Geodesic

A geodesic is a locally length-minimizing curve. Equivalently, it is a path that a particle which is not accelerating would follow. In the plane, the geodesics are straight lines. On the sphere, the geodesics are great circles (like the equator). The geodesics in a space depend on the Riemannian metric, which affects the notions of distance and acceleration.

Geodesics preserve a direction on a surface (Tietze 1965, pp. 26-27) and have many other interesting properties. The normal vector to any point of a geodesic arc lies along the normal to a surface at that point (Weinstock 1974, p. 65).

Furthermore, no matter how badly a sphere is distorted, there exist an infinite number of closed geodesics on it. This general result, demonstrated in the early 1990s, extended earlier work by Birkhoff, who proved in 1917 that there exists at least one closed geodesic on a distorted sphere, and Lyusternik and Schnirelmann, who proved in 1923 that there exist at least three closed geodesics on such a sphere (Cipra 1993, p. 28).

For a surface given parametrically by , , and , the geodesic can be found by minimizing the arc length

But

and similarly for and . Plugging in,

This can be rewritten as

where

and

Starting with equation (◇)

and taking derivatives,

so the Euler-Lagrange differential equation then gives

In the special case when , , and are explicit functions of only,

Now, if and are explicit functions of only and ,

so

In the case where and are explicit functions of only, then

so

and

For a surface of revolution in which is rotated about the x-axis so that the equation of the surface is

the surface can be parameterized by

The equation of the geodesics is then