Scientists have uncovered strange ridge networks on Mars using images from spacecraft orbiting the Red Planet over the previous two decades. How and why the ridges formed, as well as what clues they may reveal about the history of Mars have remained unknown.
Aditya Khuller of Arizona State University’s School of Earth and Space Exploration and Laura Kerber of NASA’s Jet Propulsion Laboratory led a team of scientists that set out to discover more about these Martian ridges by surveying a broad region of Mars with the participation of thousands of citizen scientists.
Their findings, which have been recently published in the journal Icarus, show that the ridges on Mars may hold fossilized records of ancient groundwater flowing through them.
How the ridge networks were formed on Mars has remained a mystery ever since they were discovered in orbital imagery. Scientists have determined that there are three stages that were involved to create the ridges, including polygonal fracture formation, fracture filling, and finally erosion, which revealed the ridge networks.
To learn more about these ridges, the team combined data from the NASA Mars Odyssey orbiter’s THEMIS camera and the Mars Reconnaissance orbiter’s CTX and HiRISE instruments. Then, they deployed their citizen scientist project using the platform Zooniverse.
Nearly 14,000 citizen scientists from around the world joined in the search for the ridge networks on Mars, focusing on an area around Jezero Crater, where NASA’s Perseverance rover landed last February. Ultimately, with the help of the citizen scientists, the team was able to map the distribution of 952 polygonal ridge networks in an area that measures about a fifth of Mars’ total surface area.
“Citizen scientists played an integral role in this research because these features are essentially patterns at the surface, so almost anyone with a computer and internet can help identify these patterns using images of Mars,” Khuller said.
Most of the ridge networks (91%, or 864 out of 952) that were analyzed are located in ancient, eroded terrain that is approximately 4 billion years old. During this time period, Mars is believed to have been warmer and wetter, which might be related to how these ridges form.
Previous research in this area has shown that those ridges which were not covered with layers of dust showed spectral signatures of clays. Since clays form from weathering in the presence of water, this suggested to the research team that the ridges may have been formed by groundwater. While the abundant surface dust in these regions makes it difficult to check whether the newly mapped ridge networks by Khuller and Kerber’s team also contain clays, their similarities in shape and dimension suggest that they might form from similar groundwater processes.
This discovery helps scientists “trace” the footprints of groundwater running through the ancient Martian surface and determine where it was suitable, during that time 4 billion years ago, for liquid water to be flowing near the surface.
“We hope to eventually map the entire planet with the help of citizen scientists,” Khuller said. “If we are lucky, the Mars 2020 Perseverance rover might be able to confirm these findings, but the nearest set of ridges is a few kilometers away, so they might only be visited on a potential extended mission.”
Reference: “Irregular polygonal ridge networks in ancient Noachian terrain on Mars” by Aditya R. Khuller, Laura Kerber, Megan E. Schwam, Sylvia Beer, Fernando E. Nogal, Ray Perry, William Hood, Klaus-Michael Aye, Ganna Portyankin and Candice J. Hanseng, 3 December 2021, Icarus.
Additional authors on this study include Megan Schwamb of Queen’s University Belfast; Fernando Nogal, Sylvia Beer, Ray Perry and William Hood of the Planet Four: Ridges Citizen Science Team; Klaus-Michael Aye and Ganna Portyankina of the University of Colorado, Boulder; and Candice Hansen of the Planetary Science Institute.