 |  |  |  |  |
| |  | |  | |
 |
Palvelut KalenteriRSS feeds Tilaa
|  |  |  |  | | | Steins-asteroidin pimeä puoli kartoitettu suomalaisvoimin 8 tammikuuta 2010
 | An animation of the closest approach of Rosetta to asteroid Steins, taken with the OSIRIS imaging system’s Wide Angle Camera. The image sequence starts 3 minutes before closest approach, from a distance of about 2000 km and ends 4 minutes after closest approach. At the start of the animation, the sun illuminated the asteroid from behind the spacecraft and no shadows are visible on the its surface. Later, the sunlight is incident from the left, and craters and more surface features become visible.
Credits: ESA ©2008 MPS for OSIRIS Team MPS/UPD/LAM/IAA /RSSD/INTA/UPM/DASP/IDA |  |  |  |  |
| | | |  |
Credits: Science Mag Jan 2010 / Kaasalainen |  |  |  |  |
| | | | Inversio-ongelma
 | The animation is composed of images that were used for the optical navigation campaign, as Rosetta followed (2867) Steins, refining its trajectory to close in on the asteroid. They were taken once a day by Navigation camera A, between 25 August and 3 September.
The images have been adjusted so that the stars are of roughly the same brightness from day to day, although the exposure times decrease and Steins becomes brighter as Rosetta appoaches.
Credits: ESA |  |  |  |  |
| | | | Seuraavaksi kiikarissa Lutetia
 | Brightness variation of the asteroid measured continuously over one day. The maximum in the light curve is about 23 percent brighter than the minimum.
Credits: Stefano Mottola (DLR), OSIRIS team |  |  |  |  |
| | | | | |
|  | ESA's comet chaser Aiheeseen liittyviä artikkeleita Steins: A diamond in the skyRosetta spacecraft meets asteroid SteinsRosetta fly-by of Steins: Orbit animationAiheeseen liittyviä linkkejä Science-lehden artikkeli 8.1.2010: H.U. Keller et al. "E-type asteroid (2867) Steins as imaged by OSIRIS on board Rosetta"Tampereen teknillinen yliopisto, Matematiikan laitos
|