Eccentricity (mathematics): Difference between revisions
a circle is an ellipse, so, strictly speaking, the eccentricity of an ellipse is >= 0, not >0 as previously written. |
I added a sqrt in the arctan equation Zvi Ner (nerzvi@gmail.com) |
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For any ellipse, where the length of the [[ellipse|semi-major axis]] is <math>a\,\!</math>, and where the same of the [[ellipse|semi-minor axis]] is <math>b\,\!</math>, the eccentricity, ''e'', is the sine of the ''[[Angular eccentricity|'''angular eccentricity''']]'', <math>o\!\varepsilon\,\!</math>, the equation being: |
For any ellipse, where the length of the [[ellipse|semi-major axis]] is <math>a\,\!</math>, and where the same of the [[ellipse|semi-minor axis]] is <math>b\,\!</math>, the eccentricity, ''e'', is the sine of the ''[[Angular eccentricity|'''angular eccentricity''']]'', <math>o\!\varepsilon\,\!</math>, the equation being: |
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:: <math>o\!\varepsilon=\arccos\left(\frac{b}{a}\right)=2\arctan\left(\frac{a-b}{a+b}\right);\,\!</math> |
:: <math>o\!\varepsilon=\arccos\left(\frac{b}{a}\right)=2\arctan\left(\sqrt{\frac{a-b}{a+b}}\right);\,\!</math> |
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:::<math>e=\sin(o\!\varepsilon)=\sqrt{1-\frac{b^2}{a^2}};\,\!</math> |
:::<math>e=\sin(o\!\varepsilon)=\sqrt{1-\frac{b^2}{a^2}};\,\!</math> |
Revision as of 13:50, 10 October 2006
In mathematics, eccentricity is a parameter associated with every conic section. It can be thought of as a measure of how much the conic section deviates from being circular. In particular,
- The eccentricity of a circle is zero.
- The eccentricity of a (non-circle) ellipse is greater than zero and less than 1.
- The eccentricity of a parabola is 1.
- The eccentricity of a hyperbola is greater than 1 and less than infinity.
- The eccentricity of a straight line is infinity.
It is given by:
Where is the length of the semimajor axis of the section, the length of the semiminor axis, and k is equal to +1 for an ellipse, 0 for a parabola, and -1 for a hyperbola.
It is also called the first eccentricity when necessary to distinguish it from the second eccentricity, e', which is sometimes used for algebraic convenience. The second eccentricity is defined as:
And is related to the first eccentricity by the equation:
Ellipse
For any ellipse, where the length of the semi-major axis is , and where the same of the semi-minor axis is , the eccentricity, e, is the sine of the angular eccentricity, , the equation being:
The eccentricity is the ratio of the distance between the foci ( and ) to the major axis; i.e. .
Likewise, the second eccentricity, e', is the tangent of :
The term linear eccentricity is used for .
Straight Line
A straight line or line segment can be shown as an ellipse with a minor axis of length 0, causing to be 0. Entering this value of into the equation of eccentricity for an ellipse gives a value of 1.
Hyperbola
For any hyperbola, where the length of the semi-major axis is , and where the same of the semi-minor axis is , eccentricity is given by:
Surfaces
The eccentricity of a surface is the eccentricity of a designated section of the surface. For example, on a triaxial ellipsoid, the meridional eccentricity is that of the ellipse formed by a section containing both the longest and the shortest axes (one of which will be the polar axis), and the equatorial eccentricity is the eccentricity of the ellipse formed by a section through the centre, perpendicular to the polar axis (i.e. in the equatorial plane).