A Taylor series is an infinite sum of polynomial terms that exactly represents a smooth function. Each term is built from the function's value and its derivatives at a chosen center point \(a\):
The idea: if you know everything about a function at one point (its value, slope, curvature, jerk, …), you can reconstruct the function everywhere nearby.
When the center is \(a = 0\), the Taylor series is also called a Maclaurin series — a common special case.
Imagine trying to impersonate a function with a polynomial. First you match the value at point \(a\). Then you match the slope. Then the curvature. Each new term you add forces the polynomial to agree with the original function in one more way at that point.
With infinitely many terms, the polynomial becomes a perfect copy — at least within some radius around \(a\).
Polynomials are the simplest functions computers and humans can evaluate — just multiply and add. If you can convert \(\sin x\), \(e^x\), or \(\ln(1+x)\) into a polynomial, you can compute them to any desired precision. That's exactly what calculators do internally using Taylor series.
Each term in the Taylor series has three parts working together:
| Part | Expression | Role |
| \(f^{(n)}(a)\) | The \(n\)-th derivative of \(f\) evaluated at \(a\) | Encodes the function's behavior at \(a\) |
| \(n!\) | Factorial: \(1 \cdot 2 \cdot 3 \cdots n\) | Cancels the derivative of \((x-a)^n\), keeping coefficients correct |
| \((x-a)^n\) | Power of the distance from center | Higher powers are small near \(a\), large far away |
Radius of Convergence — a Taylor series doesn't always converge for all \(x\). It converges within some interval \(|x - a| < R\), where \(R\) is the radius of convergence. Outside this interval, the series diverges.
These are the most frequently used Taylor series, all centered at \(a = 0\). Memorizing them saves enormous time.
| Function | Series | Converges for |
| \(e^x\) | \(\displaystyle\sum_{n=0}^{\infty} \frac{x^n}{n!} = 1 + x + \frac{x^2}{2!} + \frac{x^3}{3!} + \cdots\) | all \(x\) |
| \(\sin x\) | \(\displaystyle\sum_{n=0}^{\infty} \frac{(-1)^n\,x^{2n+1}}{(2n+1)!} = x - \frac{x^3}{6} + \frac{x^5}{120} - \cdots\) | all \(x\) |
| \(\cos x\) | \(\displaystyle\sum_{n=0}^{\infty} \frac{(-1)^n\,x^{2n}}{(2n)!} = 1 - \frac{x^2}{2} + \frac{x^4}{24} - \cdots\) | all \(x\) |
| \(\ln(1+x)\) | \(\displaystyle\sum_{n=1}^{\infty} \frac{(-1)^{n+1}\,x^n}{n} = x - \frac{x^2}{2} + \frac{x^3}{3} - \cdots\) | \(-1 < x \le 1\) |
| \(\dfrac{1}{1-x}\) | \(\displaystyle\sum_{n=0}^{\infty} x^n = 1 + x + x^2 + x^3 + \cdots\) | \(|x| < 1\) |
| \((1+x)^k\) | \(\displaystyle 1 + kx + \frac{k(k-1)}{2!}x^2 + \frac{k(k-1)(k-2)}{3!}x^3 + \cdots\) | \(|x| < 1\) |
\(f^{(n)}(0) = 1\) for all \(n\)
\(\displaystyle e^x = \sum_{n=0}^{\infty} \frac{x^n}{n!}\)
\(= 1 + x + \dfrac{x^2}{2} + \dfrac{x^3}{6} + \cdots\)
Only odd powers survive:
\(\displaystyle \sin x = \sum_{n=0}^{\infty} \frac{(-1)^n x^{2n+1}}{(2n+1)!}\)
\(= x - \dfrac{x^3}{6} + \dfrac{x^5}{120} - \cdots\)
\(f^{(n)}(1) = \dfrac{(-1)^{n+1}(n-1)!}{1}\) for \(n \ge 1\)
\(\displaystyle \ln x = \sum_{n=1}^{\infty} \frac{(-1)^{n+1}}{n}(x-1)^n\)
\(= 1 + 0.1 + 0.005 + 0.000167\)
\(\approx 1.105167\)
Exact: \(e^{0.1} \approx 1.10517\) ✅
When you stop at the \(n\)-th term, the error is given by Taylor's Remainder Theorem (Lagrange form). This lets you bound how accurate your approximation is.
In practice you bound \(|f^{(n+1)}(c)|\) by its maximum on the interval, giving a worst-case error estimate. This is how you know how many terms you need for a desired precision.
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Taylor series appear in physics, engineering, numerical methods, and everywhere in higher mathematics. Practice with our quizzes.
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