Design, manufacture and testing of a medium accuracy star tracker

Astronomy and Astrophysics – Astronomy

Scientific paper

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Ccd Star Tracker, Flight Tests, Product Development, Breadboard Models, Centroids, Gamma Ray Astronomy, Noise Reduction, Sensitivity, Signal To Noise Ratios, Target Acquisition

Scientific paper

The development, manufacturing, and testing of a CCD bright star sensor breadboard model are summarized. Adaptation potential of the model for faint star tracking; and applicability of photon event centroiding techniques to point source centroiding are discussed. A model was flown on a balloon to detect gamma ray sources. Equipment failures prevented utilization of ground recordings, but it is probable that the payload structure reached 60 C instead of the 10 to 15 C specified, allowing the sensor to see bright stars only. Postflight tests confirm that sensor performance meets design requirements: + 6 visual magnitude sensitivity; 28 sec target acquisition time (max); 25 updates/sec in tracking mode; 1.5 arcmin resolution; and 36 arcsec noise equivalent angle.

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