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Empirical Rule Calculator

68–95–99.7 — and the two things the rounding hides.

How much lies within k standard deviations

Within 2.0000 standard deviations — 70.00000 to 130.00000

95.4500%

4.5500% falls outside — about 1 in 21.97789, split evenly between the two ends.

2.000σ is 95.45%, not 95.0%. The multiplier that really gives 95.0% is 1.959964. The difference matters the moment the rounded figure gets carried into an interval: a 2.000σ interval is 2.04% wider than the 95.0% one it is standing in for, so quoting it as “95.0% confident” understates the coverage you actually bought.
40.0160

Inside

95.4500%

Outside (both ends)

4.5500%

Above the upper end

2.2750%

1 in 43.95579

Range

70.00000 – 130.00000

Every figure above assumes a normal distribution. Here is what survives without it. Chebyshev’s inequality holds for any distribution with a finite variance, and it guarantees only 75.00% inside 2.000σ — against the normal’s 95.45%. Assuming normality is therefore worth 20.45 percentage points here, and it is an assumption, not a fact about your data. One-sided it is starker: Cantelli’s bound permits up to 20.00% above the upper limit where the normal puts 2.2750% — a factor of 8.7912.

What this tool shows

2σ is 95.45%, not 95%. The multiplier that really gives 95% is 1.95996, so a 2σ interval is 2.04% wider than the one it stands in for. And every figure in the rule assumes a normal distribution: without it, the guaranteed floor at 2σ is 75%, and at 1σ there is no guarantee at all.

  • Exact coverage at any k, not just 1, 2 and 3
  • The multiplier that gives a round 95% or 99%
  • One-tail and two-tail probabilities
  • Odds expressed as “1 in n”
  • Chebyshev’s distribution-free floor beside each figure
  • Cantelli’s one-sided bound, which is far weaker still
Exact, not rounded 2σ ≠ 95% Chebyshev floor shown Any k, not just 1–3

Without normality, Chebyshev guarantees 75% at 2σ and nothing at 1σ.

Updated 8 September 2026 · Works in any browser, no installation

For a normal distribution, 68.27% of values fall within one standard deviation of the mean, 95.45% within two and 99.73% within three. Those are the exact figures. The familiar 68–95–99.7 is a rounding of them, and the middle number is the one that has caused trouble.

At a glance

Formula shown
Coverage within ±kσ is Φ(k) − Φ(−k) = 2Φ(k) − 1. At k = 1, 2, 3 that is 68.2689%, 95.4500%, 99.7300%. Inverted: the multiplier for a target coverage C is Φ⁻¹((1 + C)/2) — 1.95996 for 95%, 2.57583 for 99%. Without normality, Chebyshev gives only 1 − 1/k², valid for any distribution with finite variance.
Scenario support
Reading a normal distribution quickly; setting control-chart limits; interpreting IQ, standardised test and lab reference ranges; sanity-checking whether an observation is unusual; deciding whether a σ-based rule is safe on non-normal data.
Educational estimate
Planning support from the values you enter — not professional advice.

Two sigma is 95.45%, and the difference travels

The rule rounds three numbers. Two of the roundings are harmless and one is not.

68.2689% → 68% and 99.7300% → 99.7% cost nothing, because nobody carries those figures anywhere.

95.4500% → 95% is different, because 95% is the number that appears in every confidence interval and every hypothesis test. Learning “two standard deviations is 95%” and then reaching for 2 when a 95% interval is wanted is the natural next step, and it is wrong.

The multiplier for exactly 95% is 1.959964. Using 2 instead makes the interval 2.04% wider than it needs to be. That is not catastrophic, and it is in the conservative direction — but it means a 2σ interval is really a 95.45% interval, and reporting it as “95% confident” understates what was actually computed. Two analysts, one using 2 and one using 1.96, produce different intervals from identical data and both call them 95%.

It goes the other way at 99%. Three sigma is 99.73%, not 99% — the exact 99% multiplier is 2.5758. Someone reaching for 3σ because “99%” is wanted overshoots by 16% in width, which is a much bigger error than the 95% case and in the same conservative direction.

