TOPICS
Search

Eccentric Anomaly


EccentricAnomaly

The angle obtained by drawing the auxiliary circle of an ellipse with center O and focus F, and drawing a line perpendicular to the semimajor axis and intersecting it at A. The angle E is then defined as illustrated above. Then for an ellipse with eccentricity e,

 AF=OF-AO=ae-acosE.
(1)

But the distance AF is also given in terms of the distance from the focus r=FP and the supplement of the angle from the semimajor axis v by

 AF=rcos(pi-v)=-rcosv.
(2)

Equating these two expressions gives

 r=(a(cosE-e))/(cosv),
(3)

which can be solved for cosv to obtain

 cosv=(a(cosE-e))/r.
(4)

To get E in terms of r, plug (◇) into the equation of the ellipse

 r=(a(1-e^2))/(1+ecosv).
(5)

Rearranging,

 r(1+ecosv)=a(1-e^2)
(6)

and plugging in (◇) then gives

r(1+(aecosE)/r-(ae^2)/r)=r+aecosE-e^2a
(7)
=a(1-e^2).
(8)

Solving for r gives

 r=a(1-ecosE),
(9)

so differentiating yields the result

 r^.=aeE^.sinE.
(10)

The eccentric anomaly is a very useful concept in orbital mechanics, where it is related to the so-called mean anomaly M by Kepler's equation

 M=E-esinE.
(11)

M can also be interpreted as the area of the shaded region in the above figure (Finch 2003).


See also

Eccentricity, Ellipse, Kepler's Equation

Explore with Wolfram|Alpha

References

Danby, J. M. Fundamentals of Celestial Mechanics, 2nd ed., rev. ed. Richmond, VA: Willmann-Bell, 1988.Finch, S. R. "Laplace Limit Constant." §4.8 Mathematical Constants. Cambridge, England: Cambridge University Press, pp. 266-268, 2003.Montenbruck, O. and Pfleger, T. Astronomy on the Personal Computer, 4th ed. Berlin: Springer-Verlag, p. 62, 2000.

Referenced on Wolfram|Alpha

Eccentric Anomaly

Cite this as:

Weisstein, Eric W. "Eccentric Anomaly." From MathWorld--A Wolfram Web Resource. https://mathworld.wolfram.com/EccentricAnomaly.html

Subject classifications