X ~ Binomial(n, p) — the number of successes in n independent trials, each with success probability p. Drag the sliders (or type exact values) to see the distribution change.
The binomial distribution isn't an approximation of anything — it predicts the actual result of flipping n coins. Sample from a process with a known probability of success p (the odds of a coin landing heads, say) over a fixed number of trials n (how many times you flip it), repeat that experiment over and over, and the results land exactly on the binomial distribution. That's not just a classroom exercise, either — it's the same math behind calculating the odds of a match for a bone marrow transplant, or how many left-handed people to expect in a small group. It can be built directly, outcome by outcome, with no approximation involved — which is exactly what the chart above is doing.
About 100 years ago, this was done with printed tables: a book of reference tables could reproduce a great many binomial distributions directly, one page per combination of n and p. But once n grew large, working in raw counts became unwieldy, so the scale was often switched to a proportion instead (X/n rather than X). The trouble was that no tables existed for that proportional distribution, and constructing one by hand — the same term-by-term way the binomial tables had been built — simply wasn't possible at that scale.
The only way forward was to invent a stand-in: a smooth, bell-shaped (Gaussian) curve that could approximate the real distribution without ever being it. Call it a ghost — a curve that looks like the distribution but was never actually built from it. Even that ghost wasn't practical on its own, though: a Gaussian curve has no closed-form antiderivative, so it cannot be integrated over an interval by hand, no matter how much calculus you throw at it. The workaround was to rescale every ghost curve's x-axis into Z-units — standard deviations from the mean, using the real standard deviation of the binomial or proportional distribution behind it. Once every ghost is measured this way, they all collapse into the exact same single, standard normal curve. That one curve was integrated by hand exactly once, producing a master reference — the Z-table — reusable for every ghost, for any n and p, because every Gaussian curve obeys the same fixed rule: 68.27% of its area sits within 1 standard deviation of the mean, 95.45% within 2, and 99.73% within 3 — always.
There's just one thing that whole method requires: the standard deviation of the binomial or proportional distribution being approximated.
Here's what most textbooks never say out loud: you can calculate that standard deviation without ever constructing the binomial or proportional distribution at all. That's possible because variance — the standard deviation squared — is linear: it simply adds up across independent trials, so it can be worked out directly from n and p alone, with no need to build the full distribution first. (You'll see exactly how, later in this tool.)
In a standard textbook, that standard deviation quietly becomes a Z-score, where “1” just means “one standard deviation of the binomial or proportional distribution” — which is also the standard deviation of its ghost — mapped onto the one generic bell curve printed in the book. But because the book never shows you the actual ghost, scaled to your specific n and p, you only ever see one fixed, moderately plump curve, and it's easy to assume every distribution looks like that. In reality, the ghost behind any particular binomial or proportional distribution can be very tall and very skinny (a small standard deviation relative to the mean) or short and wide (a large one) — and that difference is exactly what matters when you go on to compare two populations against each other.
Try it yourself. Press the ▶ Sweep n button next to Trials (n) below and watch its effect on the variance as n climbs from 1 to 1000 — the girth of the binomial (or proportional) distribution visibly changes right along with it. That's because variance is linear. Switch the x-axis to k/n first, then press the button again, and you'll see the paradox: instead of growing, the spread narrows. Later in this tool, we'll show that a higher n doesn't just narrow that spread — it also means more accurate predictions.
Take a sample. Press the orange Take 1 sample button and watch the coins show that sample's number of heads — plotted as a dot on the binomial distribution. Then press ▶ Run automatically: as the coin keeps getting tossed, sample after sample, you'll watch those dots build up into the very same shape the mathematical distribution already predicted.
Watch the ghost appear. Turn on the 🔔 Normal curve overlay, then press ▶ Sweep n. Once n is large enough, that curve stops being just an overlay — it becomes the ghost of the binomial distribution itself, and of the proportional distribution too if you're viewing k/n.
Putting the cart before the horse. Set n to 1000 and p to .001, with the x-axis on k (the binomial count view), then turn on the 🔔 Normal curve overlay — watch it not fit. That's the famous np = 1, below the rule-of-thumb minimum of 5, telling you right there that the normal approximation is a poor one here. Now turn on 🌟 Poisson instead: the magenta dots track the binomial very closely, right where a very high n meets a very low p. Again, that's the genius of the mathematicians who worked this out — a binomial distribution like this one, at n = 1000, couldn't have been built by hand, not even back when I was in high school.
