Asteroid 1997 QK1 is shown to be an elongated, peanut-shaped near-Earth object in this series of 28 radar images obtained by the Deep Space Network’s Goldstone Solar System Radar on Aug. 21, 2025. The asteroid is about 660 feet (200 meters) long and completes one rotation every 4.8 hours. It passed closest to our planet on the day before these observations were made at a distance of about 1.9 million miles (3 million kilometers), or within eight times the distance between Earth and the Moon.
The 2025 flyby is the closest that 1997 QK1 has approached to Earth in more than 350 years. Prior to the recent Goldstone observations, very little was known about the asteroid.
These observations resolve surface features down to a resolution of about 25 feet (7.5 meters) and reveal that the object has two rounded lobes that are connected, with one lobe twice the size of the other. Both lobes appear to have concavities that are tens of meters deep. Asteroid 1997 QK1 is likely a “contact binary,” one of dozens of such objects imaged by Goldstone. At least 15% of near-Earth asteroids larger than about 660 feet (200 meters) have a contact binary shape.
The asteroid is classified as potentially hazardous, but it does not pose a hazard to Earth for the foreseeable future. These Goldstone measurements have greatly reduced the uncertainties in the asteroid’s distance from Earth and in its future motion for many decades.
The Goldstone Solar System Radar Group is supported by NASA’s Near-Earth Object Observations Program within the Planetary Defense Coordination Office at the agency’s headquarters in Washington. Managed by NASA’s Jet Propulsion Laboratory, the Deep Space Network receives programmatic oversight from Space Communications and Navigation program office within the Space Operations Mission Directorate, also at NASA Headquarters.
More information about planetary radar and near-Earth objects can be found at:
https://www.jpl.nasa.gov/asteroid-watch