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| This collage shows six planetary radar observations of 2011 AG5 a day after the asteroid made its close approach to Earth on Feb. 3. With dimensions comparable to the Empire State Building, 2011 AG5 is one of the most elongated asteroids to be observed by planetary radar to date. Credit: NASA/JPL-Caltech |
On Feb. 3, an asteroid more than three times as long as it is wide safely
flew past Earth at a distance of about 1.1 million miles (1.8 million
kilometers, or a little under five times the distance between the Moon and
Earth). While there was no risk of the asteroid—called 2011 AG5—impacting
our planet, scientists at NASA's Jet Propulsion Laboratory in Southern
California closely tracked the object, making invaluable observations to
help determine its size, rotation, surface details, and, most notably,
shape.
This close approach provided the first opportunity to take a detailed look
at the asteroid since it was discovered in 2011, revealing an object about
1,600 feet (500 meters) long and about 500 feet (150 meters) wide—dimensions
comparable to the Empire State Building. The powerful 230-foot (70-meter)
Goldstone Solar System Radar antenna dish at the Deep Space Network's
facility near Barstow, California, revealed the dimensions of this extremely
elongated asteroid.
"Of the 1,040 near-Earth objects observed by planetary radar to date, this
is one of the most elongated we've seen," said Lance Benner, principal
scientist at JPL who helped lead the observations.
The Goldstone radar observations took place from Jan. 29 to Feb. 4,
capturing several other details: Along with a large, broad concavity in one
of the asteroid's two hemispheres, 2011 AG5 has subtle dark and lighter
regions that may indicate small-scale surface features a few dozen meters
across. And if the asteroid were viewed by the human eye, it would appear as
dark as charcoal. The observations also confirmed 2011 AG5 has a slow
rotation rate, taking nine hours to fully rotate.
Beyond contributing to a better understanding of what this object looks like
up close, the Goldstone radar observations provide a key measurement of the
asteroid's orbit around the Sun. Radar provides precise distance
measurements that can help scientists at NASA's Center for Near Earth Object
Studies (CNEOS) refine the asteroid's orbital path. Asteroid 2011 AG5 orbits
the Sun once every 621 days and won't have a very close encounter with Earth
until 2040, when it will safely pass our planet at a distance of about
670,000 miles (1.1 million kilometers, or nearly three times the Earth-Moon
distance).
"Interestingly, shortly after its discovery, 2011 AG5 became a poster-child
asteroid when our analysis showed it had a small chance of a future impact,"
said Paul Chodas, the director for CNEOS at JPL. "Continued observations of
this object ruled out any chance of impact, and these new ranging
measurements by the planetary radar team will further refine exactly where
it will be far into the future."
CNEOS calculates every known near-Earth asteroid orbit to provide
assessments of potential impact hazards. Both the Goldstone Solar System
Radar Group and CNEOS are supported by NASA's Near-Earth Object Observations
Program within the Planetary Defense Coordination Office at the agency's
headquarters in Washington.
Source: NASA
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Space & Astrophysics