Artificial satellites, minor planets, and the ETS

Details Artificial satellites, minor planets, and the ETS Artificial satellites, minor planets, and the ETS

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8112143b&link_type=abstract

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Computer Science

Artificial Satellites, Asteroids, Optical Countermeasures, Satellite Tracking, Signal Processing, Space Surveillance (Spaceborne), Target Recognition, Analysis Of Variance, Brightness, Detection, Photometry

Scientific paper

This report summarizes the successful modification of Lincoln Laboratory's Experimental Test System hardware and software for the detection and discrimination of asteroids rather than artificial satellites. The minor planets are found by exploiting their proper motion and the limiting magnitude is roughly brightness magnitude = 17.5. The complete observing cycle, including the 2 - 3 sec measurement of position, requires about four minutes at present. The commonality of asteroids and artificial satellite observing, searching, data reduction, orbital analysis, and lightcurve analysis is stressed.

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