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| -0.0 | 0.5000 | 0.4960 | 0.4920 | 0.4880 | 0.4840 | 0.4801 | 0.4761 | 0.4721 | 0.4681 | 0.4641 |
| -0.1 | 0.4602 | 0.4562 | 0.4522 | 0.4483 | 0.4443 | 0.4404 | 0.4364 | 0.4325 | 0.4286 | 0.4247 |
| -0.2 | 0.4207 | 0.4168 | 0.4129 | 0.4090 | 0.4052 | 0.4013 | 0.3974 | 0.3936 | 0.3897 | 0.3859 |
| -0.3 | 0.3821 | 0.3783 | 0.3745 | 0.3707 | 0.3669 | 0.3632 | 0.3594 | 0.3557 | 0.3520 | 0.3483 |
| -0.4 | 0.3446 | 0.3409 | 0.3372 | 0.3336 | 0.3300 | 0.3264 | 0.3228 | 0.3192 | 0.3156 | 0.3121 |
| -0.5 | 0.3085 | 0.3050 | 0.3015 | 0.2981 | 0.2946 | 0.2912 | 0.2877 | 0.2843 | 0.2810 | 0.2776 |
| -0.6 | 0.2743 | 0.2709 | 0.2676 | 0.2643 | 0.2611 | 0.2578 | 0.2546 | 0.2514 | 0.2483 | 0.2451 |
| -0.7 | 0.2420 | 0.2389 | 0.2358 | 0.2327 | 0.2296 | 0.2266 | 0.2236 | 0.2206 | 0.2177 | 0.2148 |
| -0.8 | 0.2119 | 0.2090 | 0.2061 | 0.2033 | 0.2005 | 0.1977 | 0.1949 | 0.1922 | 0.1894 | 0.1867 |
| -0.9 | 0.1841 | 0.1814 | 0.1788 | 0.1762 | 0.1736 | 0.1711 | 0.1685 | 0.1660 | 0.1635 | 0.1611 |
| -1.0 | 0.1587 | 0.1562 | 0.1539 | 0.1515 | 0.1492 | 0.1469 | 0.1446 | 0.1423 | 0.1401 | 0.1379 |
| -1.1 | 0.1357 | 0.1335 | 0.1314 | 0.1292 | 0.1271 | 0.1251 | 0.1230 | 0.1210 | 0.1190 | 0.1170 |
| -1.2 | 0.1151 | 0.1131 | 0.1112 | 0.1093 | 0.1075 | 0.1056 | 0.1038 | 0.1020 | 0.1003 | 0.0985 |
| -1.3 | 0.0968 | 0.0951 | 0.0934 | 0.0918 | 0.0901 | 0.0885 | 0.0869 | 0.0853 | 0.0838 | 0.0823 |
| -1.4 | 0.0808 | 0.0793 | 0.0778 | 0.0764 | 0.0749 | 0.0735 | 0.0721 | 0.0708 | 0.0694 | 0.0681 |
| -1.5 | 0.0668 | 0.0655 | 0.0643 | 0.0630 | 0.0618 | 0.0606 | 0.0594 | 0.0582 | 0.0571 | 0.0559 |
| -1.6 | 0.0548 | 0.0537 | 0.0526 | 0.0516 | 0.0505 | 0.0495 | 0.0485 | 0.0475 | 0.0465 | 0.0455 |
| -1.7 | 0.0446 | 0.0436 | 0.0427 | 0.0418 | 0.0409 | 0.0401 | 0.0392 | 0.0384 | 0.0375 | 0.0367 |
| -1.8 | 0.0359 | 0.0351 | 0.0344 | 0.0336 | 0.0329 | 0.0322 | 0.0314 | 0.0307 | 0.0301 | 0.0294 |
| -1.9 | 0.0287 | 0.0281 | 0.0274 | 0.0268 | 0.0262 | 0.0256 | 0.0250 | 0.0244 | 0.0239 | 0.0233 |
| -2.0 | 0.0228 | 0.0222 | 0.0217 | 0.0212 | 0.0207 | 0.0202 | 0.0197 | 0.0192 | 0.0188 | 0.0183 |
| -2.1 | 0.0179 | 0.0174 | 0.0170 | 0.0166 | 0.0162 | 0.0158 | 0.0154 | 0.0150 | 0.0146 | 0.0143 |
| -2.2 | 0.0139 | 0.0136 | 0.0132 | 0.0129 | 0.0125 | 0.0122 | 0.0119 | 0.0116 | 0.0113 | 0.0110 |
| -2.3 | 0.0107 | 0.0104 | 0.0102 | 0.0099 | 0.0096 | 0.0094 | 0.0091 | 0.0089 | 0.0087 | 0.0084 |
| -2.4 | 0.0082 | 0.0080 | 0.0078 | 0.0075 | 0.0073 | 0.0071 | 0.0069 | 0.0068 | 0.0066 | 0.0064 |
| -2.5 | 0.0062 | 0.0060 | 0.0059 | 0.0057 | 0.0055 | 0.0054 | 0.0052 | 0.0051 | 0.0049 | 0.0048 |
| -2.6 | 0.0047 | 0.0045 | 0.0044 | 0.0043 | 0.0041 | 0.0040 | 0.0039 | 0.0038 | 0.0037 | 0.0036 |
| -2.7 | 0.0035 | 0.0034 | 0.0033 | 0.0032 | 0.0031 | 0.0030 | 0.0029 | 0.0028 | 0.0027 | 0.0026 |
| -2.8 | 0.0026 | 0.0025 | 0.0024 | 0.0023 | 0.0023 | 0.0022 | 0.0021 | 0.0021 | 0.0020 | 0.0019 |
| -2.9 | 0.0019 | 0.0018 | 0.0018 | 0.0017 | 0.0016 | 0.0016 | 0.0015 | 0.0015 | 0.0014 | 0.0014 |
| -3.0 | 0.0013 | 0.0013 | 0.0013 | 0.0012 | 0.0012 | 0.0011 | 0.0011 | 0.0011 | 0.0010 | 0.0010 |
| -3.1 | 0.0010 | 0.0009 | 0.0009 | 0.0009 | 0.0008 | 0.0008 | 0.0008 | 0.0008 | 0.0007 | 0.0007 |
| -3.2 | 0.0007 | 0.0007 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0005 | 0.0005 | 0.0005 |
| -3.3 | 0.0005 | 0.0005 | 0.0005 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0003 |
| -3.4 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0002 |
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| 0.0 | 0.5000 | 0.5040 | 0.5080 | 0.5120 | 0.5160 | 0.5199 | 0.5239 | 0.5279 | 0.5319 | 0.5359 |