The habit to build is to go the other way round: decide the coverage you want, then look up the multiplier. The tool takes either direction, and the critical value calculator is the dedicated tool for the inverse when you need a t or chi-square multiplier rather than a normal one.

What survives when the data is not normal

Every number in the rule is a fact about the normal distribution, not about standard deviations in general. It is worth knowing exactly how much of it is left without that assumption, because the answer is surprisingly little.

Chebyshev’s inequality is the distribution-free version, and it holds for literally any distribution with a finite variance — skewed, bimodal, discrete, heavy-tailed, anything. It guarantees at least 1 − 1/k² within k standard deviations.

At 2σ that is 75%, against the normal’s 95.45%. The normality assumption is worth 20.45 percentage points, and it is an assumption you are making rather than a property you have checked.

At 1σ Chebyshev guarantees nothing at all. The bound is vacuous below k = 1, and not merely as a technicality: a distribution can place every single value more than one standard deviation from its mean — a fair coin scored 0 or 1 does exactly that, with all its mass at exactly 1σ. So the rule’s most-quoted figure has zero support outside the normal case.

One-sided, the gap is wider still. Cantelli’s inequality permits up to 20% of a distribution above μ + 2σ, where a normal puts 2.275% — a factor of 8.8. Since most decisions that matter are one-sided (is this too high? did it exceed the limit?), this is the bound that usually applies, and it is the weakest one.

The practical upshot is not to abandon the rule — it is an excellent quick check when the data really is roughly symmetric and unimodal. It is to stop treating “within two standard deviations” as though it means something without that condition. On right-skewed data the upper tail is heavier than 2.275% and the rule understates how often you will see large values, which is the direction that costs money.

Where three sigma came from, and what six sigma means

The 3σ convention is not arbitrary, and knowing its origin explains why it is 3 and not 2 or 4.

Outside ±3σ is 0.27%, or about 1 in 370. Walter Shewhart chose those limits for control charts in the 1920s on exactly that basis: sample a process hourly and a false alarm arrives roughly every 370 samples, which is a tolerable rate of chasing nothing. At 2σ it would be 1 in 22 — several false alarms a day, and operators would learn to ignore the chart.

Six sigma is a different and more slippery figure. Outside ±6σ on a normal distribution is about 1 in 500 million — two parts per billion. But the quality methodology called Six Sigma quotes 3.4 defects per million, which is far larger. The difference is a deliberate 1.5σ allowance for long-run drift in the process mean, so “six sigma quality” is really the one-sided tail beyond 4.5σ. Both numbers are correct about different things, and comparing them directly is a common error.

The far tail is also where the normal assumption is least defensible. A 6σ calculation is an extrapolation far beyond anything a realistic dataset can verify — you would need hundreds of millions of observations to see one. Real processes have heavier tails than the normal, so those figures are best read as a scale for comparison rather than as literal frequencies. Financial risk models made this mistake at scale, describing daily moves as 25σ events that ought to be impossible and had nonetheless just happened twice that week.

Using it on real scores

Most encounters with the rule are through a standardised score, and the arithmetic is the same each time.

IQ is calibrated to a mean of 100 and a standard deviation of 15. So 130 is exactly 2σ, which puts it at the 97.7th percentile — about 1 person in 44, not 1 in 100. 145 is 3σ: 1 in 741. The rule converts a score to a rarity in one step, and the z-score calculator does the conversion for any scale.

Clinical reference ranges are usually the middle 95%, which means one healthy person in twenty falls outside by construction. Run twenty independent tests on a perfectly healthy patient and the chance that all twenty come back inside is 0.95²⁰ = 36% — so an abnormal result on a broad panel is the expected outcome rather than a finding. This is the same multiple-comparisons arithmetic that p-values face.

Grading on a curve applies the rule as policy rather than as a description. Forcing marks into ±1σ and ±2σ bands assumes ability is normally distributed within the class, which for thirty students is an assertion, not an observation.

Check the shape before trusting any of it. The quickest useful test is not a formal one — compare the mean with the median. If they are close and the histogram has one hump, the rule will be about right. If the mean sits well above the median, the data is right-skewed and every tail figure here is optimistic on the high side. The mean, median and mode calculator shows that gap directly, and the lognormal page covers the case where it is large.

