An apse line, or line of apsides, is an imaginary line defined by an orbit's eccentricity vector. It is strictly defined for elliptic, parabolic, and hyperbolic orbits.

The line of apsides of an ellipse connects point 2 and 3 (major axis).

For such orbits the apse line is found:[1]

For circular orbits, the apse line is not defined because the eccentricity is equal to zero. As it is required as a base for the definition of true anomaly, it is usually arbitrarily assumed (as a line pointing into the direction of the vernal equinox).

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References

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  1. ^ "Line of apsides – Astronomy". Encyclopædia Britannica. Retrieved 23 August 2015.