Geometric Series

The most important series in all of mathematics is the geometric series: an infinite sum whose terms form a geometric sequence, each a fixed ratio r times the last,

\sum_{n=0}^{\infty} a r^{n} = a + ar + ar^2 + ar^3 + \cdots

with first term a \ne 0 and common ratio r. Whether this converges turns entirely on the size of r: if |r| < 1 each term is a fraction of the last and the total settles; if |r| \ge 1 the terms do not shrink and the sum runs away. And when it does converge, the value is a single clean formula.

The centerpiece: closed form, then the limit

We derive everything from scratch. First a formula for the partial sum s_N, then its limit.

Step 1 — Write the partial sum. Add the first N+1 terms (indices 0 through N):

s_N = a + ar + ar^2 + \cdots + ar^{N}.

Step 2 — Multiply the whole thing by r. Every term's power steps up by one:

r\,s_N = ar + ar^2 + ar^3 + \cdots + ar^{N+1}.

Step 3 — Subtract. Line up s_N - r\,s_N: every middle term ar, ar^2, \dots, ar^N appears in both lists and cancels, leaving only the first term of s_N and the last of r s_N:

s_N - r\,s_N = a - ar^{N+1}.

Step 4 — Factor and solve for s_N. The left side is s_N(1 - r); the right is a(1 - r^{N+1}). Provided r \ne 1 we may divide:

s_N = a\,\frac{1 - r^{\,N+1}}{1 - r}.

That is the closed form for the partial sum — exact, with no infinity in sight yet.

Step 5 — Take N \to \infty. The only place N appears is the term r^{N+1}. Its fate depends on |r|:

|r| < 1 \implies r^{\,N+1} \to 0, \qquad |r| \ge 1 \implies r^{\,N+1} \not\to 0.

Step 6 — Read off the sum when |r| < 1. The r^{N+1} term vanishes, and the partial sums converge:

\sum_{n=0}^{\infty} a r^{n} = \lim_{N\to\infty} a\,\frac{1 - r^{\,N+1}}{1 - r} = a\,\frac{1 - 0}{1 - r} = \frac{a}{1 - r}. \qquad \blacksquare

For |r| \ge 1 the term r^{N+1} either blows up (|r| > 1) or refuses to settle (r = -1 oscillates; r = 1 gives s_N = a(N+1) \to \pm\infty) — so the series diverges. The dividing line is exactly |r| = 1.

For the geometric series \sum_{n=0}^{\infty} a r^{n} with a \ne 0:

The surprising identity 0.999\ldots = 1 is simply a geometric series in disguise. Read the repeating 9s as a sum:

0.999\ldots = \frac{9}{10} + \frac{9}{100} + \frac{9}{1000} + \cdots = \sum_{n=0}^{\infty} \frac{9}{10}\left(\frac{1}{10}\right)^{n},

a geometric series with a = \tfrac{9}{10} and r = \tfrac{1}{10} (so |r| < 1). The formula gives

\sum_{n=0}^{\infty} \frac{9}{10}\left(\frac{1}{10}\right)^{n} = \frac{a}{1-r} = \frac{9/10}{1 - 1/10} = \frac{9/10}{9/10} = 1.

Not "approximately" 1, not "infinitely close" — exactly 1. The same machine turns any repeating decimal into a fraction. For 0.\overline{27} = 0.272727\ldots, take a = \tfrac{27}{100}, r = \tfrac{1}{100}:

0.\overline{27} = \frac{27/100}{1 - 1/100} = \frac{27/100}{99/100} = \frac{27}{99} = \frac{3}{11}.

Every repeating decimal is rational precisely because it is a convergent geometric series.

Slide r across the convergence boundary

Here are the partial sums s_N of \sum a r^n with a = 1, plotted as dots. Move the ratio r: for |r| < 1 the dots level off at the dashed line \tfrac{1}{1-r}; for negative r they spiral in to it from both sides; and as |r| approaches and passes 1 the limit line shoots off and the partial sums blow up. The boundary |r| = 1 is where convergence is won or lost.