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Kepler’s laws of planetary motion
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Kepler’s laws of planetary motion Article

What is eccentricity and how is it determined?

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The eccentricity of an ellipse measures how flattened a circle it is. It is equal to the square root of [1 - b*b/(a*a)]. The letter a stands for the semimajor axis, ½ the distance across the long axis of the ellipse. The letter b stands for the semiminor axis, ½ the distance across the short axis of the ellipse. For a perfect circle, a and b are the same such that the eccentricity is zero. Earth’s orbit has an eccentricity of 0.0167, so it is very nearly a perfect circle.

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