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Astronomers have identified a significant population of previously undetected asteroids in the main belt between Mars and Jupiter, according to research published on December 9, 2024, in Nature. This discovery was made through analysis of archival images from the James Webb Space Telescope (JWST). Among these asteroids, some have been found on trajectories that could bring them close to Earth, as per the findings. The detected asteroids, ranging from the size of a bus to that of multiple stadiums, represent the smallest known objects within the main asteroid belt.

Although smaller than the asteroid linked to the extinction of the dinosaurs, these space rocks carry potential risks due to their capacity for destruction. For instance, a decametre-sized asteroid exploded above Chelyabinsk, Russia, a decade ago, releasing energy equivalent to 30 Hiroshima bombs.

A Computational Breakthrough in Asteroid Detection

As per reports, Julien de Wit, Associate Professor of Planetary Science at MIT, and his team have employed a computationally intensive technique to identify these space rocks. The approach, applied to JWST images originally focused on the TRAPPIST-1 system, allowed for the discovery of 138 new asteroids. Six of these appear to have been influenced by planetary gravitational forces, potentially positioning them near Earth in the future. De Wit described the unexpected volume of detections as indicative of a “new population regime”.

Advantages of Infrared Detection

The telescope’s infrared capabilities were key to this achievement, as they captured thermal emissions from the asteroids more effectively than traditional visible-light methods. Artem Burdanov, a research scientist at MIT, noted this as an example of how revisiting data with modern technology can yield substantial discoveries.

Upcoming observations using JWST and other telescopes, such as the Vera C. Rubin Observatory, are expected to identify thousands more small asteroids, advancing planetary defence and orbital tracking.

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Astronomers Spot Signs of Baby Planets in a Star’s Mysterious Disk

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Astronomers using Keck Observatory have imaged the dusty disk around HD 34282, a young star about 400 light-years away, revealing bright clumps and a 40 AU gap—clear signs of planet formation. The system provides a rare glimpse into early planetary birth, helping refine models of how gas and dust evolve into new worlds.

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NASA’s James Webb Space Telescope Telescope Challenges Old Theories on Mini-Neptune Worlds

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New models suggest mini-Neptunes—planets smaller than Neptune with thick gas envelopes—may have solid rocky surfaces instead of molten magma. Data from NASA’s JWST revealed high-pressure atmospheres capable of compressing molten rock into solid crusts. This discovery challenges earlier assumptions and offers key insights into exoplanet composition and planetary …

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Mystery Deepens as Interstellar Comet 3I/ATLAS Brightens Unexpectedly Near the Sun

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Interstellar comet 3I/ATLAS defied expectations during its 2025 solar flyby, brightening far faster than predicted. Observatories worldwide recorded a blue coma rich in exotic gases, suggesting unique chemistry from another star system. Scientists are investigating whether its unusual composition or speed caused the outburst, marking a new interstellar mystery.

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