[meteorite-list] Spacecraft Earth to Perform Asteroid 'Flyby' This Fall (Asteroid 2005 YU55)

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Mon, 2 May 2011 15:54:50 -0700 (PDT)
Message-ID: <201105022254.p42Mso9q018586_at_zagami.jpl.nasa.gov>

http://www.jpl.nasa.gov/news/news.cfm?release=2011-129

Spacecraft Earth to Perform Asteroid 'Flyby' This Fall
Jet Propulsion Laboratory
May 02, 2011

Since the dawn of the space age, humanity has sent 16 robotic emissaries
to fly by some of the solar system's most intriguing and nomadic
occupants -- comets and asteroids. The data and imagery collected on
these deep-space missions of exploration have helped redefine our
understanding of how Earth and our part of the galaxy came to be. But
this fall, Mother Nature is giving scientists around the world a
close-up view of one of her good-sized space rocks -- no rocket required.

"On November 8, asteroid 2005 YU55 will fly past Earth and at its
closest approach point will be about 325,000 kilometers [201,700 miles]
away," said Don Yeomans, manager of NASA's Near-Earth Object Program
Office at the Jet Propulsion Laboratory in Pasadena, Calif. "This
asteroid is about 400 meters [1,300 feet] wide ??? the largest space rock
we have identified that will come this close until 2028."

Despite the relative proximity and size, Yeomans said, "YU55 poses no
threat of an Earth collision over, at the very least, the next 100
years. 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, a scientist
at JPL. "When it flies past, it should be a great opportunity for
science instruments on the ground to get a good look."

2005 YU55 was discovered in December 2005 by Robert McMillan, head of
the NASA-funded Spacewatch Program at the University of Arizona, Tucson.
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 2.3 million kilometers (1.5 million miles) from Earth. (See
related story: http://www.jpl.nasa.gov/news/news.cfm?release=2010-144 .

"The best resolution of the radar images was 7.5 meters [25 feet] per
pixel," said JPL radar astronomer Lance Benner. "When 2005 YU55 returns
this fall, we intend to image it at 4-meter resolution with our recently
upgraded equipment at the Deep Space Network at Goldstone, California.
Plus, the asteroid will be seven times closer. We're expecting some very
detailed radar images."

Radar astronomy employs the world's most massive dish-shaped antennas.
The antennas beam directed 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 three-dimensional 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 4 meters 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." Yeomans adds, "So stay tuned. This is going to be
fun."

The 70-meter (230-foot) Goldstone antenna in California's Mojave Desert,
part of NASA's Deep Space Network, is one of only two facilities capable
of imaging asteroids with radar. The other is the National Science
Foundation's 1,000-foot-diameter (305 meters) Arecibo Observatory in
Puerto Rico. The capabilities of the two instruments are complementary.
The Arecibo radar is about 20 times more sensitive and can detect
asteroids about twice as far away, but because the main dish is
stationary it can only see about one-third of the sky. Goldstone is
fully steerable and can see about 80 percent of the accessible sky, so
it can track objects several times longer per day and can image
asteroids at finer spatial resolution. To date, Goldstone and Arecibo
have observed 272 near-Earth asteroids and 14 comets with radar. JPL
manages the Goldstone Solar System Radar and the Deep Space Network for
NASA.

NASA detects, tracks and characterizes asteroids and comets passing
close to Earth using both ground- and space-based telescopes. The
Near-Earth Object Observations Program, commonly called "Spaceguard,"
discovers these objects, characterizes a subset of them, and plots their
orbits to determine if any could be potentially hazardous to our planet.

JPL manages the Near-Earth Object Program Office for NASA's Science
Mission Directorate in Washington. JPL is a division of the California
Institute of Technology in Pasadena.

More information about asteroids and near-Earth objects is at:
http://www.jpl.nasa.gov/asteroidwatch .

More information about asteroid radar research is at:
http://echo.jpl.nasa.gov/ .

More information about the Deep Space Network is at:
http://deepspace.jpl.nasa.gov/dsn .

DC Agle (818) 393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
agle at jpl.nasa.gov

2011-129
Received on Mon 02 May 2011 06:54:50 PM PDT