Toutatis
(4179)
immagini radar da Terra, 4 gennaio 1993
In 1989, asteroid 4179 was discovered by
French astronomers and named after a Celtic god that was the
protector of the tribe in ancient Gaul. Its eccentric, four-year
orbit extends from just inside 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.
In December 1992, Toutatis made a close approach to Earth. At the
time, it was an average of about 4 million kilometers (2.5
million miles) from Earth. Images of Toutatis were acquired using
radar carried out at the Goldstone Deep Space Communications
Complex in California's Mojave desert. For most of the work, a
400,000-watt coded radio transmission was beamed at Toutatis from
the Goldstone main 70-meter (230-foot) antenna. The echoes, which
took as little as 24 seconds to travel to Toutatis and back, were
received by the new 34-meter (112-foot) antenna and relayed back
to the 70-meter (230-foot) station, where they were decoded and
processed into images.
The images of Toutatis reveal two irregularly shaped, cratered
objects about 4 and 2.5 kilometers (2.5 and 1.6 miles) in average
diameter which are probably in contact with each other. These
contact binaries may be fairly common since another
one, 4769 Castalia, was observed in 1989 when it passed near the
Earth. Numerous surface features on Toutatis, including a pair of
half-mile-wide craters, side by side, and a series of three
prominent ridges -- a type of asteroid mountain range -- are
presumed to result from a complex history of impacts.
Toutatis is 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.
The vast majority of asteroids, and all the planets, spin
about a single axis, like a football thrown in a perfect spiral,
but Toutatis tumbles like a flubbed pass, said Dr. Scott
Hudson of Washington State University. 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 asteroids 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.
On September 29, 2004, Toutatis will pass by Earth at a range of
four times the distance between the Earth and the Moon, 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, the orbit of Toutatis is thought to be
one of the most chaotic.