The star camera is currently being commissioned. Below is a picture taken by the camera with four stars indicated that were extracted by the on-board algorithm used to detect valid stars.
03 February 2010
01 February 2010
GPS commissioned
The graph below shows the telemetry from the on-board GPS over three orbits. The bottom trace indicates a valid "lock"; the yellow trace the number of satellites tracked; and the top three traces the X,Y,Z position vectors.
In a perfectly circular orbit, the satellite velocity would be constant. In a near-circular orbit (as is the case with Sumbandila), the velocity fluctuates slightly between a minimum at Apogee and a maximum at Perigee. This effect is clearly visible in the measured velocity data from the GPS (see below). It shows a difference of 30m/s between Apogee and Perigee. Also note the very low level of "noise" on the measurement.
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Current Keplerian Elements
Last Update: 1 Febr 2010
Element set: 404
Sumbandila 1 35870U 09049F 10032.48635300 .00000433 00000-0 21444-4 0 4040 2 35870 097.3525 084.8560 0011505 166.1189 300.7196 15.22856092 20818