Publication Date:
2019-07-13
Description:
A satellite being designed by the Stanford University to measure (with extremely high precision) the effect of General Relativity is described. Specifically, the satellite will measure two relativistic precessions predicted by the theory: the geodetic effect (6.9 arcsec/yr), due solely to motion about the earth, and the motional effect (0.05 arcsec/yr), due to rotation of the earth. The gyro design requirements, including the requirement for precise attitude control and a dynamic model for attitude control synthesis, are discussed. Closed loop simulation of the satellite's natural dynamics on an analog computer is described.
Keywords:
SPACE VEHICLES
Type:
Joint Automatic Control Conference; Jun 20, 1973 - Jun 22, 1973; Columbus, OH
Format:
text
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