| 0.1 | 0.5398 | 0.5438 | 0.5478 | 0.5517 | 0.5557 | 0.5596 | 0.5636 | 0.5675 | 0.5714 | 0.5753 |
| 0.2 | 0.5793 | 0.5832 | 0.5871 | 0.5910 | 0.5948 | 0.5987 | 0.6026 | 0.6064 | 0.6103 | 0.6141 |
| 0.3 | 0.6179 | 0.6217 | 0.6255 | 0.6293 | 0.6331 | 0.6368 | 0.6406 | 0.6443 | 0.6480 | 0.6517 |
| 0.4 | 0.6554 | 0.6591 | 0.6628 | 0.6664 | 0.6700 | 0.6736 | 0.6772 | 0.6808 | 0.6844 | 0.6879 |
| 0.5 | 0.6915 | 0.6950 | 0.6985 | 0.7019 | 0.7054 | 0.7088 | 0.7123 | 0.7157 | 0.7190 | 0.7224 |
| 0.6 | 0.7257 | 0.7291 | 0.7324 | 0.7357 | 0.7389 | 0.7422 | 0.7454 | 0.7486 | 0.7517 | 0.7549 |
| 0.7 | 0.7580 | 0.7611 | 0.7642 | 0.7673 | 0.7704 | 0.7734 | 0.7764 | 0.7794 | 0.7823 | 0.7852 |
| 0.8 | 0.7881 | 0.7910 | 0.7939 | 0.7967 | 0.7995 | 0.8023 | 0.8051 | 0.8078 | 0.8106 | 0.8133 |
| 0.9 | 0.8159 | 0.8186 | 0.8212 | 0.8238 | 0.8264 | 0.8289 | 0.8315 | 0.8340 | 0.8365 | 0.8389 |
| 1.0 | 0.8413 | 0.8438 | 0.8461 | 0.8485 | 0.8508 | 0.8531 | 0.8554 | 0.8577 | 0.8599 | 0.8621 |
| 1.1 | 0.8643 | 0.8665 | 0.8686 | 0.8708 | 0.8729 | 0.8749 | 0.8770 | 0.8790 | 0.8810 | 0.8830 |
| 1.2 | 0.8849 | 0.8869 | 0.8888 | 0.8907 | 0.8925 | 0.8944 | 0.8962 | 0.8980 | 0.8997 | 0.9015 |
| 1.3 | 0.9032 | 0.9049 | 0.9066 | 0.9082 | 0.9099 | 0.9115 | 0.9131 | 0.9147 | 0.9162 | 0.9177 |
| 1.4 | 0.9192 | 0.9207 | 0.9222 | 0.9236 | 0.9251 | 0.9265 | 0.9279 | 0.9292 | 0.9306 | 0.9319 |
| 1.5 | 0.9332 | 0.9345 | 0.9357 | 0.9370 | 0.9382 | 0.9394 | 0.9406 | 0.9418 | 0.9429 | 0.9441 |
| 1.6 | 0.9452 | 0.9463 | 0.9474 | 0.9484 | 0.9495 | 0.9505 | 0.9515 | 0.9525 | 0.9535 | 0.9545 |
| 1.7 | 0.9554 | 0.9564 | 0.9573 | 0.9582 | 0.9591 | 0.9599 | 0.9608 | 0.9616 | 0.9625 | 0.9633 |
| 1.8 | 0.9641 | 0.9649 | 0.9656 | 0.9664 | 0.9671 | 0.9678 | 0.9686 | 0.9693 | 0.9699 | 0.9706 |
| 1.9 | 0.9713 | 0.9719 | 0.9726 | 0.9732 | 0.9738 | 0.9744 | 0.9750 | 0.9756 | 0.9761 | 0.9767 |
| 2.0 | 0.9772 | 0.9778 | 0.9783 | 0.9788 | 0.9793 | 0.9798 | 0.9803 | 0.9808 | 0.9812 | 0.9817 |
| 2.1 | 0.9821 | 0.9826 | 0.9830 | 0.9834 | 0.9838 | 0.9842 | 0.9846 | 0.9850 | 0.9854 | 0.9857 |
| 2.2 | 0.9861 | 0.9864 | 0.9868 | 0.9871 | 0.9875 | 0.9878 | 0.9881 | 0.9884 | 0.9887 | 0.9890 |
| 2.3 | 0.9893 | 0.9896 | 0.9898 | 0.9901 | 0.9904 | 0.9906 | 0.9909 | 0.9911 | 0.9913 | 0.9916 |
| 2.4 | 0.9918 | 0.9920 | 0.9922 | 0.9925 | 0.9927 | 0.9929 | 0.9931 | 0.9932 | 0.9934 | 0.9936 |
| 2.5 | 0.9938 | 0.9940 | 0.9941 | 0.9943 | 0.9945 | 0.9946 | 0.9948 | 0.9949 | 0.9951 | 0.9952 |
| 2.6 | 0.9953 | 0.9955 | 0.9956 | 0.9957 | 0.9959 | 0.9960 | 0.9961 | 0.9962 | 0.9963 | 0.9964 |
| 2.7 | 0.9965 | 0.9966 | 0.9967 | 0.9968 | 0.9969 | 0.9970 | 0.9971 | 0.9972 | 0.9973 | 0.9974 |
| 2.8 | 0.9974 | 0.9975 | 0.9976 | 0.9977 | 0.9977 | 0.9978 | 0.9979 | 0.9979 | 0.9980 | 0.9981 |
| 2.9 | 0.9981 | 0.9982 | 0.9982 | 0.9983 | 0.9984 | 0.9984 | 0.9985 | 0.9985 | 0.9986 | 0.9986 |
| 3.0 | 0.9987 | 0.9987 | 0.9987 | 0.9988 | 0.9988 | 0.9989 | 0.9989 | 0.9989 | 0.9990 | 0.9990 |
| 3.1 | 0.9990 | 0.9991 | 0.9991 | 0.9991 | 0.9992 | 0.9992 | 0.9992 | 0.9992 | 0.9993 | 0.9993 |
| 3.2 | 0.9993 | 0.9993 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9995 | 0.9995 | 0.9995 |
| 3.3 | 0.9995 | 0.9995 | 0.9995 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9997 |
| 3.4 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9998 |
Two independent binomial populations, A and B. Repeatedly sample one outcome from each, then take the difference in their sample proportions p̂A − p̂B — and watch its own sampling distribution build up below.
X ~ Binomial(n, p) — the number of successes in n independent trials, each with success probability p. Drag the sliders (or type exact values) to see the distribution change.
