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Mathematics · Ch 10 — Conic Sections

Eccentricity

10.5.2

Eccentricity

Eccentricity — The Shape-Defining Ratio

An ellipse is defined by its two fixed foci and the constant sum of distances property. But how stretched is it? That is what eccentricity measures. It is a single number, always between 0 and 1 for an ellipse, that tells you how far the ellipse is from being a circle.

The eccentricity ee is defined as the ratio of two distances measured from the centre of the ellipse:

e=distance from centre to a focusdistance from centre to a vertexe = \frac{\text{distance from centre to a focus}}{\text{distance from centre to a vertex}}

If the distance from the centre to a focus is cc, and the distance from the centre to a vertex is aa, then

e=cae = \frac{c}{a}

Since the focus lies inside the ellipse and the vertex lies on the ellipse, c<ac < a for any non-degenerate ellipse. Therefore 0<e<10 < e < 1. For a circle, the two foci coincide at the centre, so c=0c = 0 and e=0e = 0.

Important

The eccentricity ee is always between 0 and 1 for an ellipse. The closer ee is to 0, the more circular the ellipse; the closer ee is to 1, the more elongated it becomes.

Expressing the Focus Distance in Terms of Eccentricity

From the definition e=c/ae = c/a, we can immediately write the distance from the centre to a focus as

c=aec = a e

This is a very convenient form. Instead of carrying cc through calculations, you can replace it with aeae. The vertices, which are at distance aa from the centre, remain at (±a,0)(\pm a, 0) for the horizontal ellipse. The foci, originally at (±c,0)(\pm c, 0), become (±ae,0)(\pm a e, 0).

Note

The same relation holds for the vertical ellipse: the foci are at (0,±ae)(0, \pm a e) and the vertices at (0,±a)(0, \pm a), where aa is the semi-major axis length.

Relating aa, bb, and ee

You already know the fundamental relationship for an ellipse: c2=a2−b2c^2 = a^2 - b^2, where bb is the semi-minor axis length. Substitute c=aec = a e into this:

(ae)2=a2−b2(a e)^2 = a^2 - b^2

a2e2=a2−b2a^2 e^2 = a^2 - b^2

Rearrange to solve for b2b^2:

b2=a2−a2e2=a2(1−e2)b^2 = a^2 - a^2 e^2 = a^2 (1 - e^2)

This gives a direct link between the semi-minor axis, the semi-major axis, and the eccentricity. It also lets you express bb in terms of aa and ee:

b=a1−e2b = a \sqrt{1 - e^2}

b2=a2(1−e2)b^2 = a^2 (1 - e^2)

The Standard Ellipse Equation in Terms of ee

The standard equation of an ellipse with centre at the origin and major axis along the xx-axis is

x2a2+y2b2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1

Using b2=a2(1−e2)b^2 = a^2 (1 - e^2), you can rewrite this entirely in terms of aa and ee:

x2a2+y2a2(1−e2)=1\frac{x^2}{a^2} + \frac{y^2}{a^2 (1 - e^2)} = 1

This form is particularly useful when you know the eccentricity and the semi-major axis but not the semi-minor axis directly. …

Definition 5Eccentricity

The eccentricity of an ellipse is the fixed ratio e=cae = \frac{c}{a}, where cc is the distance from the centre to a focus, and aa is the distance from the centre to a vertex. Since the focus lies at a distance cc from the centre, this also means the focus is at a distance aeae from the centre.

Intuition: Eccentricity tells you how "stretched" the ellipse is. A circle has e=0e = 0 (foci coincide with the centre); as ee increases toward 11, the ellipse becomes more elongated. …