There are three fundamental kinds of elliptic integrals, and these are prosaically but unhelpfully called elliptic integrals of the first kind, the second kind, and the third kind. These names sound odd to modern ears, but it’s no different than classical musicians naming symphonies Symphony No. 1, Symphony No. 2, etc.

This post covers the classical forms of elliptic integrals dating back to Adrien-Marie Legendre (1752–1833) and the next post will cover the modern formulation by Bille Carlson (1924–2013).

## Comparing Legendre and Beethoven

This post will present Legendre’s classification theorem for elliptic integrals, but first let’s look at a few similarities between Legendre and Beethoven.

The image above is a caricature of Legendre, which is unfortunately the only image we have of him. But in this watercolor Legendre looks a little like Beethoven.

Legendre was studying elliptic integrals while Beethoven was writing symphonies—Legendre published his classification of elliptic integrals around a year after Beethoven finished his 9th symphony—and there was a common aesthetic in how they named things

A name like “Symphony No. 5 in C minor” isn’t that descriptive. If we know the difference between Beethoven’s Symphony No. 4 and Symphony No. 5, it’s because we’ve become familiar with each symphony; the names alone aren’t significant. It’s not as if Beethoven’s fourth symphony was written in 4/4 time and his fifth in 5/4 or anything like that.

But we just accept that that’s the way classical composers named things, and we should extend the same understanding to mathematics of the same era. Legendre named his functions analogously to the way Beethoven named his symphonies.

## Elliptic integrals

Before we classify elliptic integrals, we should say what elliptic integrals are. These are functions of the form

where *R* is a rational function and *P* is a polynomial of degree three or four.

## Classification

Legendre’s classification theorem says that any elliptic integral can be written as a linear combination of elementary functions and three special functions: *F*, *E*, and Π. These are the elliptic integrals of the first, second, and third kind, defined below. Said another way, you can evaluate elliiptic integrals if you add just three advanced functions—*F*, *E*, and Π— to the set of functions covered in a calculus class.

The elliptic integral of the second kind comes up in calculating the length of an elliptic arc, and the family of elliptic integrals take their name from this association. I think of *E* as mnemonic for “ellipse” and *F* as mnemonic for “first.” I don’t know whether this was the original motivation for the names. Legendre was French, and I doubt he would call a function *F* for “first” because the French word for “first” is *première*. Maybe an English speaker came up with the notation.

Elliptic integrals of the first kind describe the motion of a pendulum [1]. So you might think of *F* as pendulum functions. It would have been nice if these functions were denoted *P* rather than *F*; French speakers could think *P* stands for “première” and English speakers could think it stand for “pendulum.”

At least in my experience, elliptic integrals of the second kind come up most often, with elliptic integrals of the first kind a distant second, and elliptic integrals of the third kind are rare. I believe my experience is typical; many sources only discuss integrals of the first and second kind and leave out integrals of the third kind.

## Definitions

Here are Legendre’s three basic elliptic integrals.

## Elliptic integrals versus elliptic functions

Elliptic integrals are functions defined by integrals. They’re not the same as elliptic functions, though there’s a connection. It is often said that the inverse of an elliptic integral is an elliptic function. That’s not true without some qualification. What’s true is that the inverse of an elliptic integral *of the first kind* is an elliptic function.

## Related posts

[1] The equation for pendulum motion that is first introduced to students makes the simplifying assumption that the displacement angle θ is so small that sin θ can be replaced with θ. In this case the motion is described by sines and cosines. But if you don’t make this assumption, then the differential equation for motion is nonlinear and its solution is an elliptic integral of the first kind.