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| -0.0 | 0.5000 | 0.4960 | 0.4920 | 0.4880 | 0.4840 | 0.4801 | 0.4761 | 0.4721 | 0.4681 | 0.4641 |
| -0.1 | 0.4602 | 0.4562 | 0.4522 | 0.4483 | 0.4443 | 0.4404 | 0.4364 | 0.4325 | 0.4286 | 0.4247 |
| -0.2 | 0.4207 | 0.4168 | 0.4129 | 0.4090 | 0.4052 | 0.4013 | 0.3974 | 0.3936 | 0.3897 | 0.3859 |
| -0.3 | 0.3821 | 0.3783 | 0.3745 | 0.3707 | 0.3669 | 0.3632 | 0.3594 | 0.3557 | 0.3520 | 0.3483 |
| -0.4 | 0.3446 | 0.3409 | 0.3372 | 0.3336 | 0.3300 | 0.3264 | 0.3228 | 0.3192 | 0.3156 | 0.3121 |
| -0.5 | 0.3085 | 0.3050 | 0.3015 | 0.2981 | 0.2946 | 0.2912 | 0.2877 | 0.2843 | 0.2810 | 0.2776 |
| -0.6 | 0.2743 | 0.2709 | 0.2676 | 0.2643 | 0.2611 | 0.2578 | 0.2546 | 0.2514 | 0.2483 | 0.2451 |
| -0.7 | 0.2420 | 0.2389 | 0.2358 | 0.2327 | 0.2296 | 0.2266 | 0.2236 | 0.2206 | 0.2177 | 0.2148 |
| -0.8 | 0.2119 | 0.2090 | 0.2061 | 0.2033 | 0.2005 | 0.1977 | 0.1949 | 0.1922 | 0.1894 | 0.1867 |
| -0.9 | 0.1841 | 0.1814 | 0.1788 | 0.1762 | 0.1736 | 0.1711 | 0.1685 | 0.1660 | 0.1635 | 0.1611 |
| -1.0 | 0.1587 | 0.1562 | 0.1539 | 0.1515 | 0.1492 | 0.1469 | 0.1446 | 0.1423 | 0.1401 | 0.1379 |
| -1.1 | 0.1357 | 0.1335 | 0.1314 | 0.1292 | 0.1271 | 0.1251 | 0.1230 | 0.1210 | 0.1190 | 0.1170 |
| -1.2 | 0.1151 | 0.1131 | 0.1112 | 0.1093 | 0.1075 | 0.1056 | 0.1038 | 0.1020 | 0.1003 | 0.0985 |
| -1.3 | 0.0968 | 0.0951 | 0.0934 | 0.0918 | 0.0901 | 0.0885 | 0.0869 | 0.0853 | 0.0838 | 0.0823 |
| -1.4 | 0.0808 | 0.0793 | 0.0778 | 0.0764 | 0.0749 | 0.0735 | 0.0721 | 0.0708 | 0.0694 | 0.0681 |
| -1.5 | 0.0668 | 0.0655 | 0.0643 | 0.0630 | 0.0618 | 0.0606 | 0.0594 | 0.0582 | 0.0571 | 0.0559 |
| -1.6 | 0.0548 | 0.0537 | 0.0526 | 0.0516 | 0.0505 | 0.0495 | 0.0485 | 0.0475 | 0.0465 | 0.0455 |
| -1.7 | 0.0446 | 0.0436 | 0.0427 | 0.0418 | 0.0409 | 0.0401 | 0.0392 | 0.0384 | 0.0375 | 0.0367 |
| -1.8 | 0.0359 | 0.0351 | 0.0344 | 0.0336 | 0.0329 | 0.0322 | 0.0314 | 0.0307 | 0.0301 | 0.0294 |
| -1.9 | 0.0287 | 0.0281 | 0.0274 | 0.0268 | 0.0262 | 0.0256 | 0.0250 | 0.0244 | 0.0239 | 0.0233 |
| -2.0 | 0.0228 | 0.0222 | 0.0217 | 0.0212 | 0.0207 | 0.0202 | 0.0197 | 0.0192 | 0.0188 | 0.0183 |
| -2.1 | 0.0179 | 0.0174 | 0.0170 | 0.0166 | 0.0162 | 0.0158 | 0.0154 | 0.0150 | 0.0146 | 0.0143 |
| -2.2 | 0.0139 | 0.0136 | 0.0132 | 0.0129 | 0.0125 | 0.0122 | 0.0119 | 0.0116 | 0.0113 | 0.0110 |
| -2.3 | 0.0107 | 0.0104 | 0.0102 | 0.0099 | 0.0096 | 0.0094 | 0.0091 | 0.0089 | 0.0087 | 0.0084 |
| -2.4 | 0.0082 | 0.0080 | 0.0078 | 0.0075 | 0.0073 | 0.0071 | 0.0069 | 0.0068 | 0.0066 | 0.0064 |
| -2.5 | 0.0062 | 0.0060 | 0.0059 | 0.0057 | 0.0055 | 0.0054 | 0.0052 | 0.0051 | 0.0049 | 0.0048 |
| -2.6 | 0.0047 | 0.0045 | 0.0044 | 0.0043 | 0.0041 | 0.0040 | 0.0039 | 0.0038 | 0.0037 | 0.0036 |
| -2.7 | 0.0035 | 0.0034 | 0.0033 | 0.0032 | 0.0031 | 0.0030 | 0.0029 | 0.0028 | 0.0027 | 0.0026 |
| -2.8 | 0.0026 | 0.0025 | 0.0024 | 0.0023 | 0.0023 | 0.0022 | 0.0021 | 0.0021 | 0.0020 | 0.0019 |
| -2.9 | 0.0019 | 0.0018 | 0.0018 | 0.0017 | 0.0016 | 0.0016 | 0.0015 | 0.0015 | 0.0014 | 0.0014 |
| -3.0 | 0.0013 | 0.0013 | 0.0013 | 0.0012 | 0.0012 | 0.0011 | 0.0011 | 0.0011 | 0.0010 | 0.0010 |
| -3.1 | 0.0010 | 0.0009 | 0.0009 | 0.0009 | 0.0008 | 0.0008 | 0.0008 | 0.0008 | 0.0007 | 0.0007 |
| -3.2 | 0.0007 | 0.0007 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0005 | 0.0005 | 0.0005 |
| -3.3 | 0.0005 | 0.0005 | 0.0005 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0003 |
| -3.4 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0002 |
