Sinusoidal spiral

Family of curves of the form r^n = a^n cos(nθ)
Sinusoidal spirals (rn = –1n cos(), θ = π/2) in polar coordinates and their equivalents in rectangular coordinates:
  n = −2: Equilateral hyperbola
  n = −1: Line
  n = −1/2: Parabola
  n = 1/2: Cardioid
  n = 1: Circle
  n = 2: Lemniscate of Bernoulli

In algebraic geometry, the sinusoidal spirals are a family of curves defined by the equation in polar coordinates

r n = a n cos ( n θ ) {\displaystyle r^{n}=a^{n}\cos(n\theta )\,}

where a is a nonzero constant and n is a rational number other than 0. With a rotation about the origin, this can also be written

r n = a n sin ( n θ ) . {\displaystyle r^{n}=a^{n}\sin(n\theta ).\,}

The term "spiral" is a misnomer, because they are not actually spirals, and often have a flower-like shape. Many well known curves are sinusoidal spirals including:

  • Rectangular hyperbola (n = −2)
  • Line (n = −1)
  • Parabola (n = −1/2)
  • Tschirnhausen cubic (n = −1/3)
  • Cayley's sextet (n = 1/3)
  • Cardioid (n = 1/2)
  • Circle (n = 1)
  • Lemniscate of Bernoulli (n = 2)

The curves were first studied by Colin Maclaurin.

Equations

Differentiating

r n = a n cos ( n θ ) {\displaystyle r^{n}=a^{n}\cos(n\theta )\,}

and eliminating a produces a differential equation for r and θ:

d r d θ cos n θ + r sin n θ = 0. {\displaystyle {\frac {dr}{d\theta }}\cos n\theta +r\sin n\theta =0.}

Then

( d r d s ,   r d θ d s ) cos n θ d s d θ = ( r sin n θ ,   r cos n θ ) = r ( sin n θ ,   cos n θ ) {\displaystyle \left({\frac {dr}{ds}},\ r{\frac {d\theta }{ds}}\right)\cos n\theta {\frac {ds}{d\theta }}=\left(-r\sin n\theta ,\ r\cos n\theta \right)=r\left(-\sin n\theta ,\ \cos n\theta \right)}

which implies that the polar tangential angle is

ψ = n θ ± π / 2 {\displaystyle \psi =n\theta \pm \pi /2}

and so the tangential angle is

φ = ( n + 1 ) θ ± π / 2. {\displaystyle \varphi =(n+1)\theta \pm \pi /2.}

(The sign here is positive if r and cos nθ have the same sign and negative otherwise.)

The unit tangent vector,

( d r d s ,   r d θ d s ) , {\displaystyle \left({\frac {dr}{ds}},\ r{\frac {d\theta }{ds}}\right),}

has length one, so comparing the magnitude of the vectors on each side of the above equation gives

d s d θ = r cos 1 n θ = a cos 1 + 1 n n θ . {\displaystyle {\frac {ds}{d\theta }}=r\cos ^{-1}n\theta =a\cos ^{-1+{\tfrac {1}{n}}}n\theta .}

In particular, the length of a single loop when n > 0 {\displaystyle n>0} is:

a π 2 n π 2 n cos 1 + 1 n n θ   d θ {\displaystyle a\int _{-{\tfrac {\pi }{2n}}}^{\tfrac {\pi }{2n}}\cos ^{-1+{\tfrac {1}{n}}}n\theta \ d\theta }

The curvature is given by

d φ d s = ( n + 1 ) d θ d s = n + 1 a cos 1 1 n n θ . {\displaystyle {\frac {d\varphi }{ds}}=(n+1){\frac {d\theta }{ds}}={\frac {n+1}{a}}\cos ^{1-{\tfrac {1}{n}}}n\theta .}

Properties

The inverse of a sinusoidal spiral with respect to a circle with center at the origin is another sinusoidal spiral whose value of n is the negative of the original curve's value of n. For example, the inverse of the lemniscate of Bernoulli is a rectangular hyperbola.

The isoptic, pedal and negative pedal of a sinusoidal spiral are different sinusoidal spirals.

One path of a particle moving according to a central force proportional to a power of r is a sinusoidal spiral.

When n is an integer, and n points are arranged regularly on a circle of radius a, then the set of points so that the geometric mean of the distances from the point to the n points is a sinusoidal spiral. In this case the sinusoidal spiral is a polynomial lemniscate.

Wikimedia Commons has media related to Sinusoidal spiral.

References

  • Yates, R. C.: A Handbook on Curves and Their Properties, J. W. Edwards (1952), "Spiral" p. 213–214
  • "Sinusoidal spiral" at www.2dcurves.com
  • "Sinusoidal Spirals" at The MacTutor History of Mathematics
  • Weisstein, Eric W. "Sinusoidal Spiral". MathWorld.