Skip to main content

Radar Images Capture Asteroid 2024 JV33 Before Close Earth Approach.


 

On August 18, 2024, the Goldstone Solar System Radar, located near Barstow, California, captured a series of radar images of asteroid 2024 JV33 as it neared Earth. At the time of observation, the asteroid was 2.8 million miles (4.6 million kilometers) away—approximately 12 times the distance between the Moon and Earth.


Discovered by the NASA-funded Catalina Sky Survey in Tucson, Arizona, on May 4, the asteroid is notably shaped like a peanut, with two distinct lobes, one larger than the other. Radar imaging revealed that 2024 JV33 is about 980 feet (300 meters) long and twice as long as it is wide. It completes a rotation every seven hours.


Radar technology is pivotal in identifying such "contact binary" asteroids. The Goldstone radar, part of NASA's Deep Space Network, has imaged dozens of these objects. Notably, about 14% of near-Earth asteroids larger than 660 feet (200 meters) are contact binaries. With an elongated orbit similar to many comets, influenced by Jupiter's gravity, 2024 JV33 might be an inactive cometary nucleus, although no comet-like activity has been observed.


Despite being classified as potentially hazardous, 2024 JV33 does not pose any immediate threat to Earth. The recent radar measurements have significantly refined our understanding of its distance and trajectory for decades to come.


The Goldstone Solar System Radar Group is supported by NASA's Near-Earth Object Observations Program and managed by NASA's Jet Propulsion Laboratory. The Deep Space Network, overseen by NASA's Space Communications and Navigation program office, plays a crucial role in planetary radar observations.


For more details on planetary radar and near-Earth objects, visit: NASA JPL Asteroid Watch.

Comments

Popular posts from this blog

James Webb Space Telescope Opens New Frontiers in the Search for Life Beyond Earth.

  This image illustrates a science-based artist’s impression of K2-18 b, a potentially habitable exoplanet 120 light-years away, orbiting a cool dwarf star in its habitable zone. NASA’s James Webb Space Telescope (JWST) is revolutionizing the search for life beyond our solar system, offering humanity its most detailed look yet at distant, potentially habitable worlds. With its extraordinary infrared capabilities, Webb is not only detecting atmospheres on small rocky exoplanets but also probing their chemical makeup in search of biosignatures—clues that could hint at the presence of life. However, scientists caution that context is everything. Atmospheric data alone is not enough to confirm life; understanding a planet’s surface, interior, and broader environment is essential. Even detecting a potential biosignature, such as a gas possibly produced by biological processes, doesn’t equate to discovery. Multiple, independent lines of evidence would be needed to confirm such a find. “F...

Webb Telescope Reveals Tangled Rings and Dusty Chaos in Dying Star System NGC 1514.

  NASA’s James Webb Space Telescope has captured the most detailed image yet of planetary nebula NGC 1514, revealing clumpy dust rings and clear holes in its vibrant pink core using mid-infrared light. A dying star’s final performance has been brought into sharp focus by NASA’s James Webb Space Telescope, revealing a cosmic display of tangled rings, drifting dust, and mysterious holes in the planetary nebula NGC 1514. This mesmerizing structure lies about 1,500 light-years away in the constellation Taurus and has been evolving for at least 4,000 years. At the heart of the nebula are two tightly bound stars, orbiting each other every nine years, their light diffracted in Webb’s images like a celestial jewel. While the stars appear as one in mid-infrared light, they are central to the nebula’s complex architecture. One of these stars, once several times the mass of our Sun, ejected its outer layers in a slow, dense stellar wind as it aged. The other star’s close approach may have twi...

Astronomers have discovered a 'Death Star' black hole in action.

A team of astronomers has studied 16 supermassive black holes that are firing powerful beams into space, tracking where these beams, or jets, are pointing now and where they were aimed in the past, as reported in our latest press release. Using NASA’s Chandra X-ray Observatory and the U.S. National Science Foundation (NSF) National Radio Astronomical Observatory’s (NRAO) Very Large Baseline Array (VLBA), they found that some of the beams have changed directions by large amounts. These two Chandra images show hot gas in the middle of the galaxy cluster Abell 478 (left) and the galaxy group NGC 5044 (right). The center of each image contains one of the sixteen black holes firing beams outwards. Each black hole is located in the center of a galaxy embedded in the hot gas. In the images below, labels and the radio images appear. Ellipses show a pair of cavities in the hot gas for Abell 478 (left), while ellipses indicate two pairs of cavities for NGC 5044 (right). These cavities were carve...