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| 0.0 | 0.5000 | 0.5040 | 0.5080 | 0.5120 | 0.5160 | 0.5199 | 0.5239 | 0.5279 | 0.5319 | 0.5359 |
| 0.1 | 0.5398 | 0.5438 | 0.5478 | 0.5517 | 0.5557 | 0.5596 | 0.5636 | 0.5675 | 0.5714 | 0.5753 |
| 0.2 | 0.5793 | 0.5832 | 0.5871 | 0.5910 | 0.5948 | 0.5987 | 0.6026 | 0.6064 | 0.6103 | 0.6141 |
| 0.3 | 0.6179 | 0.6217 | 0.6255 | 0.6293 | 0.6331 | 0.6368 | 0.6406 | 0.6443 | 0.6480 | 0.6517 |
| 0.4 | 0.6554 | 0.6591 | 0.6628 | 0.6664 | 0.6700 | 0.6736 | 0.6772 | 0.6808 | 0.6844 | 0.6879 |
| 0.5 | 0.6915 | 0.6950 | 0.6985 | 0.7019 | 0.7054 | 0.7088 | 0.7123 | 0.7157 | 0.7190 | 0.7224 |
| 0.6 | 0.7257 | 0.7291 | 0.7324 | 0.7357 | 0.7389 | 0.7422 | 0.7454 | 0.7486 | 0.7517 | 0.7549 |
| 0.7 | 0.7580 | 0.7611 | 0.7642 | 0.7673 | 0.7704 | 0.7734 | 0.7764 | 0.7794 | 0.7823 | 0.7852 |
| 0.8 | 0.7881 | 0.7910 | 0.7939 | 0.7967 | 0.7995 | 0.8023 | 0.8051 | 0.8078 | 0.8106 | 0.8133 |
| 0.9 | 0.8159 | 0.8186 | 0.8212 | 0.8238 | 0.8264 | 0.8289 | 0.8315 | 0.8340 | 0.8365 | 0.8389 |
| 1.0 | 0.8413 | 0.8438 | 0.8461 | 0.8485 | 0.8508 | 0.8531 | 0.8554 | 0.8577 | 0.8599 | 0.8621 |
| 1.1 | 0.8643 | 0.8665 | 0.8686 | 0.8708 | 0.8729 | 0.8749 | 0.8770 | 0.8790 | 0.8810 | 0.8830 |
| 1.2 | 0.8849 | 0.8869 | 0.8888 | 0.8907 | 0.8925 | 0.8944 | 0.8962 | 0.8980 | 0.8997 | 0.9015 |
| 1.3 | 0.9032 | 0.9049 | 0.9066 | 0.9082 | 0.9099 | 0.9115 | 0.9131 | 0.9147 | 0.9162 | 0.9177 |
| 1.4 | 0.9192 | 0.9207 | 0.9222 | 0.9236 | 0.9251 | 0.9265 | 0.9279 | 0.9292 | 0.9306 | 0.9319 |
| 1.5 | 0.9332 | 0.9345 | 0.9357 | 0.9370 | 0.9382 | 0.9394 | 0.9406 | 0.9418 | 0.9429 | 0.9441 |
| 1.6 | 0.9452 | 0.9463 | 0.9474 | 0.9484 | 0.9495 | 0.9505 | 0.9515 | 0.9525 | 0.9535 | 0.9545 |
| 1.7 | 0.9554 | 0.9564 | 0.9573 | 0.9582 | 0.9591 | 0.9599 | 0.9608 | 0.9616 | 0.9625 | 0.9633 |
| 1.8 | 0.9641 | 0.9649 | 0.9656 | 0.9664 | 0.9671 | 0.9678 | 0.9686 | 0.9693 | 0.9699 | 0.9706 |
| 1.9 | 0.9713 | 0.9719 | 0.9726 | 0.9732 | 0.9738 | 0.9744 | 0.9750 | 0.9756 | 0.9761 | 0.9767 |
| 2.0 | 0.9772 | 0.9778 | 0.9783 | 0.9788 | 0.9793 | 0.9798 | 0.9803 | 0.9808 | 0.9812 | 0.9817 |
| 2.1 | 0.9821 | 0.9826 | 0.9830 | 0.9834 | 0.9838 | 0.9842 | 0.9846 | 0.9850 | 0.9854 | 0.9857 |
| 2.2 | 0.9861 | 0.9864 | 0.9868 | 0.9871 | 0.9875 | 0.9878 | 0.9881 | 0.9884 | 0.9887 | 0.9890 |
| 2.3 | 0.9893 | 0.9896 | 0.9898 | 0.9901 | 0.9904 | 0.9906 | 0.9909 | 0.9911 | 0.9913 | 0.9916 |
| 2.4 | 0.9918 | 0.9920 | 0.9922 | 0.9925 | 0.9927 | 0.9929 | 0.9931 | 0.9932 | 0.9934 | 0.9936 |
| 2.5 | 0.9938 | 0.9940 | 0.9941 | 0.9943 | 0.9945 | 0.9946 | 0.9948 | 0.9949 | 0.9951 | 0.9952 |
| 2.6 | 0.9953 | 0.9955 | 0.9956 | 0.9957 | 0.9959 | 0.9960 | 0.9961 | 0.9962 | 0.9963 | 0.9964 |
| 2.7 | 0.9965 | 0.9966 | 0.9967 | 0.9968 | 0.9969 | 0.9970 | 0.9971 | 0.9972 | 0.9973 | 0.9974 |
| 2.8 | 0.9974 | 0.9975 | 0.9976 | 0.9977 | 0.9977 | 0.9978 | 0.9979 | 0.9979 | 0.9980 | 0.9981 |
| 2.9 | 0.9981 | 0.9982 | 0.9982 | 0.9983 | 0.9984 | 0.9984 | 0.9985 | 0.9985 | 0.9986 | 0.9986 |
| 3.0 | 0.9987 | 0.9987 | 0.9987 | 0.9988 | 0.9988 | 0.9989 | 0.9989 | 0.9989 | 0.9990 | 0.9990 |
| 3.1 | 0.9990 | 0.9991 | 0.9991 | 0.9991 | 0.9992 | 0.9992 | 0.9992 | 0.9992 | 0.9993 | 0.9993 |
| 3.2 | 0.9993 | 0.9993 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9995 | 0.9995 | 0.9995 |
| 3.3 | 0.9995 | 0.9995 | 0.9995 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9997 |
| 3.4 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9998 |
X ~ Binomial(n, p) — the number of successes in n independent trials, each with success probability p. Drag the sliders (or type exact values) to see the distribution change.
