PUBLIC INFORMATION OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109. TELEPHONE (818) 354-5011
Contact: Jim Doyle
EMBARGOED FOR RELEASE AT 6 P.M. EASTERN TIME, OCTOBER 5, 1995
TOUTATIS ONE OF THE STRANGEST OBJECTS IN THE SOLAR SYSTEM
Two NASA-sponsored scientists studying the Earth-crossing
asteroid 4179 Toutatis with radio telescopes have found it to be
one of the strangest objects in the solar system, with a highly
irregular shape and an extraordinarily complex "tumbling"
rotation.
Both its shape and rotation are thought to be the outcome of
a history of violent collisions. A detailed description of the
asteroid and its observed rotation are reported in this week's
issue of the journal Science, by Drs. Scott Hudson of Washington
State University and Steven Ostro of NASA's Jet Propulsion
Laboratory, Pasadena, CA.
"The vast majority of asteroids, and all the planets, spin
about a single axis, like a football thrown in a perfect spiral,"
Hudson said, "but Toutatis tumbles like a flubbed pass."
One consequence of this strange rotation is that Toutatis
does not have a fixed north pole like the Earth. Instead, its
north pole wanders along a curve on the asteroid about every 5.4
days. "The stars viewed from Toutatis wouldn't repeatedly follow
circular paths, but would crisscross the sky, never following the
same path twice," Hudson said.
"The motion of the Sun during a Toutatis year, which is
about four Earth years, would be even more complex," he
continued. "In fact, Toutatis doesn't have anything you could
call a 'day.' Its rotation is the result of two different types
of motion with periods of 5.4 and 7.3 Earth days that combine in
such a way that Toutatis's orientation with respect to the solar
system never repeats."
The rotations of hundreds of asteroids have been studied
with optical telescopes. The vast majority of them appear to be
in simple rotation with a fixed pole and periods typically
between one hour and one day, the scientists said, even though
the violent collisions these objects are thought to have
experienced would mean that every one of them, at some time in
the past, should have been tumbling like Toutatis.
Internal friction has caused them to change into simple
rotational patterns in relatively brief amounts of time. However,
Toutatis rotates so slowly that this "dampening" process would
take much longer than the age of the solar system. This means
that the rotation of Toutatis is a remarkable, well-preserved
relic of the collision-related evolution of an asteroid.
Hudson and Ostro used radar images obtained with the Deep
Space Network Goldstone radar antenna in California and the
Arecibo telescope in Puerto Rico in 1992, when Toutatis passed to
within a little more than 2 million miles of the Earth. The
images are reported in a companion paper, also in this week's
issue of Science.
Toutatis was discovered by French astronomers in 1989 and
was named after a Celtic god that was the protector of the tribe
in ancient Gaul. Its eccentric, four-year orbit extends from
just inside the Earth's orbit to the main asteroid belt between
Mars and Jupiter. The plane of Toutatis's orbit is closer to the
plane of the Earth's orbit than any known Earth-orbit-crossing
asteroid.
On September 29, 2004, Toutatis will pass four lunar
distances from Earth, the closest approach of any known asteroid
or comet between now and 2060. One consequence of the asteroid's
frequent close approaches to Earth is that its trajectory more
than several centuries from now cannot be predicted accurately.
In fact, of all the Earth-crossing asteroids, Toutatis's orbit is
thought to be one of the most chaotic.
Earth-crossing asteroids are of great interest to scientists
for their relationships to meteorites, main-belt asteroids and
comets; as targets of human or robotic exploration; as sources of
materials with potential commercial value; and as long-term
collision hazards.
Nearly 300 Earth-crossing asteroids have been discovered, but the
entire population is thought to include some 1,500 objects larger
than one kilometer and some 135,000 objects that are larger than
100 meters.
The scientists' work was funded by the Planetary Geology and
Geophysics Program and the Planetary Astronomy Program of NASA's
Office of Space Science, Washington, D.C.
#####
10/5/95 JJD
#9567