ESA's comet chaser to fly by Earth

The spacecraft will make its closest approach to Earth at about 23:10 CET and come within 1900 kilometres, at which time it will be over Mexico, having already passed over Europe.

Watchers in Europe may have best evening view
On the evening of the closest approach, sky watchers in Europe will be favourably placed to follow this event using smaller telescopes or binoculars. Unfortunately, Rosetta is not expected to become visible to the naked eye from Europe as it will still be about 10 000 kilometres away until it disappears below the horizon.

However, amateur astronomers using video or photo-imaging in conjunction with a telescope should have a great viewing opportunity — weather permitting. They may even be able to see Rosetta's solar panels, which extend over 32 metres; the high-gain antenna may also be distinguishable.

After sunset on 4 March, it will appear to travel from south east to south west, moving from the constellation Sextans towards the setting Sun, crossing the complete sky. It will move faster as it heads west, disappearing below the horizon around 23:00 CET. As seen from Europe it will only reach a 'magnitude' of about +8 or +9 on the brightness scale used by astronomers. This is dimmer than a typical faint star and not readily apparent to the eye.

Rosetta swings between Earth and Mars
This fly-by manoeuvre will swing the three-tonne Rosetta spacecraft around our planet and out towards Mars, where it will make a fly-by on 26 February 2007, only to come back again to Earth. Fly-bys are necessary to accelerate the spacecraft, using planetary gravity, such that the orbital velocity of the target comet can eventually be matched.

This is the first of four planet fly-bys (three times with Earth, once with Mars) that Rosetta will carry out in its long journey to its target, Comet 67P/Churyumov-Gerasimenko. Rosetta will reach the comet in 2014, enter into orbit and deliver a lander, Philae, onto the surface.

Moon to serve as 'dummy' asteroid
A number of activities are planned during the current fly-by. A few hours before the closest approach the spacecraft will be pointed towards the Moon and the remote sensing and several other instruments will be switched on for calibration purposes.

After this fly-by, one of the two Navigation Cameras will be switched on to test Rosetta's ability to track asteroids using the Moon as a 'dummy' asteroid. Rosetta is scheduled to fly past two asteroids, Steins in September 2008 and Lutetia in July 2010, during which this tracking mode will be used to keep the spacecraft instruments centred on target.

Source: ESA