A planet revolves around its star in an elliptical orbit of eccentricity , the star being at one of the ellipse's foci.
The planet is said to be at aphelion when the distance between the planet and the star its maximum; at perihelion, when the distance between the star and the planet is minimum.
If and are the distances between the planet and the star at aphelion and perihelion respectively, then find .
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Let c be the distance between the center of the ellipse and the foci, and let a be half the length of the major axis. The eccentricity of an ellipse is given by a c .
By the conditions of the problem, c = 0 . 6 a .
The quantity that we are being asked for is a − c a + c , which is equal to a − 0 . 6 a a + 0 . 6 a = 0 . 4 a 1 . 6 a = 4 .