Mars Gullies Linked to Carbon Dioxide, not Water
Dune gullies in the Matara Crater on Mars change year after year: Between 2008 and 2010 (top to bottom), the alcoves at the dune’s crest and the channel beds widened during the Martian winter as material moved down the slope. New deposits are visible in the bottom image as the darker material extending from the channels. Material can be seen filling the down-slope portion of the upper channel, only to be carved out the following year. Credit: NASA/JPL-Caltech/The University of Arizona
A growing bounty of images from NASA’s Mars Reconnaissance Orbiter reveals that the timing of new activity in a type of gully on Mars implicates carbon dioxide frost, rather than water, as the agent causing fresh flows. Because life as we know it requires liquid water, determining whether or not the gullies were formed by water has important implications in the search for signs of past or present life on Mars.
Researchers have tracked changes in gullies on the faces of sand dunes in seven locations on southern Mars. The periods when changes occurred, as determined by comparisons of before-and-after images, overlapped in all cases with the known winter build-up of carbon-dioxide frost on the dunes. Before-and-after pairs that covered periods only in spring, summer and autumn showed no new activity in those seasons.
The findings will published in the article, “Seasonality of present-day martian dune-gully activity,” in the November issue of the journal Geology.
“Gullies that look like this on Earth are caused by flowing water, but Mars is a different planet with its own mysteries,” said lead author Serina Diniega, who graduated from the University of Arizona this summer with a doctorate in applied mathematics and a minor in planetary science. “The timing we see points to carbon dioxide, and if the mechanism is linked to carbon-dioxide frost at these dune gullies, the same could be true for other gullies on Mars.”
Scientists have suggested various explanations for modern gullies on Mars since fresh-looking ones were discovered in images from NASA’s Mars Global Surveyor in 2000. Some of the proposed mechanisms involve water, some carbon dioxide and some neither.
Some fresh gullies are on sand dunes, commonly starting at a crest. Others are on rockier slopes, such as the inner walls of craters and sometimes starting partway down the slope.
Diniega and UA co-authors Shane Byrne, Colin Dundas and Alfred McEwen, together with Nathan Bridges at Johns Hopkins University Applied Physics Laboratory in Laurel, Md., focused their study on dune gullies that are shaped like slope gullies, with an alcove at the top, a channel or multiple channels in the middle, and an apron at the bottom. The 18 dune gullies in which the researchers observed new activity ranged in size from about 50 meters or yards long to more than 3 kilometers (2 miles) long.
“The alcove is a cutout at the top,” Diniega said. “Material being removed from there ends up in a fan-shaped apron below.”
The gullies on a Martian sand dune resemble features on Earth that are carved by streams of water. However, these gullies likely owe their existence to entirely different geological processes apparently related to the winter buildup of carbon-dioxide frost. Image Credit: NASA/JPL-Caltech/University of Arizona
Because new flows in these gullies apparently occur in winter, rather than at a time when any frozen water might be most likely to melt, the new report calls for studies of how carbon dioxide, rather than water, could be involved in the flows. Some carbon dioxide from the martian atmosphere freezes on the ground during winter and sublimates back to gaseous form as spring approaches. The dunes studied are poleward of 40 degrees south latitude.
“One possibility is that a pile of carbon-dioxide frost accumulating on a dune gets thick enough to avalanche down and drag other material with it,” Diniega said. Other suggested mechanisms are that gas from sublimating frost could lubricate a flow of dry sand or erupt in puffs energetic enough to trigger slides.
The new report uses images from the Mars Orbiter Camera on Mars Global Surveyor, which operated from 1997 to 2006, and from the High Resolution Science Imaging Experiment, or HiRISE, camera and Context Camera on the Mars Reconnaissance Orbiter, which has been examining Mars since 2006.
“The Mars Reconnaissance Orbiter is enabling valuable studies of seasonal changes in surface features on Mars,” said Sue Smrekar of NASA’s Jet Propulsion Laboratory and deputy project scientist for this orbiter. “One key to doing that has been the capability to point from side to side, so that priority targets can be checked more frequently than just when the spacecraft flies directly overhead,” she said. “Another is the lengthening span of years covered by first Mars Global Surveyor, and now this mission.”