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Pure · Sequences & series

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Arithmetic sequences and series

Sequences with a constant common difference — the nth-term rule and the sum formula, and where each comes from.

Pure · Sequences & series

Arithmetic sequences and series

Sequences with a constant common difference — the nth-term rule and the sum formula, and where each comes from.

Why it works

An arithmetic sequence goes up (or down) by the same amount each step — the common difference dd. Starting from the first term aa: a, a+d, a+2d, a+3d, a,\ a + d,\ a + 2d,\ a + 3d,\ \dots By the nnth term you've added dd a total of (n1)(n - 1) times (not nn — the first term has had no steps added), so un=a+(n1)d.u_n = a + (n - 1)d.

The sum of the first nn terms, SnS_n, has a neat shortcut. Write the sum forwards and backwards and add them in pairs: every pair totals a+la + l (first plus last), and there are nn of them, so 2Sn=n(a+l)2S_n = n(a + l). Hence Sn=n2(a+l)=n2[2a+(n1)d],S_n = \frac{n}{2}(a + l) = \frac{n}{2}\big[2a + (n - 1)d\big], using l=a+(n1)dl = a + (n-1)d for the last term. The two forms are the same — use whichever fits what you're given.

The usual mistakes are arithmetic-vs-geometric (here you add dd, you don't multiply) and the "n1n - 1" slip in the nnth term.