The Normal Distribution
The normal distribution — the bell curve — is the most important shape in statistics: symmetric around the mean, thin in the tails, and fully described by just two numbers, mean μ and standard deviation σ.
The 68–95–99.7 rule
| Range | Share of values |
|---|---|
| μ ± 1σ | ~68.3% |
| μ ± 2σ | ~95.4% |
| μ ± 3σ | ~99.7% |
Those three numbers are the fast mental version of the z table: the table simply answers the same question for any boundary, not just whole standard deviations.
Why it appears everywhere
The Central Limit Theorem: when many small independent effects add up — measurement errors, biological variation, averages of samples — their sum tends toward the normal shape regardless of each effect’s own distribution. That is why heights, lab errors and sample means look bell-shaped, and why so much of statistics is built on normal assumptions.
The standard normal
Setting μ = 0 and σ = 1 gives the standard normal distribution — the reference version every other normal converts into via z-scores. One table serves every normal problem because every normal problem can be standardized first.
When it’s the wrong model
Incomes, house prices and waiting times are typically skewed — using normal logic on them misleads. Check the shape before trusting the bell.