|oblate spheroid||prolate spheroid|
If the ellipse is rotated about its major axis, the result is a prolate (elongated) spheroid, like an American football or rugby ball. If the ellipse is rotated about its minor axis, the result is an oblate (flattened) spheroid, like a lentil. If the generating ellipse is a circle, the result is a sphere.
Because of the combined effects of gravitation and rotation, the Earth's shape is roughly that of a sphere slightly flattened in the direction of its axis. For that reason, in cartography the Earth is often approximated by an oblate spheroid instead of a sphere. The current World Geodetic System model uses a spheroid whose radius is 6,378.137 km at the equator and 6,356.752 km at the poles.
The word spheroid originally meant an approximately spherical body, admitting irregularities even beyond the bi- or tri-axial ellipsoidal shape, and that is how it is used in some older papers on geodesy (for example, referring to truncated spherical harmonic expansions of the Earth). In case there is risk of confusion, it is beneficial to state for clarity the one definition intended.
The equation of a tri-axial ellipsoid centred at the origin with semi-axes a,b, c aligned along the coordinate axes is
The equation of a spheroid with Oz as the symmetry axis is given by setting a=b:
The semi-axis a is the equatorial radius of the spheroid, and c is the distance from centre to pole along the symmetry axis. There are two possible cases:
- c < a : oblate spheroid
- c > a : prolate spheroid
The case of a=c reduces to a sphere.
An oblate spheroid with c < a has surface area
The oblate spheroid is generated by rotation about the Oz axis of an ellipse with semi-major axis a and semi-minor axis c, therefore e may be identified as the eccentricity. (See ellipse). A derivation of this result may be found at.
A prolate spheroid with c > a has surface area
The prolate spheroid is generated by rotation about the Oz axis of an ellipse with semi-major axis c and semi-minor axis a, therefore e may again be identified as the eccentricity. (See ellipse). A derivation of this result may be found at.
These formulas are identical in the sense that the formula for can be used to calculate the surface area of a prolate spheroid and vice versa. However, e then becomes imaginary and can no longer directly be identified with the eccentricity. Both of these results may be cast into many other forms using standard mathematical identities and relations between parameters of the ellipse.
The volume inside a spheroid (of any kind) is . If A=2a is the equatorial diameter, and C=2c is the polar diameter, the volume is .
If a spheroid is parameterized as
and its mean curvature is
Both of these curvatures are always positive, so that every point on a spheroid is elliptic.
The aspect ratio of an oblate spheroid/ellipse, b:a, is the ratio of the polar to equatorial lengths, while the flattening (also called oblateness) f, is the ratio of the equatorial-polar length difference to the equatorial length:
These are just two of several different parameters used to define an ellipse and its solid body counterparts.
The most common shapes for the density distribution of protons and neutrons in an atomic nucleus are spherical, prolate and oblate spheroidal, where the polar axis is assumed to be the spin axis (or direction of the spin angular momentum vector). Deformed nuclear shapes occur as a result of the competition between electromagnetic repulsion between protons, surface tension and quantum shell effects.
The oblate spheroid is the approximate shape of many planets and celestial bodies, including Saturn and Altair; in particular, cartographic and geodetic systems for the Earth are based on a reference ellipsoid.
The prolate spheroid is the shape of the ball in several sports, such as in rugby union, rugby league, and Australian rules football. In American football and Canadian football, a more pointed prolate spheroid is used (one resembling a vesica piscis in cross section).
Several moons of the Solar system approximate prolate spheroids in shape, though they are actually triaxial ellipsoids. Examples are Mimas, Enceladus, and Tethys (satellites of Saturn) and Miranda (a satellite of Uranus). In contrast to being distorted into oblate spheroids via rapid rotation, celestial objects distort slightly into prolate spheroids via tidal forces when they orbit a massive body in a close orbit. The most extreme example is Jupiter's moon Io, which becomes slightly more or less prolate in its orbit due to a slight eccentricity, causing spectacular volcanism. It should be noted that the major axis of the prolate spheroid does not run through the satellite's poles in this case, but through the two points on its equator directly facing toward and away from the primary. A famous example in science fiction is Jinx in Larry Niven's Known Space.
Many submarines have a shape which can be described as prolate spheroid.
|Wikimedia Commons has media related to Spheroids.|
- Torge, Geodesy, p.104
- "Oblate Spheroid - from Wolfram MathWorld". Mathworld.wolfram.com. Retrieved 2014-06-24.
- "Prolate Spheroid - from Wolfram MathWorld". Mathworld.wolfram.com. 2003-10-07. Retrieved 2014-06-24.
- See 2008 NCAA Football Rules and Interpretations, Sec. 1, Art. 1
- Trimble, Virginia Louise (October 1973), "The Distance to the Crab Nebula and NP 0532", Publications of the Astronomical Society of the Pacific 85 (507): 579, Bibcode:1973PASP...85..579T, doi:10.1086/129507