Researchers deduced that this process could explain one enigmatic class of gullies seen on martian sand dunes by examining images from NASA’s Mars Reconnaissance Orbiter (MRO) and performing experiments on sand dunes in Utah and California.
“I have always dreamed of going to Mars,” said lead author Serina Diniega, a planetary scientist at NASA’s Jet Propulsion Laboratory in Pasadena, California. “Now I dream of snowboarding down a martian sand dune on a block of dry ice.”
The hillside grooves on Mars, called linear gullies, show relatively constant width — up to a few yards, or meters, across — with raised banks or levees along the sides. Unlike gullies caused by water flows on Earth and possibly on Mars, they do not have aprons of debris at the downhill end of the gully. Instead, many have pits at the downhill end.
“In debris flows, you have water carrying sediment downhill, and the material eroded from the top is carried to the bottom and deposited as a fan-shaped apron,” said Diniega. “In the linear gullies, you’re not transporting material. You’re carving out a groove, pushing material to the sides.”
Images from MRO’s High Resolution Imaging Science Experiment (HiRISE) camera show sand dunes with linear gullies covered by carbon-dioxide frost during the martian winter. By comparing before-and-after images from different seasons, researchers determined that the grooves are formed during early spring. Some images have even caught bright objects in the gullies.
Scientists theorize the bright objects are pieces of dry ice that have broken away from points higher on the slope. According to the new hypothesis, the pits could result from the blocks of dry ice completely sublimating away into carbon-dioxide gas after they have stopped traveling.
That is exactly what report co-author Candice Hansen of the Planetary Science Institute in Tucson, Arizona, did. Hansen has studied other effects of seasonal carbon dioxide ice on Mars, such as spider-shaped features that result from explosive release of carbon dioxide gas trapped beneath a sheet of dry ice as the underside of the sheet thaws in spring. She suspected a role for dry ice in forming linear gullies, so she bought some slabs of dry ice at a supermarket and slid them down sand dunes.
That day and in several later experiments, gaseous carbon dioxide from the thawing ice maintained a lubricating layer under the slab and also pushed sand aside into small levees as the slabs glided down even low-angle slopes.
The outdoor tests did not simulate martian temperature and pressure, but calculations indicate that the dry ice would act similarly in early martian spring where the linear gullies form. Although water ice, too, can sublimate directly to gas under some martian conditions, it would stay frozen at the temperatures at which these gullies form, the researchers calculate.
“MRO is showing that Mars is a very active planet,” Hansen said. “Some of the processes we see on Mars are like processes on Earth, but this one is in the category of uniquely martian.”
Hansen also noted that the process could be unique to the linear gullies described on martian sand dunes.
“There are a variety of different types of features on Mars that sometimes get lumped together as ‘gullies,’ but they are formed by different processes,” she said. “Just because this dry-ice hypothesis looks like a good explanation for one type doesn’t mean it applies to others.”
