**Special Curves**

A large number of curves, called *special curves*, have been studied by mathematicians. A curve is the path traced out by a point moving in space. To keep things simple, we assume that the point is confined to two-dimensional Euclidean space so that it generates a plane curve as it moves. This, a curve results from a mapping .

Special curves have played a central role in the development of mathematics. Seventeenth century mathematicians were interested in rectifying curves — that is, calculating their arc-lengths — and also finding the areas surrounded by closed curves. These questions stimulated the evolution of differential and integral calculus.

**Simple Constraints**

Many simple curves can be defined by applying simple constraints. If the generating point remains at a constant distance from a fixed point , a circle emerges. If it is equidistant from two fixed points, it traces a straight line. If the sum of the distances from two points and , called the foci, is constant, we get an ellipse. If the difference between these distances is constant, a hyperbola is generated. If the product of the two distances is constant, the result is a Cassinian oval. If the ratio is constant, the curve is a circle.

**Inversion with respect to a circle**

Given any plane curve , we can generate a range of other curves. Examples are the evolute, the involute and the pedal curves. We consider here the curve that is the *inverse* of a given curve with respect to a fixed point. To form the inverse, we specify a point called the centre of inversion, and the circle of unit radius centered at . To keep things simple, we take to be the origin. For each point on the curve , we define an inverse point by

It is clear that . The points and are on the same ray from , at distances and respectively, such that . If the inversion is applied twice, we recover the original point.

As the point moves along the curve , the inverse points trace out the inverse curve . If we replace the unit circle by a circle of radius , then the inverse point is such that and the curve has the same shape but is scaled by a factor .

In polar coordinates the inversion is especially simple. The inverse of the point with respect to the unit circle is . Thus, if the original curve is expressed in the form , the inverse curve is .

**Simple examples of inverse curves**

A line through the origin has polar equation and the inverse curve has the same equation, thus . An arbitrary line can be written , and its inverse is . This is the equation of a circle passing through the origin. More generally, the inverse of a circle not passing through is another circle.

A conic section with focus at the origin has polar equation , so the inverse curve (wrt ) is given by . This is the limaçon of Pascal. For the conic is a parabola and the inverse is a special case of the limaçon called a cardioid. The three cases, ellipse (), parabola () and hyperbola () are shown in the figure below.

**Inverse of a rectangular hyperbola wrt its centre**

The inverse changes with the point of inversion. We saw that a hyperbola wrt the focus is a limaçon. Now we look at the inverse wrt the centre. The usual equation for a hyperbola in cartesian coordinates is

Taking and inverting with respect to the origin we get, after some juggling,

which represents the lemniscate (*lemniscus* means a knotted ribbon), a figure-of-eight curve studied by Jakob Bernoulli in 1694. Bernoulli’s work on the arc length of the lemsnicate laid the foundation for later work on elliptic integrals and functions.

It is easier to work in polar coordinates. With and , the equation for the hyperbola (with ) is so the inverse may immediately be written . This converts back to the cartesian form given above.

**Inversion and the Riemann sphere**

There is another way to view inversion — in mathematics, there is always another way! We can map the plane onto the 2-sphere in . is given by . The map is a stereographic projection, as shown in the figure below. A line from the north pole links a point on the sphere to each point in the equatorial plane.

Points on the sphere can be specified by co-latitude and longitude . The southern hemisphere () maps to the interior of the unit circle in . The northern hemisphere () maps to the exterior. A point in maps onto the point in the plane with polar coordinates .

Reflection in the equatorial plane maps a point to . We easily show that maps under stereographic projection to . Therefore, , so *reflection in corresponds to inversion in *.

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