... In less then one day "Mir" station will finish its flight. ... Besides, the operability of motion control systems will be tested to ensure further dynamic operation at the final stage of "Mir" complex. ... The final third burn is given in daily orbit 2 using the "ProgressM1-5" 8 control engines and its main engine with the trust of 300 rg/s. Thus, to peform deorbit maneuver the OC"MIr" real-time tested manuevers involving control engines and their combination with the main engine are used. ...

ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: RECENT PROGRESS AND NEW HORIZONS 4-th GAMOW INTERNATIONAL CONFERENCE IN ODESSA and 9-th GAMOW SUMMER SCHOOL Astronomy and beyond: Astrophysics, Cosmology, Radioastronomy, High Energy Physics and Astrobiology 17-23 August , 2009, Odessa, Ukraine EVENTS: Monday, 17.08.2009 Arrival 09.00 ­ 22.00 Registration of participants Tuesday, 18.08.2009 05.59 09.00 10.00 11.00 13.00 13.15 14.30 16.00 ...

University Satellites and . Space Science Education . ... Simulation of Carrier Phase GPS Observables and Feasible Attitude Determination Algorithms for Universitetskiy-Tatyana Satellite . ... Carrier phase observables of radio signals transmitted by navigation satellites, when obtained from multiple antennas, potentially could provide the most accurate and stable solution for attitude determination among other methods. ...

... The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorption lines where discovered in 1802 by the English scientist William Wollaston. ... Some stars as Pollux show a spectrum similar to that of our sun with strong Ca II and Fe II lines, others as Sirius or Vega show strong absorption lines of hydrogen, others, as Mira show very complicated spectra due to molecular absorption lines (see figure 5). ...

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