Rosetta flies by asteroid Steins - campaign overview
Asteroid Steins is the first nominal scientific target for the Rosetta mission. The spacecraft will rendezvous with the asteroid in the course of its first incursion into the asteroid belt located between the orbits of Mars and Jupiter, while on its way to its primary scientific target, comet 67/P Churyumov-Gerasimenko.
End of Steins fly-by campaign
The asteroid Steins fly-by campaign ended on 4 October 2008 at which time the spacecraft was configured to low activity cruise. The two weeks following the fly-by were mostly devoted to downloading the science data recorded during the fly-by and making observations for the OSIRIS gravitational microlensing programme. Further details are given in:
Rosetta’s gravitational microlensing programmeRosetta Status Report No. 105 - Gravitational Microlensing Observations
Rosetta Status Report No. 106 - Gravitational Microlensing Observations Completed
First images and results from the fly-by campaign
First images and results from the fly-by of asteroid Steins were presented at a press conference on Saturday 6 September starting at 12:00 CEST. For further details see:
First Rosetta/OSIRIS images of asteroid Steins
Science instruments ready for action
Nearly all of the orbiter’s instruments and the ROMAP magnetometer on the lander performed scientific measurements. In the four weeks leading up to the moment of closest approach the asteroid was imaged by the navigation cameras and by the OSIRIS camera as part of an optical navigation campaign aimed at fine-tuning the trajectory of the spacecraft. Most of the scientific observations were performed in the few hours around closest approach, although some measurements began a few days before. See also:
Rosetta's scientific instruments prepare for close encounter with SteinsOptical navigation campaign - fine-tuning the spacecraft trajectory
For the month preceding closest approach to asteroid Steins the spacecraft navigation cameras and the OSIRIS camera performed an optical navigation campaign. The purpose of this was to refine the trajectory of the spacecraft relative to the asteroid and to adjust it, if necessary, to achieve the desired fly-by conditions: 800 km distance at closest approach on 5 September at 18:58 UTC and zero phase angle reached prior to closest approach. Further details can be read in the article:
Rosetta fine-tunes its approach to asteroid SteinsFirst results from the optical navigation campaign are available and are reported in:
Optical navigation campaign off to a good start
and
Perfect sight: Rosetta cameras track asteroid target
Details of the trajectory correction manoeuvres, including results from the measurements made to determine the position of the asteroid plus images from the navigation cameras and OSIRIS, can be found in:
Rosetta Status Report No. 102 - Start of Optical Navigation Campaign
Rosetta Status Report No. 103 - Closing in on Asteroid Steins
Rosetta Status Report No. 104 - Asteroid Steins Fly-by
Preparing for the encounter with asteroid Steins
Preparations for the fly by began on 1 July 2008 when the Rosetta spacecraft was taken out of near-Sun hibernation mode and configured to active cruise mode. The spacecraft and payload were then checked out prior to the start of the optical navigation campaign. You can read more about the preparatory activities in:
Preparations underway for Rosetta flyby of asteroid Steins
Rosetta Status Report No. 99 - Switch to Active Cruise Mode
Rosetta Status Report No. 100 - Active Payload Check-out 8
Rosetta Status Report No. 101 - Active Payload Checkout 8 Completed