A ``squashed'' Spheroid for which the equatorial radius
is greater than the polar radius
, so
. To
first approximation, the shape assumed by a rotating fluid (including the Earth,
which is ``fluid'' over
astronomical time scales) is an oblate spheroid. The oblate spheroid can be specified parametrically by the usual
Spheroid equations (for a Spheroid with z-Axis as the symmetry axis),
with
,
, and
. Its Cartesian equation is
 |
(4) |
The Ellipticity of an oblate spheroid is defined by
 |
(5) |
so that
 |
(6) |
Then the radial distance from the rotation axis is given by
 |
(7) |
as a function of the Latitude
.
The Surface Area and Volume of an oblate spheroid are
An oblate spheroid with its origin at a Focus has equation
 |
(10) |
Define
and expand up to Powers of
,
Expanding
in Powers of Ellipticity to
therefore yields
 |
(14) |
In terms of Legendre Polynomials,
The Ellipticity may also be expressed in terms of the Oblateness (also called Flattening), denoted
or
.
 |
(16) |
 |
(17) |
 |
(18) |
 |
(19) |
so
 |
(20) |
and
 |
(21) |
![\begin{displaymath}
r = a\left[{1 + {2\epsilon -\epsilon^2\over (1-\epsilon)^2} \sin^2\delta}\right]^{-1/2}.
\end{displaymath}](o_50.gif) |
(22) |
Define
and expand up to Powers of
Expanding
in Powers of the Oblateness to
yields
 |
(26) |
In terms of Legendre Polynomials,
To find the projection of an oblate spheroid onto a Plane, set up a coordinate system such that the z-Axis is
towards the observer, and the
-axis is in the Plane of the page. The equation for an oblate spheroid is
![\begin{displaymath}
r(\theta)=a\left[{1+{2\epsilon-\epsilon^2 \over (1-\epsilon)^2}\cos^2\theta}\right]^{-1/2}.
\end{displaymath}](o_62.gif) |
(28) |
Define
 |
(29) |
and
. Then
![\begin{displaymath}
r(\theta) =a[1+k(1-x^2)]^{-1/2} = a(1+k-kx^2)^{-1/2}.
\end{displaymath}](o_65.gif) |
(30) |
Now rotate that spheroid about the
-axis by an Angle
so that the new symmetry axes for the spheroid are
,
, and
. The projected height of a point in the
Plane on the
-axis is
To find the highest projected point,
 |
(32) |
Simplifying,
 |
(33) |
But
Plugging (34) into (33),
![\begin{displaymath}
{\sqrt{1-x^2}\tan B-x \over\sqrt{1-x^2}+x\tan B} [1+k(1-x^2)]+kx\sqrt{1-x^2} = 0
\end{displaymath}](o_79.gif) |
(35) |
and performing a number of algebraic simplifications
 |
(36) |
|
|
|
(37) |
 |
(38) |
 |
(39) |
 |
(40) |
![\begin{displaymath}
x^2[1+(1+k)^2\tan^2 B]=(1+k)^2\tan^2 B
\end{displaymath}](o_86.gif) |
(41) |
finally gives the expression for
in terms of
and
,
 |
(42) |
Combine (30) and (31) and plug in for
,
Now re-express
in terms of
and
, using
,
so
 |
(45) |
Plug (44) and (45) into (43) to obtain the
Semiminor Axis of the projected oblate spheroid,
We wish to find the equation for a spheroid which has been rotated about the
-axis by Angle
, then the
-axis by Angle
Now, in the original coordinates
, the spheroid is given by the equation
 |
(48) |
which becomes in the new coordinates,
|
|
|
(49) |
Collecting Coefficients,
 |
(50) |
where
 |
 |
 |
(51) |
 |
 |
 |
(52) |
 |
 |
 |
(53) |
 |
 |
 |
|
|
 |
 |
(54) |
 |
 |
 |
(55) |
 |
 |
 |
(56) |
If we are interested in computing
, the radial distance from the symmetry axis of the spheroid (
) corresponding to
a point
 |
(57) |
where
can now be computed using the quadratic equation when
is given,
 |
(60) |
If
, then we have
and
, so (51) to (56) and
(58) to (59) become
 |
 |
 |
(61) |
 |
 |
 |
(62) |
 |
 |
 |
(63) |
 |
 |
 |
(64) |
 |
 |
 |
(65) |
 |
 |
 |
(66) |
 |
 |
 |
(67) |
 |
 |
 |
|
|
 |
 |
(68) |
See also Darwin-de Sitter Spheroid, Ellipsoid, Oblate Spheroidal Coordinates, Prolate Spheroid,
Sphere, Spheroid
References
Beyer, W. H. CRC Standard Mathematical Tables, 28th ed. Boca Raton, FL: CRC Press, p. 131, 1987.
© 1996-9 Eric W. Weisstein
1999-05-26