Rosetta's cometary goal now in sight
Rosetta is an amazing probe launched by the European Space Agency. In 2014 it will go into orbit around the comet 67P/Churyumov-Gerasimenko, and actually deploy a lander to sample the surface!
That rendezvous is still years away, but the target is now in sight: Rosetta has returned its first image of the comet.
Oh, very cool! The top image is the wide angle shot, showing a densely-populated star field toward the center of our galaxy; from Rosetta that's the direction to the comet. The second image zooms in a bit, and you can see some distant stars and nebulosity. The bottom one has been processed to remove the stars, and the nucleus of Churyumov-Gerasimenko stands out.
Note that this image was taken when Rosetta was still 163 million kilometers (100 million miles) from the comet -- that's more than the distance from the Earth to the Sun! That's why it took a total of 13 hours of exposure time to see the comet in these images; it's still extremely faint from that great distance.
These pictures are important for several reasons: they test the cameras, a critical event for the upcoming encounter; they provide navigation cues, allowing engineers to test if the position of the comet is where they expected it to be; and they give the scientists and engineers practice in dealing with the images from the probe.
Not that Rosetta has simply been coasting along; it's passed by the Earth, Mars, and even two asteroids -- Lutetia (see the gallery below of those spectacular images!) and Steins -- returning incredibly lovely pictures of these worlds.
Rosetta is already a very successful mission, and the best is yet to come.
Image credit: ESA 2011 MPS for OSIRIS-Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
Image gallery of Rosetta's flyby of the asteroid Lutetia
Related posts:
- Ten Things You Don't Know About Comets
- Rosetta takes some home pictures
- Earth from Rosetta
- Rosetta swings by Mars
Bad Astronomy Gallery
(click any image to see it full size)
This image, taken at closest approach, shows how battered and worn Lutetia is. Craters pockmark the surface, including several that are many kilometers across. Like the Martian moon Phobos, grooves line the surface, which may be from boulders rolling around, perhaps ejected from some of the craters when they were formed. They may alternatively be stress fractures from impacts; there is still a lively debate over what causes these features in small bodies.
Much of the surface appears smooth, indicating great age for this object. Over billions of years it's been assaulted by dust grains moving at incredible speeds, as well as the solar wind. This has essentially sandblasted the surface, taking - literally - the edge off of the rims of craters.
We have very few high-resolution images of asteroids, and the more we get, the more we learn about them. Given that every now and again we get hit by them, I'm a big fan of understanding them better.
Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
This series of pictures was taken as Rosetta approached Lutetia.
The first image in the upper left was taken about 9.5 hours before closest approach, when Rosetta was still 510,000 km (315,000 miles) from the asteroid - more distant than the Moon is from the Earth!
The last image (lower right) was obtained an hour and a half before the close encounter when the probe was still 81,000 km (50,000 miles) from Lutetia.
In the first image, details only about 20 km (12 miles) across can be seen, but that improves by almost a factor of 10 in the last image!
Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA