Ellipticity
Flattening is a measure of the compression of a circle or sphere along a diameter to form an ellipse or an ellipsoid of revolution (spheroid) respectively. Other terms used are ellipticity, or oblateness. The usual notation for flattening is f and its definition in terms of the semi-axes of the resulting ellipse or ellipsoid is
The compression factor is b/a in each case. For the ellipse, this factor is also the aspect ratio of the ellipse.
There are two other variants of flattening (see below) and when it is necessary to avoid confusion the above flattening is called the first flattening. The following definitions may be found in standard texts and online web texts
In the following, a is the larger dimension (e.g. semimajor axis), whereas b is the smaller (semiminor axis). All flattenings are zero for a circle (a=b).
The flattenings are related to other parameters of the ellipse. For example:
where is the eccentricity.
For the WGS84 ellipsoid to model Earth, the defining values are
from which one derives
so that the difference of the major and minor semi-axes is 21.385 km (13 mi). (This is only 0.335% of the major axis, so a representation of Earth on a computer screen would be sized as 300px by 299px. Because this would be virtually indistinguishable from a sphere shown as 300px by 300px, illustrations typically greatly exaggerate the flattening in cases where the image needs to represent Earth's oblateness.)
Other values in the Solar System are Jupiter, f=1/16; Saturn, f= 1/10, the Moon f= 1/900. The flattening of the Sun is about 9×10−6.
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