Ellipse: Difference between revisions

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{{Image|Ellipse1.png|right|350px|Fig. 1. Ellipse. The sum  of the lengths of the two red line segments (ending in P<sub>1</sub>) is equal to the sum of the lengths of the two blue line segments (ending in P<sub>2</sub>). }}
{{Image|Ellipse1.png|right|350px|Fig. 1. Ellipse (black closed curve). The sum  of the lengths of the two red line segments (ending in P<sub>1</sub>) is equal to the sum of the lengths of the two blue line segments (ending in P<sub>2</sub>). }}
In [[mathematics]], an ellipse is a planar [[locus]] of points that have the same sum of distances to two given points. In figure 1 two fixed points F<sub>1</sub> and F<sub>2</sub> are shown, these are ''the foci of the ellipse''. An arbitrary point  P<sub>1</sub> on the ellipse has distance |F<sub>1</sub>P<sub>1</sub>| to F<sub>1</sub> and distance |F<sub>2</sub>P<sub>1</sub>| to F<sub>2</sub>. Let ''d'' be the sum of distances of P<sub>1</sub> to the foci,
In [[mathematics]], an '''ellipse''' is a planar [[locus]] of points characterized by having an equal sum of distances to two given fixed points in the plane. In figure 1 two fixed points F<sub>1</sub> and F<sub>2</sub> are shown, these are ''the foci of the ellipse''. An arbitrary point  P<sub>1</sub> on the ellipse has distance |F<sub>1</sub>P<sub>1</sub>| to F<sub>1</sub> and distance |F<sub>2</sub>P<sub>1</sub>| to F<sub>2</sub>. Let ''d'' be the sum of distances of P<sub>1</sub> to the foci,
:<math>
:<math>
d \equiv |\mathrm{F}_1 \mathrm{P}_1| + |\mathrm{F}_2 \mathrm{P}_1|
d \equiv |\mathrm{F}_1 \mathrm{P}_1| + |\mathrm{F}_2 \mathrm{P}_1|,
</math>
</math>
Another arbitrary point  P<sub>2</sub> on the ellipse has distance |F<sub>1</sub>P<sub>2</sub>| to F<sub>1</sub> and distance |F<sub>2</sub>P<sub>2</sub>| to F<sub>2</sub>. By definition the sum of distances of P<sub>2</sub> to the foci is equal ''d'',
then all points of the ellipse have the sum of distances ''d''. Thus,
another arbitrary point  P<sub>2</sub> on the ellipse has distance |F<sub>1</sub>P<sub>2</sub>| to F<sub>1</sub> and distance |F<sub>2</sub>P<sub>2</sub>| to F<sub>2</sub>. By definition the sum of distances of P<sub>2</sub> to the foci is equal to ''d'',
:<math>
:<math>
|\mathrm{F}_1 \mathrm{P}_2| + |\mathrm{F}_2 \mathrm{P}_2| = d. \,
|\mathrm{F}_1 \mathrm{P}_2| + |\mathrm{F}_2 \mathrm{P}_2| = d. \,
</math>
</math>


The horizontal line through the foci is known as the ''major axis'' of the ellipse. Traditionally, the length of the segment of the major axis bounded by its two intersections with the ellipse is indicated by 2''a''. Very often the horizontal segment itself is referred to as major axis, instead of the whole line of which it is part; from here on we will follow that usage. 
The horizontal line segment S<sub>1</sub>&ndash;S<sub>2</sub> in figure 1, going through the foci, is known as the ''major axis'' of the ellipse. Traditionally, the length of the major axis is indicated by 2''a''.  The vertical dashed line segment, drawn halfway the foci perpendicular to the major axis,  is referred to as the ''minor axis'' of the ellipse; its length is usually indicated by 2''b''.  The major and  minor axes are distinguished by ''a'' &ge; ''b''. When ''a'' = ''b'' the ellipse is a [[circle]]&mdash;a special case of an ellipse.  Clearly both axes are  symmetry axes, reflection in either of them transforms the ellipse into itself. Basically, this a consequence of the fact that a reflection conserves (sums of) distances.
The vertical dashed line segment, drawn halfway the foci perpendicular to the major axis,  is referred to as the ''minor axis'' of the ellipse.  Clearly both axes are  symmetry axes, reflection in either two of them transforms the ellipse into itself.  


The right hand intersection of  the major axis and the ellipse is a point designated by S<sub>2</sub>.  Let the point S<sub>1</sub> be the corresponding left hand intersection; both points are connected by reflection in the minor axis.  The distance of focus  F<sub>2</sub> to S<sub>2</sub> is |S<sub>2</sub>F<sub>2</sub>| &equiv; ''p''. By symmetry the distance |S<sub>1</sub>F<sub>1</sub>| is also equal to ''p''. The distance of S<sub>2</sub> to F<sub>1</sub> is equal to 2''a'' &minus; ''p''.  The distance of S<sub>2</sub> to F<sub>2</sub> is equal to ''p''. By the definition of the ellipse the sum is equal to ''d'', hence
Clearly, the two foci and the  points  S<sub>1</sub>  and S<sub>2</sub> are connected by reflection in the minor axis.  Hence the distance |S<sub>2</sub>F<sub>2</sub>| &equiv; ''p'' is by symmetry equal to the distance |S<sub>1</sub>F<sub>1</sub>|. The distance of S<sub>2</sub> to F<sub>1</sub> is equal to 2''a'' &minus; ''p''.  The distance of S<sub>2</sub> to F<sub>2</sub> is equal to ''p''. By the definition of the ellipse the sum is equal to ''d'', hence
:<math>
:<math>
d = 2a-p + p = 2a.
d = 2a-p + p = 2a. \;
</math>  
</math>  
The sum of distances ''d'' is equal to the distance between S<sub>1</sub> and S<sub>2</sub>.
The sum ''d'' of distances from any point on the ellipse to the foci is equal to the length of the major axis.

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Fig. 1. Ellipse (black closed curve). The sum of the lengths of the two red line segments (ending in P1) is equal to the sum of the lengths of the two blue line segments (ending in P2).

In mathematics, an ellipse is a planar locus of points characterized by having an equal sum of distances to two given fixed points in the plane. In figure 1 two fixed points F1 and F2 are shown, these are the foci of the ellipse. An arbitrary point P1 on the ellipse has distance |F1P1| to F1 and distance |F2P1| to F2. Let d be the sum of distances of P1 to the foci,

then all points of the ellipse have the sum of distances d. Thus, another arbitrary point P2 on the ellipse has distance |F1P2| to F1 and distance |F2P2| to F2. By definition the sum of distances of P2 to the foci is equal to d,

The horizontal line segment S1–S2 in figure 1, going through the foci, is known as the major axis of the ellipse. Traditionally, the length of the major axis is indicated by 2a. The vertical dashed line segment, drawn halfway the foci perpendicular to the major axis, is referred to as the minor axis of the ellipse; its length is usually indicated by 2b. The major and minor axes are distinguished by ab. When a = b the ellipse is a circle—a special case of an ellipse. Clearly both axes are symmetry axes, reflection in either of them transforms the ellipse into itself. Basically, this a consequence of the fact that a reflection conserves (sums of) distances.

Clearly, the two foci and the points S1 and S2 are connected by reflection in the minor axis. Hence the distance |S2F2| ≡ p is by symmetry equal to the distance |S1F1|. The distance of S2 to F1 is equal to 2ap. The distance of S2 to F2 is equal to p. By the definition of the ellipse the sum is equal to d, hence

The sum d of distances from any point on the ellipse to the foci is equal to the length of the major axis.