Illustration of the main asteroid belt, orbiting the
Sun between Mars and Jupiter
NASA
NASA’s powerful James Webb Space Telescope includes asteroids on
its list of objects studied and secrets revealed.
A team led by researchers at the
Massachusetts Institute of Technology (MIT) in Cambridge repurposed Webb’s
observations of a distant star to reveal a population of small asteroids —
smaller than astronomers had ever detected orbiting the Sun in the main
asteroid belt between Mars and Jupiter.
The 138 new asteroids range from
the size of a bus to the size of a stadium — a size range in the main belt that
has not been observable with ground-based telescopes. Knowing how many main
belt asteroids are in different size ranges can tell us something about how
asteroids have been changed over time by collisions. That process is related to
how some of them have escaped the main belt over the solar system’s history,
and even how meteorites end up on Earth.
“We now understand more about how
small objects in the asteroid belt are formed and how many there could be,”
said Tom Greene, an astrophysicist at NASA’s Ames Research Center in
California’s Silicon Valley and co-author on the paper presenting the results. “Asteroids this size
likely formed from collisions between larger ones in the main belt and are
likely to drift towards the vicinity of Earth and the Sun.”
Insights from this research could
inform the work of the Asteroid Threat Assessment Project at Ames. ATAP
works across disciplines to support NASA’s Planetary Defense Coordination Office by studying what would happen in the case of an
Earth impact and modeling the associated risks.
“It’s exciting that Webb’s capabilities can be used to glean insights into asteroids,” said Jessie Dotson, an astrophysicist at Ames and member of ATAP. “Understanding the sizes, numbers, and evolutionary history of smaller main belt asteroids provides important background about the near-Earth asteroids we study for planetary defense.”
Illustration of the James Webb Space Telescope
NASA
The team that made the asteroid detections, led by research scientist Artem
Burdanov and professor of planetary science Julien de Wit, both of MIT,
developed a method to analyze existing Webb images for the presence of
asteroids that may have been inadvertently “caught on film” as they passed
in front of the telescope. Using the new image processing technique, they
studied more than 10,000 images of the star TRAPPIST-1, originally taken to search for atmospheres around planets orbiting the
star, in the search for life beyond Earth.
Asteroids shine more brightly in
infrared light, the wavelength Webb is tuned to detect, than in visible light,
helping reveal the population of main belt asteroids that had gone unnoticed
until now. NASA will also take advantage of that infrared glow with an upcoming
mission, the Near-Earth
Object (NEO) Surveyor. NEO Surveyor is the first space telescope specifically designed to hunt
for near-Earth asteroids and comets that may be potential hazards to Earth.
The paper presenting this research,
“Detections
of decameter main-belt asteroids with JWST,” was published Dec. 9 in Nature.
The James Webb Space Telescope is
the world’s premier space science observatory. Webb is solving mysteries in our
solar system, looking beyond to distant worlds around other stars, and probing
the mysterious structures and origins of our universe and our place in it. Webb
is an international program led by NASA with its partners, ESA (European Space
Agency) and CSA (Canadian Space Agency).
By: Aaron McKinnon, Abby Tabor
Source: NASA’s Webb Reveals Smallest Asteroids Yet Found in Main Asteroid Belt - NASA
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