“On November 8, asteroid 2005 YU55 will fly past Earth, and at its closest approach point will be about 201,700 miles (325,000 kilometers) away,” said Don Yeomans from NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. “This asteroid is about 1,300 feet (400 meters) wide — the largest space rock we have identified that will come this close until 2028.”
“YU55 poses no threat of an Earth collision over, at the very least, the next 100 years,” Yeomans said. “During its closest approach, its gravitational effect on the Earth will be so miniscule as to be immeasurable. It will not affect the tides or anything else.”
Then why all the hubbub for a space rock a little bit wider than an aircraft carrier? After all, scientists estimate that asteroids the size of YU55 come this close about every 25 years.
“While near-Earth objects of this size have flown within a lunar distance in the past, we did not have the foreknowledge and technology to take advantage of the opportunity,” said Barbara Wilson from JPL. “When it flies past, it should be a great opportunity for science instruments on the ground to get a good look.”
Robert McMillan from the University of Arizona, Tucson, discovered 2005 YU55 in December 2005. The space rock has been in astronomers’ crosshairs before. In April 2010, Mike Nolan and colleagues at the Arecibo Observatory in Puerto Rico generated some ghostly images of 2005 YU55 when the asteroid was about 1.5 million miles (2.3 million km) from Earth
“The best resolution of the radar images was 25 feet (7.5m) per pixel,” said Lance Benner from JPL. “When 2005 YU55 returns this fall, we intend to image it at 13-foot (4m) resolution with our recently upgraded equipment at the Deep Space Network in Goldstone, California. Plus, the asteroid will be 7 times closer.
We’re expecting some very detailed radar images.”
Radar astronomy employs the world’s most massive dish-shaped antennas. The antennas beam direct microwave signals at their celestial targets — which can be as close as our Moon and as far away as the moons of Saturn. These signals bounce off the target, and the resulting “echo” is collected and precisely collated to create radar images, which can be used to reconstruct detailed 3-D models of the object. This defines its rotation precisely and gives scientists a good idea of the object’s surface roughness. They can even make out surface features.
“Using the Goldstone radar operating with the software and hardware upgrades, the resulting images of YU55 could come in with resolution as fine as 13 feet (4m) per pixel,” said Benner. “We’re talking about getting down to the kind of surface detail you dream of when you have a spacecraft fly by one of these targets.”
At that resolution, JPL astronomers can see boulders and craters on the surfaces of some asteroids, and establish if an asteroid has a moon or two of its own. (Note: the 2010 Arecibo imaging of YU55 did not show any moons). But beyond the visually intriguing surface, the data collected from Goldstone, Arecibo, and ground-based optical and infrared telescopes are expected to detail the mineral composition of the asteroid.
“This is a C-type asteroid, and those are thought to be representative of the primordial materials from which our solar system was formed,” said Wilson. “This flyby will be an excellent opportunity to test how we study, document, and quantify which asteroids would be most appropriate for a future human mission.”
Yeomans reiterated Wilson’s view that the upcoming pass of asteroid 2005 YU55 will be a positive event, which he describes as an “opportunity for scientific discovery.”
“On November 8, asteroid 2005 YU55 will fly past Earth, and at its closest approach point will be about 201,700 miles (325,000 kilometers) away,” said Don Yeomans from NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. “This asteroid is about 1,300 feet (400 meters) wide — the largest space rock we have identified that will come this close until 2028.”
“YU55 poses no threat of an Earth collision over, at the very least, the next 100 years,” Yeomans said. “During its closest approach, its gravitational effect on the Earth will be so miniscule as to be immeasurable. It will not affect the tides or anything else.”
Then why all the hubbub for a space rock a little bit wider than an aircraft carrier? After all, scientists estimate that asteroids the size of YU55 come this close about every 25 years.
“While near-Earth objects of this size have flown within a lunar distance in the past, we did not have the foreknowledge and technology to take advantage of the opportunity,” said Barbara Wilson from JPL. “When it flies past, it should be a great opportunity for science instruments on the ground to get a good look.”
Robert McMillan from the University of Arizona, Tucson, discovered 2005 YU55 in December 2005. The space rock has been in astronomers’ crosshairs before. In April 2010, Mike Nolan and colleagues at the Arecibo Observatory in Puerto Rico generated some ghostly images of 2005 YU55 when the asteroid was about 1.5 million miles (2.3 million km) from Earth
“The best resolution of the radar images was 25 feet (7.5m) per pixel,” said Lance Benner from JPL. “When 2005 YU55 returns this fall, we intend to image it at 13-foot (4m) resolution with our recently upgraded equipment at the Deep Space Network in Goldstone, California. Plus, the asteroid will be 7 times closer.
We’re expecting some very detailed radar images.”
Radar astronomy employs the world’s most massive dish-shaped antennas. The antennas beam direct microwave signals at their celestial targets — which can be as close as our Moon and as far away as the moons of Saturn. These signals bounce off the target, and the resulting “echo” is collected and precisely collated to create radar images, which can be used to reconstruct detailed 3-D models of the object. This defines its rotation precisely and gives scientists a good idea of the object’s surface roughness. They can even make out surface features.
“Using the Goldstone radar operating with the software and hardware upgrades, the resulting images of YU55 could come in with resolution as fine as 13 feet (4m) per pixel,” said Benner. “We’re talking about getting down to the kind of surface detail you dream of when you have a spacecraft fly by one of these targets.”
At that resolution, JPL astronomers can see boulders and craters on the surfaces of some asteroids, and establish if an asteroid has a moon or two of its own. (Note: the 2010 Arecibo imaging of YU55 did not show any moons). But beyond the visually intriguing surface, the data collected from Goldstone, Arecibo, and ground-based optical and infrared telescopes are expected to detail the mineral composition of the asteroid.
“This is a C-type asteroid, and those are thought to be representative of the primordial materials from which our solar system was formed,” said Wilson. “This flyby will be an excellent opportunity to test how we study, document, and quantify which asteroids would be most appropriate for a future human mission.”
Yeomans reiterated Wilson’s view that the upcoming pass of asteroid 2005 YU55 will be a positive event, which he describes as an “opportunity for scientific discovery.”