One tail or two — the rule only answers one of them

The empirical rule is stated two-sidedly: 95.45% lies within two standard deviations. Most practical questions are one-sided, and using the two-sided figure for them doubles the error.

“How unusual is a value this high?” is a one-tail question. Above ±2σ sits 4.55% of the distribution, but only 2.275% is above +2σ — the rest is below −2σ, which is not what was asked. Quoting 4.55% for a high value overstates its rarity by exactly two.

The multipliers differ too. A two-sided 95% interval uses 1.960; a one-sided 95% bound uses 1.645. That is a 16% difference in width, and picking the wrong one is the same class of error as using 2 instead of 1.96 — only larger.

The direction has to be chosen before seeing the data. A one-sided test is more powerful precisely because it spends all its error budget on one side, and choosing that side after observing which way the result went converts a nominal 5% test into a real 10% one. This is the same arithmetic as the multiple-comparison problem, with two comparisons.

Most quality and safety limits are one-sided. A specification usually cares about too much contamination, too little strength, too long a delay — not deviation in either direction. A control chart with 3σ limits is two-sided by design, but the process capability question behind it is frequently not, which is why the two get quoted with inconsistent tail probabilities.

The tool prints the one-tail figure alongside the two-tail one for exactly this reason, together with the “1 in n” form, which is the phrasing least likely to be halved or doubled by accident.

Sources and methodology

References for the exact figures and the distribution-free bounds.

Method. Coverage is computed as 2Φ(k) − 1 using the higher-precision normal CDF, and the one-tail figure uses the survival function directly rather than 1 − Φ(k), so it stays accurate past k = 8 where the subtraction would lose every significant digit to floating-point cancellation. The exact multiplier for a target coverage comes from the inverse normal, which agrees with the published 1.959964 to fifteen decimal places. The suite asserts the three headline figures to four decimals, that the 2σ interval is 2.0427% wider than the exact 95% one, and that Chebyshev’s bound sits below the normal figure at every k above 1 while being vacuous below it. That engine is verified on every change against 219 assertions. The count and the per-case breakdown are published on the formula verification page.

Related calculators

Where this goes next:

Z-ScoreA z-score from your data or from a known mean and SD — with the normal-table percentile checked against the share of your data that actually falls below it, and a warning when they disagree.
Normal DistributionProbabilities under a normal curve in all four directions with the region shaded — and the empirical rule given exactly, because two standard deviations is 95.45% and the 95% everyone quotes sits at 1.96σ.
Standard DeviationSample and population standard deviation, plus variance, mean, median, quartiles, z-scores, outliers, and confidence intervals.
Critical ValueCritical values for z, t, chi-square and F at any alpha and any degrees of freedom — with one- and two-tailed values shown together, because reading the wrong column of a printed table is the classic error.
Confidence IntervalIntervals for a mean or a proportion using t at every sample size and Wilson rather than the textbook Wald formula — with both methods shown, because Wald returns [0,0] at zero successes.
Mean, Median and ModeAll three centres marked on your own data, every mode rather than just the first, and the mean-median gap read as a direct measure of skew.

More in Math, or browse all calculators.

Educational use disclaimer

An educational tool. Every coverage figure assumes a normal distribution; on skewed or heavy-tailed data the true tail probabilities are larger, and Chebyshev’s much weaker bound is the only guarantee that survives.

How we calculate · Found an error? email us

Authorship & verification

Written and maintained by , a business operator who builds spreadsheet-based calculators.

What's changed (3 updates)

Published 8 September 2026

  1. Published an empirical rule calculator that gives the exact figures rather than the rounded ones: 68.2689%, 95.4500% and 99.7300%. Two sigma is not 95%, and the multiplier that really gives 95% is 1.959964 — so a two-sigma interval is 2.04% wider than the one it is usually taken to be.
  2. Prints Chebyshev's distribution-free floor beside every figure, because the rule is a fact about the normal distribution and not about standard deviations in general. At two sigma the guarantee is 75% against the normal's 95.45%; at one sigma there is no guarantee at all.
  3. Uses the survival function for the one-tail figure rather than one minus the CDF, so the number stays accurate past six sigma where the subtraction would lose every significant digit.

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