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| -0.0 | 0.5000 | 0.4960 | 0.4920 | 0.4880 | 0.4840 | 0.4801 | 0.4761 | 0.4721 | 0.4681 | 0.4641 |
| -0.1 | 0.4602 | 0.4562 | 0.4522 | 0.4483 | 0.4443 | 0.4404 | 0.4364 | 0.4325 | 0.4286 | 0.4247 |
| -0.2 | 0.4207 | 0.4168 | 0.4129 | 0.4090 | 0.4052 | 0.4013 | 0.3974 | 0.3936 | 0.3897 | 0.3859 |
| -0.3 | 0.3821 | 0.3783 | 0.3745 | 0.3707 | 0.3669 | 0.3632 | 0.3594 | 0.3557 | 0.3520 | 0.3483 |
| -0.4 | 0.3446 | 0.3409 | 0.3372 | 0.3336 | 0.3300 | 0.3264 | 0.3228 | 0.3192 | 0.3156 | 0.3121 |
| -0.5 | 0.3085 | 0.3050 | 0.3015 | 0.2981 | 0.2946 | 0.2912 | 0.2877 | 0.2843 | 0.2810 | 0.2776 |
| -0.6 | 0.2743 | 0.2709 | 0.2676 | 0.2643 | 0.2611 | 0.2578 | 0.2546 | 0.2514 | 0.2483 | 0.2451 |
| -0.7 | 0.2420 | 0.2389 | 0.2358 | 0.2327 | 0.2296 | 0.2266 | 0.2236 | 0.2206 | 0.2177 | 0.2148 |
| -0.8 | 0.2119 | 0.2090 | 0.2061 | 0.2033 | 0.2005 | 0.1977 | 0.1949 | 0.1922 | 0.1894 | 0.1867 |
| -0.9 | 0.1841 | 0.1814 | 0.1788 | 0.1762 | 0.1736 | 0.1711 | 0.1685 | 0.1660 | 0.1635 | 0.1611 |
| -1.0 | 0.1587 | 0.1562 | 0.1539 | 0.1515 | 0.1492 | 0.1469 | 0.1446 | 0.1423 | 0.1401 | 0.1379 |
| -1.1 | 0.1357 | 0.1335 | 0.1314 | 0.1292 | 0.1271 | 0.1251 | 0.1230 | 0.1210 | 0.1190 | 0.1170 |
| -1.2 | 0.1151 | 0.1131 | 0.1112 | 0.1093 | 0.1075 | 0.1056 | 0.1038 | 0.1020 | 0.1003 | 0.0985 |
| -1.3 | 0.0968 | 0.0951 | 0.0934 | 0.0918 | 0.0901 | 0.0885 | 0.0869 | 0.0853 | 0.0838 | 0.0823 |
| -1.4 | 0.0808 | 0.0793 | 0.0778 | 0.0764 | 0.0749 | 0.0735 | 0.0721 | 0.0708 | 0.0694 | 0.0681 |
| -1.5 | 0.0668 | 0.0655 | 0.0643 | 0.0630 | 0.0618 | 0.0606 | 0.0594 | 0.0582 | 0.0571 | 0.0559 |
| -1.6 | 0.0548 | 0.0537 | 0.0526 | 0.0516 | 0.0505 | 0.0495 | 0.0485 | 0.0475 | 0.0465 | 0.0455 |
| -1.7 | 0.0446 | 0.0436 | 0.0427 | 0.0418 | 0.0409 | 0.0401 | 0.0392 | 0.0384 | 0.0375 | 0.0367 |
| -1.8 | 0.0359 | 0.0351 | 0.0344 | 0.0336 | 0.0329 | 0.0322 | 0.0314 | 0.0307 | 0.0301 | 0.0294 |
| -1.9 | 0.0287 | 0.0281 | 0.0274 | 0.0268 | 0.0262 | 0.0256 | 0.0250 | 0.0244 | 0.0239 | 0.0233 |
| -2.0 | 0.0228 | 0.0222 | 0.0217 | 0.0212 | 0.0207 | 0.0202 | 0.0197 | 0.0192 | 0.0188 | 0.0183 |
| -2.1 | 0.0179 | 0.0174 | 0.0170 | 0.0166 | 0.0162 | 0.0158 | 0.0154 | 0.0150 | 0.0146 | 0.0143 |
| -2.2 | 0.0139 | 0.0136 | 0.0132 | 0.0129 | 0.0125 | 0.0122 | 0.0119 | 0.0116 | 0.0113 | 0.0110 |
| -2.3 | 0.0107 | 0.0104 | 0.0102 | 0.0099 | 0.0096 | 0.0094 | 0.0091 | 0.0089 | 0.0087 | 0.0084 |
| -2.4 | 0.0082 | 0.0080 | 0.0078 | 0.0075 | 0.0073 | 0.0071 | 0.0069 | 0.0068 | 0.0066 | 0.0064 |
| -2.5 | 0.0062 | 0.0060 | 0.0059 | 0.0057 | 0.0055 | 0.0054 | 0.0052 | 0.0051 | 0.0049 | 0.0048 |
| -2.6 | 0.0047 | 0.0045 | 0.0044 | 0.0043 | 0.0041 | 0.0040 | 0.0039 | 0.0038 | 0.0037 | 0.0036 |
| -2.7 | 0.0035 | 0.0034 | 0.0033 | 0.0032 | 0.0031 | 0.0030 | 0.0029 | 0.0028 | 0.0027 | 0.0026 |
| -2.8 | 0.0026 | 0.0025 | 0.0024 | 0.0023 | 0.0023 | 0.0022 | 0.0021 | 0.0021 | 0.0020 | 0.0019 |
| -2.9 | 0.0019 | 0.0018 | 0.0018 | 0.0017 | 0.0016 | 0.0016 | 0.0015 | 0.0015 | 0.0014 | 0.0014 |
| -3.0 | 0.0013 | 0.0013 | 0.0013 | 0.0012 | 0.0012 | 0.0011 | 0.0011 | 0.0011 | 0.0010 | 0.0010 |
| -3.1 | 0.0010 | 0.0009 | 0.0009 | 0.0009 | 0.0008 | 0.0008 | 0.0008 | 0.0008 | 0.0007 | 0.0007 |
| -3.2 | 0.0007 | 0.0007 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0005 | 0.0005 | 0.0005 |
| -3.3 | 0.0005 | 0.0005 | 0.0005 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0003 |
| -3.4 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0002 |
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| 0.0 | 0.5000 | 0.5040 | 0.5080 | 0.5120 | 0.5160 | 0.5199 | 0.5239 | 0.5279 | 0.5319 | 0.5359 |
| 0.1 | 0.5398 | 0.5438 | 0.5478 | 0.5517 | 0.5557 | 0.5596 | 0.5636 | 0.5675 | 0.5714 | 0.5753 |
