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Chelyabinsk a decade on: the Sun's invisible asteroids
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By NASA
Illustration of the main asteroid belt, orbiting the Sun between Mars and JupiterNASA 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 TelescopeNASA 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).
For news media:
Members of the news media interested in covering this topic should reach out to the NASA Ames newsroom.
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By USH
Where do asteroids get all those craters? Countless small circular craters, plus almost always a few that look like massive killers. Even more confusing is that these craters are at a perfect 90º angle, as if an electric arc had run across the surface.
According to ThunderboltsProject, the Electric Universe (EU) model, the scars observed on asteroids are caused by electric arcs which cut surface depressions, scoop out material, accelerate it into space, then leave behind clean-cut geological relief.
This theory is supported by Electric Discharge Machining (EDM), a process we use every day to shape materials with electric arcs, producing similar clean-cut effects.
This brings us to the following hypothesis: Could it be that, instead of craters on asteroids being formed solely by natural space phenomena, that all these craters at a perfect 90º angle with clean-cut geological relief are the result of asteroid mining originated by alien races who use advanced electric arc/laser technology by extracting raw minerals they urgently need for use on their planet or for in-space manufacturing?
Asteroids vary greatly in composition, ranging from those rich in volatile substances to those composed of metals like gold, silver, platinum, cobalt, and palladium, alongside more common elements such as iron and nickel. This makes them potential treasure troves of valuable resources.
For us as Earthlings, asteroid mining is a technology in its earliest stages and requires significant advances in robotic technology before asteroid mining becomes a reality, however, if more advanced civilizations exist elsewhere in the universe, it's quite plausible that some of them have already turned to asteroid mining long ago.
Could their efforts be leaving behind the very craters on asteroids we observe today?
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By European Space Agency
ESA’s star-surveying Gaia mission has again proven to be a formidable asteroid explorer, spotting potential moons around more than 350 asteroids not known to have a companion.
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By European Space Agency
As ESA’s Hera mission for planetary defence completes its pre-launch testing, its target asteroids have come into focus as tiny worldlets of their own. A special issue of Nature Communications published this week presents studies of the Didymos asteroid and its Dimorphos moon, based on the roughly five and a half minutes of close-range footage returned by NASA’s DART spacecraft before it impacted the latter body – along with post-impact images from the Italian Space Agency’s LICIACube.
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