Epispiral Explained

r=a\sec{n\theta}

.There are n sections if n is odd and 2n if n is even.

It is the polar or circle inversion of the rose curve.

In astronomy the epispiral is related to the equations that explain planets' orbits.

Alternative definition

There is another definition of the epispiral that has to do with tangents to circles:[1]

Begin with a circle.

Rotate some single point on the circle around the circle by some angle

\theta

and at the same time by an angle in constant proportion to

\theta

, say

c\theta

for some constant

c

.

The intersections of the tangent lines to the circle at these new points rotated from that single point for every

\theta

would trace out an epispiral.

The polar equation can be derived through simple geometry as follows:

To determine the polar coordinates

(\rho,\phi)

of the intersection of the tangent lines in question for some

\theta

and

-1<c<1

, note that

\phi

is halfway between

\theta

and

c\theta

by congruence of triangles, so it is
(c+1)\theta
2
. Moreover, if the radius of the circle generating the curve is

r

, then since there is a right-angled triangle (it's right-angled as a tangent to a circle meets the radius at a right angle at the point of tangency) with hypotenuse

\rho

and an angle
(1-c)\theta
2
to which the adjacent leg of the triangle is

r

, the radius

\rho

at the intersection point of the relevant tangents is
r\sec((1-c)\theta
2

)

. This gives the polar equation of the curve,
\rho=r\sec((1-c)\phi
c+1

)

for all points

(\rho,\phi)

on it.

See also

References

Notes and References

  1. Web site: construction of the epispiral by tangent lines . 2023-12-02 . Desmos . en.