Meteorite Shock Waves Cause Dust Avalanches on Mars
“We expected that some of the streaks of dust that we see on slopes are caused by seismic shaking during impact,” said Kaylan Burleigh, who led the research project. “We were surprised to find that it rather looks like shock waves in the air trigger the avalanches even before the impact.”
Because of Mars’ thin atmosphere, which is 100 times less dense than Earth’s, even small rocks that would burn up or break up before they could hit the ground here on Earth crash into the Martian surface relatively unimpeded.
Each year, about 20 fresh craters between 1 and 50 meters (3 to 165 feet) show up in images taken by the HiRISE camera on board NASA’s Mars Reconnaissance Orbiter. The High Resolution Imaging Science Experiment, or HiRISE, is operated by the UA’s Lunar and Planetary Laboratory and has been photographing the Martian surface since 2006, revealing features down to less than 1 meter in size.
For this study, the team zoomed in on a cluster of five large craters, which all formed in one impact event close to Mars’ equator, about 825 kilometers (512 miles) south of the boundary scarp of Olympus Mons, the tallest mountain in the solar system. Previous observations by the Mars Global Surveyor orbiter, which imaged Mars for nine years until 2006, showed that this cluster was blasted into the dusty surface between May 2004 and February 2006.
The results of the research, which Burleigh first took on as a freshman under former UA Regents Professor H. Jay Melosh, are published in the planetary science journal Icarus. Previous studies had looked at dark or light streaks on the Martian landscape interpreted as landslides, but none had tied such a large number of them to impacts.
Narrow, relatively dark streaks varying from a few meters to about 50 meters in length scour the slopes around the impact site.
“The dark streaks represent the material exposed by the avalanches, as induced by the airblast from the impact,” Burleigh said. “I counted more than 100,000 avalanches and, after repeated counts and deleting duplicates, arrived at 64,948.”
When Burleigh looked at the distribution of avalanches around the impact site, he realized their number decreased with distance in every direction, consistent with the idea that they were related to the impact event.
But it wasn’t until he noticed a pair of peculiar surface features resembling a curved dagger, described as scimitars, extending from the central impact crater, that the way in which the impact caused the avalanches became evident.
“Those scimitars tipped us off that something other than seismic shaking must be causing the dust avalanches,” Burleigh said.
As a meteor screams through the atmosphere at several times the speed of sound, it creates shock waves in the air. Simulating the shock waves generated by impacts on Martian soil with computer models, the team observed the exact pattern of scimitars they saw on their impact site.
“We think the interference among different pressure waves lifts up the dust and sets avalanches in motion. These interference regions, and the avalanches, occur in a reproducible pattern,” Burleigh said. “We checked other impact sites and realized that when we see avalanches, we usually see two scimitars, not just one, and they both tend to be at a certain angle to each other. This pattern would be difficult to explain by seismic shaking.”
“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 project and one of the co-authors of the 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.”
The accepted manuscript is available online:
Interpreting physical features on Mars and understanding how they were formed is an important step in determining the potential habitability of past and present Mars. For instance, knowing the difference between features formed by impacts and those formed in the presence of liquid water can help scientists determine where to send missions designed to search for signs of past and present life on Mars.