| 0.2 | 0.5793 | 0.5832 | 0.5871 | 0.5910 | 0.5948 | 0.5987 | 0.6026 | 0.6064 | 0.6103 | 0.6141 |
| 0.3 | 0.6179 | 0.6217 | 0.6255 | 0.6293 | 0.6331 | 0.6368 | 0.6406 | 0.6443 | 0.6480 | 0.6517 |
| 0.4 | 0.6554 | 0.6591 | 0.6628 | 0.6664 | 0.6700 | 0.6736 | 0.6772 | 0.6808 | 0.6844 | 0.6879 |
| 0.5 | 0.6915 | 0.6950 | 0.6985 | 0.7019 | 0.7054 | 0.7088 | 0.7123 | 0.7157 | 0.7190 | 0.7224 |
| 0.6 | 0.7257 | 0.7291 | 0.7324 | 0.7357 | 0.7389 | 0.7422 | 0.7454 | 0.7486 | 0.7517 | 0.7549 |
| 0.7 | 0.7580 | 0.7611 | 0.7642 | 0.7673 | 0.7704 | 0.7734 | 0.7764 | 0.7794 | 0.7823 | 0.7852 |
| 0.8 | 0.7881 | 0.7910 | 0.7939 | 0.7967 | 0.7995 | 0.8023 | 0.8051 | 0.8078 | 0.8106 | 0.8133 |
| 0.9 | 0.8159 | 0.8186 | 0.8212 | 0.8238 | 0.8264 | 0.8289 | 0.8315 | 0.8340 | 0.8365 | 0.8389 |
| 1.0 | 0.8413 | 0.8438 | 0.8461 | 0.8485 | 0.8508 | 0.8531 | 0.8554 | 0.8577 | 0.8599 | 0.8621 |
| 1.1 | 0.8643 | 0.8665 | 0.8686 | 0.8708 | 0.8729 | 0.8749 | 0.8770 | 0.8790 | 0.8810 | 0.8830 |
| 1.2 | 0.8849 | 0.8869 | 0.8888 | 0.8907 | 0.8925 | 0.8944 | 0.8962 | 0.8980 | 0.8997 | 0.9015 |
| 1.3 | 0.9032 | 0.9049 | 0.9066 | 0.9082 | 0.9099 | 0.9115 | 0.9131 | 0.9147 | 0.9162 | 0.9177 |
| 1.4 | 0.9192 | 0.9207 | 0.9222 | 0.9236 | 0.9251 | 0.9265 | 0.9279 | 0.9292 | 0.9306 | 0.9319 |
| 1.5 | 0.9332 | 0.9345 | 0.9357 | 0.9370 | 0.9382 | 0.9394 | 0.9406 | 0.9418 | 0.9429 | 0.9441 |
| 1.6 | 0.9452 | 0.9463 | 0.9474 | 0.9484 | 0.9495 | 0.9505 | 0.9515 | 0.9525 | 0.9535 | 0.9545 |
| 1.7 | 0.9554 | 0.9564 | 0.9573 | 0.9582 | 0.9591 | 0.9599 | 0.9608 | 0.9616 | 0.9625 | 0.9633 |
| 1.8 | 0.9641 | 0.9649 | 0.9656 | 0.9664 | 0.9671 | 0.9678 | 0.9686 | 0.9693 | 0.9699 | 0.9706 |
| 1.9 | 0.9713 | 0.9719 | 0.9726 | 0.9732 | 0.9738 | 0.9744 | 0.9750 | 0.9756 | 0.9761 | 0.9767 |
| 2.0 | 0.9772 | 0.9778 | 0.9783 | 0.9788 | 0.9793 | 0.9798 | 0.9803 | 0.9808 | 0.9812 | 0.9817 |
| 2.1 | 0.9821 | 0.9826 | 0.9830 | 0.9834 | 0.9838 | 0.9842 | 0.9846 | 0.9850 | 0.9854 | 0.9857 |
| 2.2 | 0.9861 | 0.9864 | 0.9868 | 0.9871 | 0.9875 | 0.9878 | 0.9881 | 0.9884 | 0.9887 | 0.9890 |
| 2.3 | 0.9893 | 0.9896 | 0.9898 | 0.9901 | 0.9904 | 0.9906 | 0.9909 | 0.9911 | 0.9913 | 0.9916 |
| 2.4 | 0.9918 | 0.9920 | 0.9922 | 0.9925 | 0.9927 | 0.9929 | 0.9931 | 0.9932 | 0.9934 | 0.9936 |
| 2.5 | 0.9938 | 0.9940 | 0.9941 | 0.9943 | 0.9945 | 0.9946 | 0.9948 | 0.9949 | 0.9951 | 0.9952 |
| 2.6 | 0.9953 | 0.9955 | 0.9956 | 0.9957 | 0.9959 | 0.9960 | 0.9961 | 0.9962 | 0.9963 | 0.9964 |
| 2.7 | 0.9965 | 0.9966 | 0.9967 | 0.9968 | 0.9969 | 0.9970 | 0.9971 | 0.9972 | 0.9973 | 0.9974 |
| 2.8 | 0.9974 | 0.9975 | 0.9976 | 0.9977 | 0.9977 | 0.9978 | 0.9979 | 0.9979 | 0.9980 | 0.9981 |
| 2.9 | 0.9981 | 0.9982 | 0.9982 | 0.9983 | 0.9984 | 0.9984 | 0.9985 | 0.9985 | 0.9986 | 0.9986 |
| 3.0 | 0.9987 | 0.9987 | 0.9987 | 0.9988 | 0.9988 | 0.9989 | 0.9989 | 0.9989 | 0.9990 | 0.9990 |
| 3.1 | 0.9990 | 0.9991 | 0.9991 | 0.9991 | 0.9992 | 0.9992 | 0.9992 | 0.9992 | 0.9993 | 0.9993 |
| 3.2 | 0.9993 | 0.9993 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9995 | 0.9995 | 0.9995 |
| 3.3 | 0.9995 | 0.9995 | 0.9995 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9997 |
| 3.4 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9998 |
A worked reference on counting license-plate arrangements two ways — position-based permutations and selection-based combinations — plus a related walkthrough of restricted combinations with marbles, and poker hands. This page is a static reference for now; an interactive version is coming next.
Setup: One combined bin of 6 distinct symbols — 3 letters (A, B, C) and 3 numbers (1, 2, 3) — with no restriction on which symbol type goes where. The plate has 3 positions, filled with no repeated symbols, and order matters.
