ellipse

An ellipse that is centered at the origin is the curve in the plane determined by

\\left(\\frac{x}{a}\\right)^{2}+\\left(\\frac{y}{b}\\right)^{2}=1,

(1)

where $a,b>0$ .

Below is a graph of the ellipse $\\displaystyle\\left(\\frac{x}{3}\\right)^{2}+\\left(\\frac{y}{2}\\right)^{2}=1$ :

The major axis of an ellipse is the longest line segment whose endpoints are on the ellipse. The minor axis of an ellipse is the shortest line segment through the midpoint of the ellipse whose endpoints are on the ellipse.

In the first equation given above, if $a=b$ , the ellipse reduces to a circle of radius $a$ , whereas if $a>b$ (as in the graph above), $a$ is said to be the major semi-axis length and $b$ the minor semi-axis length; i.e. (http://planetmath.org/Ie), the lengths of the major axis and minor axis are $2a$ and $2b$ , respectively.

More generally, given any two points $p_{1}$ and $p_{2}$ in the (Euclidean) plane and any real number $r$ , let $E$ be the set of points $p$ having the property that the sum of the distances from $p$ to $p_{1}$ and $p_{2}$ is $r$ ; i.e.,

E=\\left\\{p\\,|\\,r=\\lvert p-p_{1}\\rvert+|p-p_{2}\\rvert\\right\\}.

In terms of the geometric look of $E$ , there are three possible scenarios for $E$ : $E=\\varnothing$ , $E=\\overline{p_{1}p_{2}}$ , the line segment with end-points $p_{1}$ and $p_{2}$ , or $E$ is an ellipse. Points $p_{1}$ and $p_{2}$ are called foci of the ellipse; the line segments connecting a point of the ellipse to the foci are the focal radii belonging to that point. When $p_{1}=p_{2}$ and $r>0$ , $E$ is a circle. Under appropriate linear transformations (a translation followed by a rotation), $E$ has an algebraic appearance expressed in (1).

In polar coordinates, the ellipse is parametrized as

	$\\displaystyle x(t)$	$\\displaystyle=$	$\\displaystyle a\\cos t,$
	$\\displaystyle y(t)$	$\\displaystyle=$	$\\displaystyle b\\sin t,\\quad t\\in[0,\\,2\\pi).$

If $a>b$ , then $t$ is the eccentric anomaly; i.e., the polar angle of the point on the circumscribed circle having the same abscissa as the point of the ellipse.

Properties

1.
If $a>b$ , the foci of the ellipse (1) are on the $x$ -axis with distances $\\sqrt{a^{2}-b^{2}}$ from the origin. The constant sum of the of a point $p$ is equal to $2a$ .
2.
The normal line of the ellipse at its point $p$ halves the angle between the focal radii drawn from $p$ .
3.
The area of an ellipse is $\\pi ab$ . (See this page (http://planetmath.org/AreaOfPlaneRegion).)
4.
The length of the perimeter of an ellipse can be expressed using an elliptic integral.

Eccentricity

By definition, the eccentricity $\\epsilon$ ( $0\\leq\\epsilon<1$ ) of the ellipse is given by

\\epsilon=\\frac{\\sqrt{a^{2}-b^{2}}}{a}\\cdot

For $\\epsilon=0$ , the ellipse reduces to a circle. Further, $b=a\\sqrt{1-\\epsilon^{2}}$ , and by assuming that foci are located on $x$ -axis, $p_{1}$ on $x<0$ and $p_{2}$ on $x>0$ , then $|O-p_{1}|=|O-p_{2}|=\\epsilon a$ , where $O(0,0)$ is the origin of the rectangular coordinate system.

Polar equation of the ellipse

By translating the $y$ -axis towards the focus $p_{1}$ , we have

	$\\displaystyle x^{\\prime}$	$\\displaystyle=$	$\\displaystyle x+\\epsilon a,$
	$\\displaystyle y^{\\prime}$	$\\displaystyle=$	$\\displaystyle y,$

but from (1) we get

\\left(\\frac{x^{\\prime}-\\epsilon a}{a}\\right)^{2}+\\left(\\frac{y^{\\prime}}{b}%\\right)^{2}=1.

(2)

By using the transformation equations to polar coordinates

	$\\displaystyle x^{\\prime}$	$\\displaystyle=$	$\\displaystyle r\\cos\\theta,$
	$\\displaystyle y^{\\prime}$	$\\displaystyle=$	$\\displaystyle r\\sin\\theta,$

and through (2) we arrive at the polar equation

r(\\theta)=\\frac{(1-\\epsilon^{2})a}{1-\\epsilon\\cos\\theta}\\cdot

(3)

This equation allows us to determine some additional properties about the ellipse:

	$\\displaystyle r_{max}:=r(0)=(1+\\epsilon)a,\\qquad\\text{which is called the {\\emaphelium%}};$
	$\\displaystyle r_{min}:=r(\\pi)=(1-\\epsilon)a,\\qquad\\text{which is called the {%\\em perihelium}}.$

Hence, the general definition of the ellipse expressed above shows that $r_{min}+r_{max}=2a$ and also that the arithmetic mean $\\displaystyle\\frac{r_{min}+r_{max}}{2}=a$ corresponds to the major semi-axis, while the geometric mean $\\sqrt{r_{min}r_{max}}=b$ corresponds to the minor semi-axis of the ellipse. Likewise, if $\\theta_{\\epsilon}$ is the angle between the polar axis $x^{\\prime}$ and the radial distance $|B-p_{1}|$ , where $B(0,b)$ is the point of the ellipse over the $y$ -axis, then we get the useful equation $\\cos\\theta_{\\epsilon}=\\epsilon$ .

Title	ellipse
Canonical name	Ellipse
Date of creation	2013-03-22 15:18:10
Last modified on	2013-03-22 15:18:10
Owner	matte (1858)
Last modified by	matte (1858)
Numerical id	33
Author	matte (1858)
Entry type	Definition
Classification	msc 53A04
Classification	msc 51N20
Classification	msc 51-00
Related topic	SqueezingMathbbRn
Related topic	Ellipsoid
Defines	major axis
Defines	minor axis
Defines	major semi-axis
Defines	minor semi-axis
Defines	focus
Defines	foci
Defines	aphelium
Defines	perihelium
Defines	eccentric anomaly
Defines	focal radius
Defines	focal radii