An extension of the topic of statistics, the mean and the standard deviation. The sum or average of many independent random factors settles into a "bell" — the normal distribution (the Gaussian curve) — regardless of the distribution of the individual terms. This is the central limit theorem. The normal distribution was described by Carl Friedrich Gauss (1809), and the general theorem was proved by Pierre-Simon Laplace (1810).

I’ll draw an interval ±1σ or ±2σ — increase n with the slider until the fraction of results in that interval hits the 68–95 rule.
What just happened?
A single die roll gives a uniform distribution — six outcomes 1–6 with equal chance 1/6. But when you sum many such independent rolls, the sum distribution stops being flat and ever more closely approximates the characteristic “bell” — the normal distribution (the Gaussian curve). The key point: this happens regardless of what distribution the terms had.
The central limit theorem (CLT)
When some quantity is a sum of many small, independent random factors, its distribution tends to the normal one. The normal distribution has the density:
where is the mean (center of the bell), and is the standard deviation (width of the bell). For the sum of n dice we compute them exactly: and .
The invariant: the 68–95–99.7 rule
For the normal distribution a constant fraction of results falls within successive intervals around the mean — regardless of μ and σ:
The panel on the right shows how the actual fraction of sum results (computed from the exact distribution) converges to these values as n grows. This is a practical tool for interpreting the standard deviation.
A bit of history
The normal distribution was described mathematically by Carl Friedrich Gauss (1809), studying measurement errors in astronomy — hence the “Gaussian curve”. The general central limit theorem was proved by Pierre-Simon Laplace (1810). The CLT is one of the pillars of statistics: it explains why the “bell” appears everywhere in nature and measurements — people’s height, measurement errors, test scores — because each of these quantities is a sum of many small, independent influences.
Why you need this for the exam:
The normal distribution and the 68–95–99.7 rule let you quickly estimate how “typical” a given result is: we measure distance from the mean in units of σ. The trick: when a problem mentions a “sum/average of many trials”, expect a normal distribution — even if a single trial was completely different.
Remember: the sum of many independent random events gives a normal distribution (the Gaussian curve) — regardless of the distribution of the terms. About 68% of results fall within ±1σ, about 95% within ±2σ, around the mean μ.
The density of the bell curve:
The average (or sum) of many independent random factors has, in the limit, a normal distribution — regardless of the distributions of the individual terms.
About of results fall within , — , — .
Notation: mean value, standard deviation, random variable.
A bell shape — the normal distribution (the Gaussian curve), regardless of the distributions of the terms.
About 68% of results fall within ±1 standard deviation of the mean, 95% within ±2σ, 99.7% within ±3σ.
Because many quantities (height, measurement errors) are sums of many small independent random factors.
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