Slope Streaks on Mars – Not A Sign Of Water After All?
A new study led by the University of Bern and Brown University in the U.S. casts doubt on one of the most tantalizing clues that water might be flowing on present-day Mars. Researchers analyzed a global database of 500,000 enigmatic streaks that occur on steep Martian slopes, concluding that they’re most likely caused by dry processes rather than liquid flow.
For years, scientists have spied strange streaks running down Martian cliffsides and crater walls. Some have interpreted those streaks as liquid flows, suggesting the possibility of currently habitable environments on the Red Planet. But this new study, which used machine learning to create and analyze a massive dataset of slope streak features, points to a different explanation: dry process related to wind and dust activity.
“A big focus of our research is understanding modern-day processes on Mars — including the possibility of liquid water on the surface,” said Valentin Bickel, a planetary scientist at the Center for Space and Habitability (CSH) at the University of Bern who authored the research with Adomas Valantinas, a former postdoctoral researcher in the Space Research and Planetary Sciences Division (WP) at the Institute of Physics at the University of Bern, and now at Brown University. “Our study reviewed these features but found no evidence of water. Our model favors dry formation processes. ”The research was published in Nature Communications on Monday, May 19.
Origin of slope streaks intensively debated
Scientists first saw the odd streaks in images returned from NASA’s Viking mission in the 1970s. The sinewy features are generally darker in hue than the surrounding terrain and extend for hundreds of meters down sloped terrain. Some last for years or decades, while others come and go more quickly. The shorter-lived features — dubbed recurring slope lineae (RSL) — seem to show up in the same locations during the warmest periods of the Martian year.
The origin of the streaks has been a hot topic among planetary scientists. Modern Mars is remarkably dry, and temperatures rarely peak above freezing. Still, it’s possible that small amounts of water — perhaps sourced from buried ice, subsurface aquifers or abnormally humid air — could mix with enough salt to create a flow even on the frozen Martian surface. If true, RSLs and slope streaks could mark rare, habitable niches on a desert world.
Other researchers haven’t been convinced. They contend the streaks are triggered by dry processes like rock falls or wind gusts, and only appear liquid-like in orbital images.
A through C: CaSSIS (Colour and Stereo Surface Imaging System89) and HiRISE color-infrared images of bright and dark slope streaks, as well as RSL; downslope direction is always pointing down- or side-wards; image IDs MY36_014887_165_0, MY36_014975_168_0, MY35_009504_159_0, MY35_010269_009_0, ESP_022689_1380, ESP_034830_1670. Raw image credits ESA/TGO/CaSSIS CC-BY-SA 3.0 IGO and NASA/MRO/UoA. D) through F): Maps of slope streak (bright, white; dark, black) and RSL (red) distribution (e.g. refs. 8,51) as well as bright-to-dark slope streak ratio per 10° by 10° quadrangle, overlain on a Viking merged color mosaic and MOLA topography81. Percentages of total population per streak hotspot indicated on the map. Our results agree well with earlier maps of streak-bearing regions3,5, while identifying a series of previously unknown streak hotspots, e.g. in Xanthe Terra and Lunae Planum (Supplementary Fig. S2). — Nature
New insights through machine learning
Hoping for new insights, Bickel and Valantinas turned to a machine learning algorithm to catalog as many slope streaks as they could. After training their algorithm on confirmed slope streak sightings, they used it to scan more than 86,000 high-resolution satellite images. The result was a first-of-its-kind global Martian map of slope streaks containing more than 500,000 streak features.
“Once we had this global map, we could compare it to databases and catalogs of other things like temperature, wind speed, hydration, rock slide activity and other factors.” Bickel said. “Then we could look for correlations over hundreds of thousands of cases to better understand the conditions under which these features form.”
This geostatistical analysis showed that slope streaks and RSLs are not generally associated with factors that suggest a liquid or frost origin, such as a specific slope orientation, high surface temperature fluctuations or high humidity. Instead, the study found that both features are more likely to form in places with above average wind speed and dust deposition — factors that point to a dry origin.
The researchers conclude that the streaks most likely form when layers of fine dust suddenly slide off steep slopes. The specific triggers may vary. Slope streaks appear more common near recent impact craters, where shockwaves might shake loose surface dust. RSLs, meanwhile, are more often found in places where dust devils or rockfalls are frequent.
Impact on future Mars missions
Taken together, the results cast new doubt on slope streaks and RSLs as habitable environments.
That has significant implications for future Mars exploration. While habitable environments might sound like good exploration targets, NASA and ESA would rather keep their distance. Any Earthly microbes that may have hitched a ride on a spacecraft could contaminate habitable Martian environments, complicating the search for Mars-based life. This study suggests that the contamination risk at slope streak sites isn’t much of a concern.
“That’s the advantage of this big data approach,” Valantinas said. “It helps us to rule out some hypotheses from orbit before we send spacecraft to explore.”
Streaks on martian slopes are dry, Nature, (Open access)
Astrobiology
