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This HiRISE image from NASA's Mars Reconnaissance Orbiter shows a central crater on Mars with two dagger-like features extending at an angle. Called scimitars, these features most likely resulted from shockwave interference just before impact, scientists say.
(Image credit: NASA/JPL-Caltech/The University of Arizona)
As meteorites careen toward the surface of Mars, they can trigger avalanches before they even hit the ground, a new study suggests.
Space rocks flying toward the Martian surface can travel at several times the speed of sound, creating shockwaves in the air. These shockwaves pummel the ground, kicking up dust that rolls over slopes in dark streaks that can be seen from orbit, scientists say.
"We expected that some of the streaks of dust that we see on slopes are caused by seismic shaking during impact," said University of Arizona undergraduate student Kaylan Burleigh, who led the research project, in a statement. "We were surprised to find that it rather looks like shockwaves in the air trigger the avalanches even before the impact."
Martian terrain with dark streaks interpreted as avalanches blasted by shockwaves from a meteorite impact are visible in this photo from NASA's Mars Reconnaissance Orbiter.
(Image credit: NASA/JPL-Caltech/The University of Arizona)
Burleigh and other researchers analyzed dark streaks seen in images from NASA's Mars Reconnaissance Orbiter, and found that many did not fit the pattern expected if they were caused by the seismic shaking produced by the impact of a space rock. Instead, these streaks bore signatures of shockwaves that would have been created before any impact occurred.
Indeed, when the scientists used a computer model to simulate the geologic features expected from such shockwaves, they found characteristic curved marks, called scimitars, exactly matching those seen on the surface of Mars.
"Those scimitars tipped us off that something other than seismic shaking must be causing the dust avalanches," Burleigh said.
Mars is regularly barraged with meteorite impacts. The planet's thin atmosphere is 100 times less dense than that of Earth and cannot shield the surface from even small space rocks.
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On average, scientists spot about 20 new impact craters between 3 and 165 feet (1 and 50 meters) wide every year.
"This is one part of a larger story about current surface activity on Mars, which we are realizing is very different than previously believed," said Alfred McEwen, principal investigator of the HiRISE (High Resolution Imaging Science Experiment) camera on the Mars Reconnaissance Orbiter, and one of the co-authors of the new study. "We must understand how Mars works today before we can correctly interpret what may have happened when the climate was different, and before we can draw comparisons to Earth."
This story was provided by SPACE.com, a sister site to LiveScience. You can follow SPACE.com assistant managing editor Clara Moskowitz on Twitter @ClaraMoskowitz. Follow SPACE.com for the latest in space science and exploration news on Twitter @Spacedotcomand on Facebook.
Clara has a bachelor's degree in astronomy and physics from Wesleyan University, and a graduate certificate in science writing from the University of California, Santa Cruz. She has written for both Space.com and Live Science.
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