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CLP-4 Vector Calculus

Section 1.11 Optional — The Astroid

Imagine a ball of radius \(a/4\) rolling around the inside of a circle of radius \(a\text{.}\) The curve traced by a point \(P\) painted on the inner circle (that's the blue curve in the figures below) is called an astroid 1 . We shall find its equation.
Define the angles \(\theta\) and \(\phi\) as in the figure in the left below.
That is
  • the vector from the centre, \(O\text{,}\) of the circle of radius \(a\) to the centre, \(Q\text{,}\) of the ball of radius \(a/4\) is \(\frac{3}{4}a\big(\cos\theta,\sin\theta\big)\) and
  • the vector from the centre, \(Q\text{,}\) of the ball of radius \(a/4\) to the point \(P\) is \(\frac{1}{4}a\big(\cos\phi,-\sin\phi\big)\)
As \(\theta\) runs from 0 to \(\frac{\pi}{2}\text{,}\) the point of contact between the two circles travels through one quarter of the circumference of the circle of radius \(a\text{,}\) which is a distance \(\frac{1}{4}(2\pi a)\text{,}\) which, in turn, is exactly the circumference of the inner circle. Hence if \(\phi=0\) for \(\theta=0\) (i.e. if \(P\) starts on the \(x\)-axis), then for \(\theta=\frac{\pi}{2}\text{,}\) \(P\) is back in contact with the big circle at the north pole of both the inner and outer circles. That is, \(\phi=\frac{3\pi}{2}\) when \(\theta=\frac{\pi}{2}\text{.}\) (See the figure on the right above.) So \(\phi=3\theta\) and \(P\) has coordinates
\begin{equation*} \frac{3}{4}a\big(\cos\theta,\sin\theta\big) +\frac{1}{4}a\big(\cos\phi,-\sin\phi\big) =\frac{a}{4}\big(3\cos\theta+\cos 3\theta,3\sin\theta-\sin 3\theta\big) \end{equation*}
As, recalling your double angle, or even better your triple angle, trig identities,
\begin{align*} \cos3\theta&=\cos\theta\cos2\theta-\sin\theta\sin 2\theta\\ &=\cos\theta[\cos^2\theta-\sin^2\theta]-2\sin^2\theta\cos\theta\\ &=\cos\theta[\cos^2\theta-3\sin^2\theta]\\ \sin3\theta&=\sin\theta\cos2\theta+\cos\theta\sin 2\theta\\ &=\sin\theta[\cos^2\theta-\sin^2\theta]+2\sin\theta\cos^2\theta\\ &=\sin\theta[3\cos^2\theta-\sin^2\theta] \end{align*}
we have
\begin{alignat*}{2} 3\cos\theta+\cos 3\theta &=\cos\theta[3+\cos^2\theta-3\sin^2\theta] & &=\cos\theta[3+\cos^2\theta-3(1-\cos^2\theta)] \\ &=4\cos^3\theta\\ 3\sin\theta-\sin 3\theta &=\sin\theta[3-3\cos^2\theta+\sin^2\theta] & &=\sin\theta[3-3(1-\sin^2\theta)+\sin^2\theta] \\ &=4\sin^3\theta \end{alignat*}
and the coordinates of \(P\) simplify to
\begin{equation*} x(\theta)= a\cos^3\theta\qquad y(\theta)=a\sin^3\theta \end{equation*}
Oof! As \(\ x^{2/3}+y^{2/3}=a^{2/3}\cos^2\theta+a^{2/3}\sin^2\theta \ ,\) the path traced by \(P\) obeys the equation
\begin{equation*} x^{2/3}+y^{2/3} =a^{2/3} \end{equation*}
which is surprisingly simple, considering what we went through to get here.
There remains the danger that there could exist points \((x,y)\) obeying the equation \(x^{2/3}+y^{2/3}=a^{2/3}\) that are not of the form \(x= a\cos^3\theta,\ y=a\sin^3\theta\) for any \(\theta\text{.}\) That is, there is a danger that the parametrized curve \(x= a\cos^3\theta,\ y=a\sin^3\theta\) covers only a portion of \(x^{2/3}+y^{2/3}=a^{2/3}\text{.}\) We now show that the parametrized curve \(x= a\cos^3\theta,\ y=a\sin^3\theta\) in fact covers all of \(x^{2/3}+y^{2/3}=a^{2/3}\) as \(\theta\) runs from \(0\) to \(2\pi\text{.}\)
First, observe that \(x^{2/3}=\big(\root 3\of x\big)^2\ge 0\) and \(y^{2/3}=\big(\root 3\of y\big)^2\ge 0\text{.}\) Hence, if \((x,y)\) obeys \(x^{2/3}+y^{2/3}=a^{2/3}\text{,}\) then necessarily \(0\le x^{2/3}\le a^{2/3} \) and so \(-a\le x\le a\text{.}\) As \(\theta\) runs from \(0\) to \(2\pi\text{,}\) \(a\cos^3\theta\) takes all values between \(-a\) and \(a\) and hence takes all possible values of \(x\text{.}\) For each \(x\in[-a,a]\text{,}\) \(y\) takes two values, namely \(\pm{[a^{2/3}-x^{2/3}]}^{3/2}\text{.}\) If \(x=a\cos^3\theta_0=a\cos^3(2\pi-\theta_0)\text{,}\) the two corresponding values of \(y\) are precisely \(a\sin^3\theta_0\) and \(-a\sin^3\theta_0=a\sin^3(2\pi-\theta_0)\text{.}\)
The name “astroid” comes from the Greek word “aster”, meaning star, with the suffix “oid” meaning “having the shape of”. The curve was first discussed by Johann Bernoulli in 1691–92.