# How do you calculate the aphelion and perihelion of a comet's orbit if it has an orbital period of 83 years and an eccentricity of .875?

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Using Kepler's 3rd law the perihelion distance is about 2.375AU and the aphelion distance is about 35.625AU.

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Kepler's 3rd law enables an approximate calculation of the size of the comet's orbit. The actual obit will not be a true ellipse due to the gravitational effect of other bodies in the solar system.

Kepler's 3rd law states that the square of the orbital period divided by the cube of the cube of the semi-major axis of the orbit is a constant. For our solar system if the period T is in years and the semi-major a axis is in Astronomical Units, then the constant is one. Then

The Astronomical Unit is based on the distance of the Earth from the Sun. Earths period

For the comet with a period of

The perihelion distance

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