ага, вот информация с официального сайта - 
http://www.esa.int/SPECIALS/Rosetta/SEMR7IBE8YE_0.html 23 February 2007
The timeline for Rosetta's speedy swingby of Mars on 25 February includes a series of slew manoeuvres, an occultation and signal blackout, an eclipse and some excellent opportunities for scientific observations. 
Rosetta's Mars swingby kicks off today with a series of complex slew manoeuvres to enable instrument calibration. The spacecraft has been correctly lined up on the proper trajectory since a series of engine firings in the past several weeks. 
Rosetta is expected to pass the Red Planet at 250 km altitude and 36 191 km/hour with respect to Mars at closest approach. The swingby should reduce Rosetta's velocity with respect to the Sun by 7887 km/hour, and the spacecraft should depart Mars travelling at 78 779 km/hour relative to the Sun.   
Timeline of major activities 
Note: Times shown are ground event times in Central European Time, equivalent to UTC (Coordinated Universal Time) + 1 hour. Spacecraft event time is 17 mins 33 secs earlier.   
23 February 
17:32 First of a series of slew manoeuvres to perform instrument calibrations 
19:30 Flight Control Team in ESOC's Main Control Room (MCR) around the clock 
24 February  
 View from Earth: Rosetta passing Mars 
~14:00 Webcam in MCR switched on (access via ESA portal) 
18:35 Additional slew manoeuvres to perform Mars observations with onboard instruments 
22:30 End of observations until after Mars swingby   
25 February 
02:15 -- All payload instruments switched off; CIVA camera (onboard lander) remains in operation and scheduled to take images
-- Loss of telemetry; S-band carrier signal remains 
03:13 -- Occultation starts; Rosetta behind Mars
-- Loss of S-band signal; no communication with spacecraft 
03:15 -- Closest approach to Mars (250 km)
-- Start of eclipse; no visibility for camera; no sunlight on solar panels 
03:28 -- End of occultation; S-band carrier signal back
-- Receipt of S-band carrier signal provides initial technical confirmation of swingby success 
03:40 End of eclipse; sunrise above Mars 
03:50 Start of Phobos and Mars tracking with additional scientific observations 
03:52 -- Acquisition of telemetry (radio signal & data); full technical confirmation of swingby success
-- Downloading of data and images begins 
After 13:00 Images to be available on ESA portal       
 New Norcia: ESA's first 35m deep-space station 
ESA/NASA interagency cooperation supports Rosetta 
Increased ground tracking support has been scheduled throughout the swingby period. 
In addition to ESA's 35m deep-space station at New Norcia, NASA's Deep Space Network (DSN) stations at Goldstone, Canberra and Madrid will participate. 
The two agencies often work together and regularly share tracking station resources.