Sometimes it's near, sometimes it's far

Geometry Level 3

A planet revolves around its star in an elliptical orbit of eccentricity 0.6 0.6 , 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 r ap r_\text{ap} and r per r_\text{per} are the distances between the planet and the star at aphelion and perihelion respectively, then find r ap r per \dfrac{r_\text{ap}}{r_\text{per}} .


The answer is 4.

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1 solution

Julian Yu
Apr 5, 2019

Let c c be the distance between the center of the ellipse and the foci, and let a a be half the length of the major axis. The eccentricity of an ellipse is given by c a \dfrac{c}{a} .

By the conditions of the problem, c = 0.6 a c=0.6a .

The quantity that we are being asked for is a + c a c \dfrac{a+c}{a-c} , which is equal to a + 0.6 a a 0.6 a = 1.6 a 0.4 a = 4 . \dfrac{a+0.6a}{a-0.6a}=\dfrac{1.6a}{0.4a}=\boxed{4}.

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