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IEVref:725-11-38ID:
Language:enStatus: Standard
Term: sidereal period of revolution (of a satellite)
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Definition: the time elapsing between two consecutive intersections of the projection of a satellite on to a reference plane which passes through the centre of mass of the primary body with a line in that plane extending from the centre of mass to infinity, the normal to the reference plane and the direction of the line both being fixed in relation to the stars


Publication date:1994-08
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