 2018 to study the deep interior of Mars, gathering data on the planet’s various layers, from its liquid metal core to its mantle and its crust. The InSight mission ended in 2022.
“InSight was able to measure the speed of seismic waves and how they change with depth. The speed of seismic waves depends on what the rock is made of, where it has cracks and what fills the cracks,” Wright said. “We combined the measured seismic wave speed, gravity measurements and rock physics models. The rock physics models are the same as the ones we use to measure properties of aquifers on Earth or map oil and gas resources underground.”
The data indicated the presence of this reservoir of liquid water within fractured igneous rocks – formed in the cooling and solidification of magma or lava – in the Martian crust, the planet’s outermost layer.
“A mid-crust whose rocks are cracked and filled with liquid water best explains both seismic and gravity data,” Wright said. “The water exists within fractures. If the InSight location is representative and you extract all the water from the fractures in the mid-crust, we estimate that the water would fill a 1-2 km deep (0.6-1.2 miles) ocean on Mars globally.”
The Martian surface is cold and desolate today but once was warm and wet. That changed more than 3 billion years ago. The study suggests that much of the water that had been on the Martian surface did not escape into space, but rather filtered down into the crust.
“Early Mars had liquid water on its surface in rivers, lakes and possibly oceans. The crust on Mars could also have been full of water from very early in its history, too,” Manga said. “On Earth, groundwater underground infiltrated from the surface, and we expect this to be similar to the history of water on Mars. This must have occurred during a time when the upper crust was warmer than it is today.”
Water would be a vital resource if humankind ever is to place astronauts on the Martian surface or establish some sort of long-term settlement. Mars harbors water in the form of ice at its polar regions and in its subsurface. But the depth of the apparent underground liquid water would make it difficult to access.
“Drilling to these depths is very challenging. Looking for places where geological activity expels this water, possibly the tectonically active Cerberus Fossae (a region in the northern hemisphere of Mars), is an alternative to looking for deep liquids,” Manga said, though he noted that concerns about protecting the Martian environment would need to be addressed.
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Reporting by Will Dunham, Editing by Rosalba O’Brien
