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
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(4) |
The Ellipticity of an oblate spheroid is defined by
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(5) |
so that
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(6) |
Then the radial distance from the rotation axis is given by
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(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
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(10) |
Define and expand up to Powers of ,
Expanding in Powers of Ellipticity to therefore yields
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(14) |
In terms of Legendre Polynomials,
The Ellipticity may also be expressed in terms of the Oblateness (also called Flattening), denoted
or .
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(16) |
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(17) |
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(18) |
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(19) |
so
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(20) |
and
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(21) |
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(22) |
Define and expand up to Powers of
Expanding in Powers of the Oblateness to yields
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(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
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(28) |
Define
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(29) |
and
. Then
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(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,
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(32) |
Simplifying,
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(33) |
But
Plugging (34) into (33),
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(35) |
and performing a number of algebraic simplifications
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(36) |
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(37) |
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(38) |
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(39) |
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(40) |
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(41) |
finally gives the expression for in terms of and ,
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(42) |
Combine (30) and (31) and plug in for ,
Now re-express in terms of and , using
,
so
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(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
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(48) |
which becomes in the new coordinates,
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(49) |
Collecting Coefficients,
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(50) |
where
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(51) |
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(52) |
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(53) |
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(54) |
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(55) |
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(56) |
If we are interested in computing , the radial distance from the symmetry axis of the spheroid () corresponding to
a point
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(57) |
where
can now be computed using the quadratic equation when is given,
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(60) |
If , then we have and , so (51) to (56) and
(58) to (59) become
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(61) |
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(62) |
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(63) |
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(64) |
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(65) |
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(66) |
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(67) |
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(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