Apse line
.png)
The line of apsides of an ellipse connects point 1 and 2 (major axis).
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.
For such orbits the apse line is found:[1]
- for elliptical orbits – between the orbit's periapsis and apoapsis (also known as the major axis)
- for parabolic and hyperbolic orbits – between the orbit's periapsis and focus
For circular orbits apse line is not defined, because 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).
See also
- Apsidal precession
- Apsis
- Eccentricity (orbit)
- Orbit: circular, elliptic, parabolic and hyperbolic
- True anomaly
References
- ↑ "Line of apsides – Astronomy". Encyclopaedia Britannica. Retrieved August 2015. Check date values in:
|access-date=(help)
This article is issued from Wikipedia - version of the 6/29/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.