Skip to main content

New Method Detects Small Asteroids in Main Belt, Offering Insight for Planetary Defense.

 



An international team of physicists, led by MIT researchers, has developed a groundbreaking method to detect small asteroids, as small as 10 meters in diameter, within the main asteroid belt. These space rocks, ranging from the size of a bus to several stadiums wide, were previously undetectable using traditional methods. The team's discovery, detailed in a paper published in Nature, could significantly improve tracking of potential asteroid impactors, aiding planetary defense efforts.


The main asteroid belt, located between Mars and Jupiter, is home to millions of asteroids, but until now, scientists could only detect objects roughly a kilometer in diameter. The new detection technique, which utilizes the "shift and stack" method, is able to identify much smaller asteroids, even those far from Earth, enabling more precise orbital tracking. This breakthrough is crucial for planetary defense, allowing scientists to spot near-Earth objects that may pose a threat in the future.


Lead author Artem Burdanov, a research scientist at MIT, emphasized the potential of this technique: "We have been able to detect near-Earth objects down to 10 meters in size when they are really close to Earth. Now, we can spot these small asteroids when they are much farther away, which is key for planetary defense."


The new detection method, which processes vast amounts of imaging data, was initially tested on data from the SPECULOOS survey and a telescope in Antarctica. The team then applied the technique to images from NASA's James Webb Space Telescope (JWST), which is particularly sensitive to infrared light. Using JWST data from the TRAPPIST-1 system, the researchers identified 138 new asteroids, including several small objects likely to be near-Earth asteroids.


Professor Julien de Wit, co-author of the study, noted, "We thought we would just detect a few new objects, but we detected so many more than expected, especially small ones." The researchers believe their findings provide a window into the origin of meteorites and the dynamics of asteroid families formed through collisions.


This discovery opens up a new realm of asteroid research, where smaller objects, often overlooked, are being recognized for their potential impact on Earth. The team's work exemplifies the power of reanalyzing existing data and the role of modern technology in advancing our understanding of space hazards.



Comments

Popular posts from this blog

NASA/ESA Hubble Space Telescope Reveals New Details of the Orion Nebula’s Star Formation.

  This NASA/ESA Hubble Space Telescope image captures the Orion Nebula (Messier 42, M42), the nearest star-forming region to Earth, located about 1,500 light-years away. A captivating new image captured by the NASA/ESA Hubble Space Telescope offers an extraordinary look into the Orion Nebula, the nearest massive star-forming region to Earth. Located just 1,500 light-years away, this nebula is visible to the naked eye below the three stars forming Orion's "belt." The region is home to hundreds of newborn stars, including two protostars featured in the image: HOPS 150 and HOPS 153. Named after the Herschel Orion Protostar Survey, conducted with ESA’s Herschel Space Observatory, the protostars HOPS 150 and HOPS 153 provide key insights into the early stages of star formation. HOPS 150, visible in the upper-right corner of the image, is a binary star system, with two young stars orbiting one another. These protostars are surrounded by small dusty disks, where material from th...

XSPECT Payload Successfully Validates Performance through Cas A Observation.

  The XSPECT instrument captures a detailed spectrum of the supernova remnant Cassiopeia A (Cas A), encompassing both the Galactic Cosmic Ray (GCR) background and the Cosmic X-ray Background (CXB). The flux observed above 8 keV predominantly results from the combined contributions of CXB and GCR. The presented spectrum, depicted in the figure, is derived from a cumulative integration time of 20 ksec, collected across multiple orbits, providing valuable insights into the X-ray emissions associated with Cas A. XPoSat, India's inaugural X-ray polarimetric mission, has achieved a significant as the XSPECT instrument captures its initial observations from the Cassiopeia A (Cas A) supernova remnant. Launched on January 1, 2024, XPoSat is equipped with two co-aligned instruments, namely the POLarimeter Instrument in X-rays (POLIX) and X-ray SPECtroscopy and Timing (XSPECT). This mission is designed to unravel the mysteries of cosmic X-ray sources. While POLIX focuses on examining X-ray po...