MEAN Anomaly of a Planet, is an angle which is always proportional to the time of the planet's motion from the aphelion or perihelion, or proportional to the area described by the radius vector; that is, as the whole periodic time is one revolution of the planet, so to the time past the aphelion or perihelion, so is 360° to the mean anomaly. See ANOMALY, Encycl.
MEAN Anomaly of a Planet
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