A ``squashed'' Spheroid for which the equatorial radius  is greater than the polar radius
 is greater than the polar radius  , so
, so  .  To
first approximation, the shape assumed by a rotating fluid (including the Earth,
.  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),
 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
, and ![$v\in[0, \pi]$](o_14.gif) .  Its Cartesian equation is
.  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
 and expand up to Powers of  ,
,
Expanding  in Powers of Ellipticity to
 in Powers of Ellipticity to  therefore yields
 therefore yields
|  | (14) | 
 
In terms of Legendre Polynomials,
The Ellipticity may also be expressed in terms of the Oblateness (also called Flattening), denoted
 or
 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
 and expand up to Powers of  
Expanding  in Powers of the Oblateness to
 in Powers of the Oblateness to  yields
 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
-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
.  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
-axis by an Angle  so that the new symmetry axes for the spheroid are
 so that the new symmetry axes for the spheroid are  ,
,  , and
, and  .  The projected height of a point in the
.  The projected height of a point in the  Plane on the
 Plane on the  -axis is
-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) | 
 
| ![$[(1+k)\sqrt{1-x^2}\tan B-k x^2\sqrt{1-x^2}\tan B-x-kx+kx^3]$](o_81.gif)  |  | 
| ![$ +[kx(1-x^2)+kx^2\sqrt{1-x^2}\tan B]\quad$](o_82.gif)  | (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
 in terms of  and
 and  ,
,
|  | (42) | 
 
Combine (30) and (31) and plug in for  ,
,
Now re-express  in terms of
 in terms of  and
 and  , using
, 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
-axis by Angle  , then the
, then the
 -axis by Angle
-axis by Angle  
Now, in the original coordinates  , the spheroid is given by the equation
, 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 (
, the radial distance from the symmetry axis of the spheroid ( ) corresponding to
a point
) corresponding to
a point
|  | (57) | 
 
where
 can now be computed using the quadratic equation when
 can now be computed using the quadratic equation when  is given,
 is given,
|  | (60) | 
 
If  , then we have
, then we have  and
 and  , so (51) to (56) and 
(58) to (59) become
, 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