PUBLIC INFORMATION OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109. TELEPHONE (818) 354-5011
Contact: Diane Ainsworth
FOR IMMEDIATE RELEASE
January 29, 1997
PLANETARY ASTRONOMERS START YEAR WITH TWO DISCOVERIES
Two newly detected members of the solar system -- a rare
asteroid orbiting close to Earth and a distant comet making its
only appearance -- mark the first discoveries of the year for a
team of astronomers at NASA's Jet Propulsion Laboratory.
The discoveries, reported Jan. 10 by JPL planetary
scientists Dr. Eleanor Helin, Dr. Steve Pravdo, Dr. David
Rabinowitz and Ken Lawrence, were made possible with a few nights
of clear observing weather and use of a sensitive charge-coupled
device (CCD) camera called the Near-Earth Asteroid Tracking
(NEAT) system at Mt. Haleakala, Maui, HI. Since their initial
sightings, both objects have become the focus of worldwide
observations by astronomers in Japan, China, Australia, Canada,
Italy and the Czech Republic.
"This asteroid is a member of a rare class of asteroids,
called Atens, which stay within Earth's orbit most of their
lifetimes," said Helin, principal investigator of the NEAT
project. "The object has a higher inclination to the plane of
Earth's orbit than most Atens; in fact, at 31 degrees, it has the
second highest inclination of all the Atens we've discovered."
The highly inclined orbit, which is unusual, may result from
long-range interactions with the planets, or may be the outcome
of previous orbits passing near Earth. With the discovery of
more Atens, the relative importance of these competing influences
may be better understood.
Dubbed 1997 AC11, the asteroid is a faint object with an
absolute magnitude of 21, and probably measures about 600 feet in
diameter. It is only the 24th Aten to be discovered in 21 years,
since Helin found and named the first Aten in January 1976. With
orbits that are smaller than Earth's, and short periods, Atens
are in the vicinity of Earth frequently. This closeness to Earth
makes them more likely to impact the planet than other types of
"Atens never wander far from the orbit of Earth and can
cross Earth's orbit as many as four times a year," Helin said.
"1997 AC11, for instance, has a period of 8/10ths of a year, or
roughly 9.5 months. As we continue to observe it in coming
months, we will be able to characterize its orbital path with
more precision. With more precise data, we will be able to
examine its potential for collision with Earth at some time in
Along with the newest Aten, astronomers also discovered a
new comet, still distant but moving toward Earth and the Sun, as
it passed against the backdrop of the constellation of Leo.
Designated Comet 1997 A1, the celestial snowball is expected to
make its closest approach to Earth on Feb. 6, passing at a
distance of about 370 million kilometers (230 million miles), but
remaining visible in the night sky for several months thereafter.
"This comet has traveled a long distance, originating in the
Oort Cloud, a region far beyond Pluto's orbit which is believed
to house trillions of incipient comets," Helin said. "It has a
parabolic orbit, which means it will travel through our solar
system once and probably never be seen again. Parabolic comets
do not present their calling cards before arriving in the inner
solar system. They appear without warning."
At discovery, 1997 A1 was fairly dim at magnitude 19, and
showed a weakly condensed nucleus with a diffuse halo and short
tail, Helin said. The Minor Planet Center at the Smithsonian
Astrophysical Observatory in Cambridge, MA, announced the
discovery, reporting it as a parabolic comet, with an orbital
inclination of 145 degrees from the ecliptic plane, and indicated
that it would not pass any closer than 3.17 astronomical units
(475 million kilometers, or 295 million miles) from the Sun.
JPL's NEAT team, in conjunction with another observing
effort under way at the Laboratory's Table Mountain Observatory
in San Bernardino, CA, will continue to track and characterize
the comet over the next several months until it is no longer
During its closest approach on Feb. 6, the newly discovered
comet will be visible in the constellation of Cancer and brighten
to a magnitude of about 18. Moderate-sized telescopes with CCD
chips will be able to observe the comet, Helin said. Astronomers
report that the comet is continuing to outgas, or warm up and
boil off some of its ices, as it moves toward the Sun.
Low-resolution black-and-white images of both objects are
posted on the Internet on the following web page:
Discoveries of very faint or distant objects, and those
surprisingly close by, are increasing due to the introduction of
technologically advanced, fully autonomous CCD telescopes. The
NEAT camera, for example, employs a very large, very sensitive
4,096- by 4,096-pixel CCD. The camera is installed on a 1-meter
(39-inch) telescope operated at the summit of Mt. Haleakala by
the U.S. Air Force.
Using this powerful, fully automated system, astronomers are
discovering many more objects than was possible in the past. The
January observing run, for instance, produced more than 700
asteroid sightings, including high-inclination inner-belt
asteroids and a number of potential Mars-crossers, which will be
confirmed after more observations become available. Total
detections since NEAT began operations in late 1995 have climbed
to more than 9,000 objects, of which more than 50 percent are new
objects and more than 800 of those have received new
NEAT was built and is being managed by the Jet Propulsion
Laboratory for NASA's Office of Space Science, Washington, DC.