The angle obtained by drawing the auxiliary circle of an ellipse with center and focus
, and drawing a line perpendicular
to the semimajor axis and intersecting
it at
.
The angle
is then defined as illustrated above. Then for an ellipse
with eccentricity
,
|
(1)
|
But the distance
is also given in terms of the distance from the focus
and the supplement
of the angle from the semimajor
axis
by
|
(2)
|
Equating these two expressions gives
|
(3)
|
which can be solved for to obtain
|
(4)
|
To get
in terms of
,
plug (◇) into the equation of the ellipse
|
(5)
|
Rearranging,
|
(6)
|
and plugging in (◇) then gives
|
(7)
| |||
|
(8)
|
Solving for
gives
|
(9)
|
so differentiating yields the result
|
(10)
|
The eccentric anomaly is a very useful concept in orbital mechanics, where it is related to the so-called mean anomaly by Kepler's equation
|
(11)
|
can also be interpreted as the area of the shaded region
in the above figure (Finch 2003).