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An oblate spheroid is an ellipsoid having a shorter axis and two equal longer axes (see the spheroid page for a picture). Oblateness is a measure for a planet that is a spheroid in shape, bulging outward in the center due to its rotation. Effectively the (fictitious) centrifugal force fights against gravity causing the planet to look more like a sphere stretched at the equator. Mathematically, oblateness may be defined as
where <math>R_{e}<math> the equatorial radius and <math>R_{p}<math> is the polar radius. The approximation is valid in the case of a fluid planet of uniform density; it is a function of the Newtonian constant of gravitation <math>G<math>, the rotation period <math>T<math> and the density <math>\rho<math>. |
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