During the close approach of 2008 OS7 with Earth on February 2, the agency’s Deep Space Network planetary radar gathered the first detailed images of the stadium-size asteroid.
On February 2, a large asteroid safely drifted past Earth at a distance of regarding 1.8 million miles (2.9 million kilometers, or 7 ½ times the distance between Earth and the Moon). There was no risk of the asteroid impacting our planet, but scientists at NASA’s Jet Propulsion Laboratory in Southern California used a powerful radio antenna to better determine the size, rotation, shape, and surface details of this near-Earth object (NEO). Until this close approach, asteroid 2008 OS7 had been too far from Earth for planetary radar systems to image it.
The asteroid was discovered on July 30, 2008, during routine search operations for NEOs by the NASA-funded Catalina Sky Survey, which is headquartered at the University of Arizona in Tucson. After discovery, observations of the amount of light reflected from the asteroid’s surface revealed that it was roughly between 650 to 1,640 feet (200 and 500 meters) wide and that it is comparatively slow rotating, completing one rotation every 29 ½ hours.
The rotational period of 2008 OS7 was determined by Petr Pravec, at the Astronomical Institute of the Czech Academy of Sciences in Ondřejov, Czech Republic, who observed the asteroid’s light curve – or how the brightness of the object changes over time. As the asteroid spins, variations in its shape change the brightness of reflected light astronomers see, and those changes are recorded to understand the period of the asteroid’s rotation.
During the February 2 close approach, JPL’s radar group used the powerful 230-foot (70-meter) Goldstone Solar System Radar antenna dish at the Deep Space Network’s facility near Barstow, California, to image the asteroid. What scientists found was that its surface has a mix of rounded and more angular regions with a small concavity. They also found the asteroid is smaller than previously estimated – regarding 500 to 650 feet (150 to 200 meters) wide – and confirmed its uncommonly slow rotation.
The Goldstone radar observations also provided key measurements of the asteroid’s distance from Earth as it passed by. Those measurements can help scientists at NASA’s Center for Near Earth Object Studies (CNEOS) refine calculations of the asteroid’s orbital path around the Sun. Asteroid 2008 OS7 orbits the Sun once every 2.6 years, traveling from within the orbit of Venus and past the orbit of Mars at its farthest point.
CNEOS, which is managed by JPL, calculates every known NEO orbit to provide assessments of potential impact hazards. Due to the proximity of its orbit to that of the Earth and its size, 2008 OS7 is classified as a potentially hazardous asteroid, but the February 2 close approach is the nearest it will come to our planet for at least 200 years.
The recent radar imaging of asteroid 2008 OS7 provides valuable insights into the size, rotation, and surface details of this stadium-size asteroid. The images captured by the Goldstone Solar System Radar antenna have revealed a mix of rounded and angular regions, as well as a small concavity on the asteroid’s surface. This information enhances our understanding of this near-Earth object and its potential implications for our planet.
One of the key findings from the radar observations is the revised estimate of the asteroid’s size. Previous estimates suggested a width of 650 to 1,640 feet, but the new measurements indicate that it is smaller, measuring regarding 500 to 650 feet in width. Additionally, the radar data confirmed that the asteroid has an unusually slow rotation, completing one rotation every 29 ½ hours.
These details hold significant implications for our understanding of asteroids and their potential impact hazards. By refining calculations of the asteroid’s orbital path around the Sun, scientists can better assess the potential risks associated with its proximity to Earth. The fact that asteroid 2008 OS7 is classified as a potentially hazardous asteroid highlights the importance of continued monitoring and research in this field.
While the recent close approach of the asteroid posed no immediate risk to our planet, the images and data collected during this event will contribute to ongoing efforts to improve our ability to detect and track potentially dangerous near-Earth objects. As part of NASA’s Center for Near Earth Object Studies (CNEOS), these observations will aid in refining orbital predictions and assist in developing strategies for planetary defense.
The Goldstone Solar System Radar Group and CNEOS play crucial roles in NASA’s Near-Earth Object Observations Program, which aims to identify and track objects that might potentially cause significant damage
