ESO Press Photos 06a-b/04
2 March 2004
For immediate release
ESO's Telescope Takes Picture of
ESA's Rosetta's Target,
Comet 67P/Churyumov-Gerasimenko
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ESO PR Photo 06a/04
[Preview - JPEG: 400 x 471 pix - 286k]
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ESO PR Photo 06b/04
[Preview - JPEG: 400 x 453 pix - 290k]
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Caption : PR Photo 06a/04 shows a composite image of the nucleus of Comet 67P/Churyumov-Gerasimenko (the point of light at the centre), recorded on February 26, 2004, at 6:15 UT with the SUSI-2 camera on the 3.5-m New Technology Telescope. It is based on fifteen series of exposures seen in three different wavebands and since the images were aligned on the comet, the images of stars in the field are trailed. The fact that the image of the comet's 'dirty snowball' nucleus is almost star-like indicates that it is surrounded by a very small amount of gas or dust. The distance to the comet from the Earth was approx. 600 million km. In PR Photo 06b/04 , the exposures have been combined to show the background objects in real colours. Because of its motion, the comet now appears as a trail. Technical information about the photos is available below. |
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In the morning of March 2, the Rosetta spacecraft was launched on board an Ariane-5 launcher from the European Spaceport in Kourou, French Guiana. The European Space Agency (ESA) spacecraft will be the first to land on a comet.
Before the launch, and as a salute to their colleagues at ESA, astronomers used the New Technology Telescope at the European Southern Observatory (ESO) of La Silla in Chile to image Rosetta's target, Comet 67P/Churyumov-Gerasimenko, an approximately 4 kilometre size "dirty snowball" that orbits the Sun once every 6.6 years.
These new images show the object at a distance of approximately 670 million kilometres from the Sun - 4.5 times the distance from the Earth to the Sun.
These observations provide further confirmation that at this distance the activity on 67P/Churyumov-Gerasimenko is very low.
This is very good news for the mission, because it means that when Rosetta will meet in 2014 its target comet, at 790 million kilometres from the Sun, there will not be so much dust near the nucleus to hinder the landing.
Originally timed to begin about a year ago, Rosetta's journey had to be postponed. This delay meant that the original mission's target, Comet Wirtanen, which was observed two years ago by astronomers using ESO's Very Large Telescope (see ESO PR Photo 06/02) could no longer be reached. Instead, a new target has been selected, Comet Churyumov-Gerasimenko.
The observations presented here are part of a continuous effort by astronomers to monitor Rosetta's target and provide the spacecraft controllers and the astronomers with very useful, regular updates, e.g., about the 'cometary weather' at the time of arrival.
More information
Additional information concerning ESA's Rosetta mission can be found on the dedicated ESA web site.
Technical information about the photos
PR Photo 06a/04 is based on fourty-five exposures obtained by Olivier Hainaut and Mauricio Martinez (ESO) with the SuSI-2 camera on the 3.5-m NTT telescope at La Silla (Chile) in the morning of February 26, 2004. The comet was located in the southern constellation of Libra. The exposures were made through standard B, V and R-filtres and lasted in total 35 min in V, 35 min in R and 45 min in B. The measured magnitudes of the nucleus were approx. V = 22.3 and R = 21.6. North is to the right and east is down. The field in Photo 06a/04 measures approx. 1.0 x 1.0 arcmin2.