(Image credit: JAXA/University of Tokyo/Kochi University/Rikkyo University/Nagoya University/Chiba Institute of Technology/Meiji University/University of Aizu/AIST)
Snap, crackle, pop! Dust ‘hopping’ on asteroids might influence how these small bodies migrate through space.
“The more fine-grained material, or regolith, these asteroids lose, the faster they migrate,” lead author Hsiang-Wen (Sean) Hsu, research scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder, said in a statement. (opens in new tab)
Some “curious” photos captured at Bennu, as the scientists termed it, sparked the discussion. These came courtesy of an asteroid-sampling mission known as OSIRIS-REx and showed that the surface was sandpaper-like, defying scientists expectations of smoothness. Similar images flowed from another recently studied asteroid called Ryugu, explored by a Japanese spacecraft known as Hayabusa2.
Hsu and co-lead author Xu Wang, a research associate at LASP, helmed a team creating computer simulations and laboratory experiments to better explain the imagery from these two worlds.
“Forces akin to static electricity may be kicking the smallest grains of dust, some no bigger than a single bacterium, off the asteroid and into space — leaving only larger rocks behind,” the statement said. The same process may even be at play in places like the rings of Saturn, another spot filled with airless, tiny worlds.
Asteroids are constantly spinning worlds and because they are so small, sunlight falling on their surface varies considerably. One small region may flash quickly between sunlight and shadow and strain surface rocks until they crack.
Even dust grains are affected, as they are thrown into space through a process called electrostatic lofting. The sun‘s light upon regolith eventually builds up negative charges on individual dust particles.
When the charge accumulates enough, the particles pop away from each other like two repelling magnets, at speeds sometimes exceeding 20 mph (30 kph).
“No one had ever considered this process on the surface of an asteroid before,” said Wang.
Simulations appear to show the most effect from explosions of dust on smaller asteroids, because these tiny worlds have comparatively weaker gravity. On the smaller worlds, similar in size to Ryugu, regolith may be lost into space over the eons.
This loss not only creates the boulder-strewn landscape visible on Bennu and Ryugu, but given enough time an asteroid could lose much its dust. A “cleaner” surface is more exposed to the effects of the sun‘s radiation, which can push the orbit in a different direction given enough time.
While the effects are still poorly understood, scientists hope to gain more information with NASA’s forthcoming Double Asteroid Redirection Test (DART) that will visit two other asteroids of similar scale to Ryugu and Bennu. DART will arrive at the system, called Didymos, in September and slam into the smaller rock to conduct an asteroid impact test.
A story based on the research was published July 11 in Nature Astronomy (opens in new tab).
Elizabeth Howell, Ph.D., is a contributing writer for Space.com (opens in new tab) since 2012. As a proud Trekkie and Canadian, she tackles topics like spaceflight, diversity, science fiction, astronomy and gaming to help others explore the universe. Elizabeth’s on-site reporting includes two human spaceflight launches from Kazakhstan, and embedded reporting from a simulated Mars mission in Utah. She holds a Ph.D. and M.Sc (opens in new tab). in Space Studies from the University of North Dakota, and a Bachelor of Journalism from Canada’s Carleton University. Her latest book, NASA Leadership Moments, is co-written with astronaut Dave Williams. Elizabeth first got interested in space after watching the movie Apollo 13 in 1996, and still wants to be an astronaut someday.