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Mathematics · Ch 14 — Ellipse

Parametric Equations and the Eccentric Angle

14.4

Parametric Equations and the Eccentric Angle

Why parametrise the ellipse

The equation x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 describes the ellipse but doesn't hand you individual points on it conveniently — solving for yy given xx involves a square root, and picking points scattered evenly around the curve by trial is clumsy. A parametric form, where both xx and yy are written as functions of a single angle, fixes this and turns out to connect the ellipse to something very familiar: a circle.

The auxiliary circle and the eccentric angle

Draw the circle of radius aa centred at CC, using the major axis AA′AA' as its diameter — this is called the auxiliary circle of the ellipse, with equation x2+y2=a2x^2+y^2=a^2. Since b<ab<a, the ellipse sits entirely inside this circle, touching it only at AA and A′A'.

Now take any point PP on the ellipse. Draw a perpendicular from PP to the major axis and extend it to meet the auxiliary circle at QQ. The angle θ=∠ACQ\theta = \angle ACQ (measured at the centre, from CACA to CQCQ) is called the eccentric angle of PP. As PP travels once around the ellipse, θ\theta sweeps through the full range 00 to 2π2\pi.

Since QQ lies on the circle of radius aa, its coordinates are (acos⁡θ,asin⁡θ)(a\cos\theta, a\sin\theta) — so x=acos⁡θx = a\cos\theta for the point PP too, because PP and QQ share the same foot on the major axis. Substituting x=acos⁡θx=a\cos\theta into the ellipse equation:

a2cos⁡2θa2+y2b2=1  ⇒  y2=b2sin⁡2θ  ⇒  y=±bsin⁡θ.\frac{a^2\cos^2\theta}{a^2} + \frac{y^2}{b^2} = 1 \;\Rightarrow\; y^2 = b^2\sin^2\theta \;\Rightarrow\; y = \pm b\sin\theta.

Taking the branch consistent with QQ's position gives the parametric equations of the ellipse:

x=acos⁡θ,y=bsin⁡θ,θ∈[0,2π).\boxed{x = a\cos\theta,\qquad y = b\sin\theta}, \qquad \theta \in [0, 2\pi).

For brevity, the point (acos⁡θ,bsin⁡θ)(a\cos\theta, b\sin\theta) is often just called "the point θ\theta" and written P(θ)P(\theta). Notice these two equations together are exactly equivalent to the single Cartesian equation — plugging x=acos⁡θx=a\cos\theta, y=bsin⁡θy=b\sin\theta into x2/a2+y2/b2x^2/a^2+y^2/b^2 gives cos⁡2θ+sin⁡2θ=1\cos^2\theta+\sin^2\theta=1 for every θ\theta, automatically.

This parametric form is what makes later results — the equations of the tangent and normal at a point — so clean, because a single parameter θ\theta replaces the pair (x1,y1)(x_1,y_1) subject to the constraint of lying on the ellipse.

Worked Example

Problem. Find the point on the ellipse x249+y29=1\dfrac{x^2}{49}+\dfrac{y^2}{9}=1 whose eccentric angle is θ=120°\theta = 120°. Then, in the other direction, find the eccentric angle of the point (72,332)\left(\dfrac{7}{2}, \dfrac{3\sqrt3}{2}\right) on the same ellipse.

Solution. Here a=7a=7, b=3b=3. …