Closely watched by astronomers since its discovery in January 1989, this asteroid has been found to move in an orbit that brings it close to the Earth at regular intervals, about once every four years. This happened in 1992, 1996, 2000 and now again in 2004.

Radar observations during these passages have shown that Toutatis has an elongated shape, measuring about 4.6 x 2.4 x 1.9 km. It tumbles slowly through space, with a rotation period of 5.4 days.

This image of Toutatis was taken with the ESO Very Large Telescope (during a technical test) in the evening of September 28.

It was obtained just over 12 hours before the closest approach that happened today at about 15:40 hrs Central European Summer Time (CEST), or 13:40 hrs Universal Time (UT).

At the time of these observations, Toutatis was about 1,640,000 km from the Earth, moving with a speed of about 11 km/sec relative to our planet.

They show the asteroid as a fast-moving object of magnitude 10, about 40 times fainter than what can be perceived with the unaided, dark-adapted eye.

They also prove that Toutatis is right on track, following exactly the predicted trajectory in space and passing the Earth at a safe distance, as foreseen.

Detailed calculations, taking into account all available observations of this celestial body, have shown that although Toutatis passes regularly near the Earth, today's passage will be the closest one for quite some time, at least until the year 2562.

The ESO observations, obtained at a moment when Toutatis was very close to the Earth, will help to further refine the orbital calculations.

The "parallax effect" demonstrated

Simultaneous images obtained with telescopes at ESO's two observatories at La Silla and Paranal demonstrate the closeness of Toutatis to the Earth.

As can be seen on the unique ESO PR Photo 28e/04 that combines two of the exposures from the two observatories, the sighting angle to Toutatis from the two observatories, 513 km apart, is quite different.

Astronomers refer to this effect as the "parallax". The closer the object is, the larger is the effect, i.e., the larger will be the shift of the line-of-sight.

Interestingly, the measured angular distance in the sky of the beginning and end of the two trails (about 40 arcsec), together with the known distance between the two observatories and the position of Toutatis in the sky at the moment of the exposures fully define the triangle "Paranal-Toutatis-La Silla" and thus allow to calculate the exact distance to the asteroid.

It is found to be very close to that predicted from the asteroid's position in its orbit and that of the Earth at the moment of this unique observation, 1,607,900 km.

This exceptional, simultaneous set of observations thus provides an independent measurement of Toutatis' distance in space and, like the measured positions, a confirmation of its computed orbit.

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