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Difference between revisions of "Ellipse"

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An '''ellipse''' is a [[conic section]] formed by cutting through a [[cone]] at an [[angle]].  Equivalently, it is defined as the [[locus]], or [[set]], of all [[point]]s <math>P</math> such that the sum of the distances from <math>P</math> to two fixed foci (singular [[focus]]) is a constant.  (The equivalence of these two definitions is a non-trivial fact.)
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An '''ellipse''' is a [[conic section]] formed by cutting through a [[cone]] at an [[angle]].  Equivalently, it is defined as the [[locus]], or [[set]], of all [[point]]s <math>P</math> such that the sum of the distances from <math>P</math> to two fixed [[focus|foci]] is a constant.  (The equivalence of these two definitions is a non-trivial fact.)
  
 
Ellipses tend to resemble [[circle]]s which have been "flattened" or "stretched."  They occur in nature as well as in mathematics: as was proven in [[Kepler's Laws]], the planets all revolve about the sun in elliptical, not circular, orbits with the sun at one of the foci.  Note that the circle is just a special case of the ellipse, just as a square is to a rectangle,  and occurs when (in the first definition) the cut is [[perpendicular]] to the axis of the the cone, or (in the second definition) the two foci of the ellipse coincide.
 
Ellipses tend to resemble [[circle]]s which have been "flattened" or "stretched."  They occur in nature as well as in mathematics: as was proven in [[Kepler's Laws]], the planets all revolve about the sun in elliptical, not circular, orbits with the sun at one of the foci.  Note that the circle is just a special case of the ellipse, just as a square is to a rectangle,  and occurs when (in the first definition) the cut is [[perpendicular]] to the axis of the the cone, or (in the second definition) the two foci of the ellipse coincide.

Revision as of 19:50, 24 February 2007

An ellipse is a conic section formed by cutting through a cone at an angle. Equivalently, it is defined as the locus, or set, of all points $P$ such that the sum of the distances from $P$ to two fixed foci is a constant. (The equivalence of these two definitions is a non-trivial fact.)

Ellipses tend to resemble circles which have been "flattened" or "stretched." They occur in nature as well as in mathematics: as was proven in Kepler's Laws, the planets all revolve about the sun in elliptical, not circular, orbits with the sun at one of the foci. Note that the circle is just a special case of the ellipse, just as a square is to a rectangle, and occurs when (in the first definition) the cut is perpendicular to the axis of the the cone, or (in the second definition) the two foci of the ellipse coincide.

For a given non-circular ellipse, there will be two points on the ellipse closest to the center and two points furthest away -- it will be "tall and skinny" or "short and fat." The segment connecting the center of the ellipse to one of the "farther away ends" is called the semimajor axis and the segment connecting the center to a closer end is called the semiminor axis. These two segments are perpendicular. Drawing all four semi-axes divides the ellipse into 4 congruent quarters.

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Using the second definition of an ellipse given above, one may easily construct an ellipse from household materials. To draw an ellipse with two pushpins, a loop of string, pencil, and paper, stick the pushpins in the paper place the string on the paper so that both pushpins are inside it. The pushpins will be the foci of the ellipse, and the length of the string will determine the sum of the distances from a point on the ellipse to the two foci. Hold the pencil on the paper such that the string is taut against the pencil tip and the two pushpins. Then move the pencil tip while keeping the string taut. This will traces out an ellipse.

An ellipse in a Cartesian coordinate system with center $C = (h, k)$ whose axes are parallel to the coordinate axes, with the vertical semi-axis of length $a$ and the horizontal semi-axis of length $b$ is given by the equation $\frac{(x-h)^2}{a^2}+\frac{(y-k)^2}{b^2}=1$. In particular, if the center of the ellipse is the origin this simplifies to $\frac{x^2}{a^2}+\frac{y^2}{b^2}=1$.

The three-dimensional counterpart of the ellipse is the ellipsoid.

See also

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