The Curiosity rover has studied a network of Martian “webs” — structures formed by ancient underground water. This raises the question once again of whether life could have existed on the Red Planet.

Panorama showing the Boxwork ridges on Mars.
Source: NASA/JPL-Caltech/MSSS

One of the distinctive features of Mars are geological formations called “boxworks,” which look like giant spider webs from space. They are low ridges stretching for many kilometers, with heights ranging from 1 to 2 meters, with sandy depressions between them.

To explain their shape, scientists have hypothesized that underground water once flowed through large cracks in the bedrock, leaving minerals behind. These minerals then reinforced the areas that became ridges, while other areas that did not have mineral reinforcement were eroded over time.

Martian “highway”

However, until recently, this was only a hypothesis. Although boxwork ridges also exist on Earth, they rarely exceed a few centimeters in height and are usually found in caves or dry sandy environments. To reveal the nature of these formations, it was necessary to examine them closely.

Selfie taken by the Curiosity rover.
Source: NASA/JPL-Caltech/MSSS

The Curiosity rover was used to solve this problem, which proved to be a real challenge for the team controlling it. They needed to plan the route for the 900-kilogram rover so that it could travel along the tops of ridges whose width was not much greater than the rover’s own width. 

“It almost feels like a highway we can drive on. But then we have to go down into the hollows, where you need to be mindful of Curiosity’s wheels slipping or having trouble turning in the sand,” said Ashley Stroup, an operations systems engineer at NASA’s Jet Propulsion Laboratory. “There’s always a solution. It just takes trying different paths.”

Water on Mars

Orbital images of the boxwork showed characteristic dark lines. In 2014, it was suggested that there were cracks in the rocks where groundwater seeped in and allowed minerals to concentrate. After examining the ridges up close, Curiosity confirmed that these lines are indeed cracks.

These bumpy nodules formed from minerals left behind after groundwater on Mars dried up billions of years ago.
Source: NASA/JPL-Caltech/MSSS

The rover also discovered irregular formations called nodules, which are a clear sign of the presence of underground water in the past. Unexpectedly, these nodules were found not near the central cracks, but along the walls of the ridges and in the depressions between them.

This discovery is particularly important given the geography of the region. Curiosity is climbing the slope of the 5-kilometer-high Mount Sharp. Each layer was formed during different geological eras. The higher Curiosity climbs, the more signs of alternating periods of water drying up and wet periods with rivers and lakes appear in the landscape.

“Seeing boxwork this far up the mountain suggests the groundwater table had to be pretty high,” said Tina Seeger of Rice University in Houston, one of the mission scientists leading the boxwork research. “And that means the water needed for sustaining life could have lasted much longer than we thought looking from orbit.”

Sometime in March, Curiosity will leave the boxwork and begin studying the sulfate layer covering Mount Sharp. It consists of salt minerals formed as a result of water drying up. Studying it will help us learn even more about what the climate of the Red Planet was like billions of years ago.