Since there's no letters/numbers split to track here, every one of the 6 symbols competes equally for each of the 3 positions. This single count of 120 equals the sum of all four composition cases below (6 + 54 + 54 + 6 = 120) — same total, one combined way to get there.
Setup: 3 distinct letters and 3 distinct numbers (6 symbols total). Plates fill 3 positions with no repeated symbols, and order matters.
And yes — every single plate counted below really is just a permutation. "3 Letters, 0 Numbers," "2 Letters, 1 Number," and the rest aren't a different kind of object from the 120-plate permutation total above; each one is a permutation with the count of each symbol type fixed in advance (2 letter-slots and 1 number-slot, say, instead of any 3 of the 6 symbols in any order). Another name for that is an ordered arrangement — the same symbols, but with position now mattering. That's the term the "Highlight ordered arrangements" button further down uses: it lights up exactly the entries that have become a genuine ordered arrangement, as opposed to the unordered combinations still sitting one step upstream of them.
Method 1, below, deconstructs that single 120-plate total into subsets by symbol type — all-letters, 1 number, 2 numbers, all-numbers, and so on — by sorting the letters and numbers into two separate buckets first. Taking the letters bucket's own permutations and multiplying by the numbers bucket's own permutations never mixes the two: every letter arrangement pairs with every number arrangement, but a letter never swaps places with a number in that count. The one thing that multiplication alone doesn't yet capture is where the letters block and the numbers block sit among the 3 positions — that's the small "(3 choose k)" factor in front of each case's formula. It comes from the same idea, run in reverse: permute the 3 position-slots as if every slot's occupant were fully distinct (3! ways), then divide back out the redundant swaps among slots that actually hold the same symbol type — 2! for 2 same-type letter-slots swapped with each other, 1! (no-op) for a single number-slot — since those swaps don't change which positions ended up being "letter positions" versus "number positions."
Choose which positions on the plate hold letters, then arrange the chosen letters into those spots, then arrange the chosen numbers into the remaining spots.
where k is the number of letters used, out of 3 total plate positions (3 distinct letters, 3 distinct numbers available). The bracket shows k and its complement 3−k together on the bottom row, and ₙPᵣ = n! / (n − r)! (both n and r written as subscripts around P).
The letters permutation term is shown as a marble, and the numbers permutation term is shown as a die.
A second way to land on the exact same case totals as Method 1, without ever building separate letters/numbers buckets: pick the actual letters and numbers together as one unordered set, then permute that whole set freely.
where C(3, k) picks which k letters (out of 3) go on the plate and C(3, 3−k) picks which numbers fill the rest — order isn't decided yet, so letters and numbers are already mixed into one group at that step, unlike Method 1's separate buckets. The last factor, 3!, then permutes that chosen 3-symbol set across all 3 positions. Because the selection step never imposed an order to begin with, nothing gets double-counted here, so nothing needs to be divided back out afterward.
The same position-based method as above, scaled up to the fuller 4-letter/4-number pool (8 symbols total, instead of the reduced 3+3 set): 4 total plate positions, choosing how many hold letters vs. numbers, then arranging each side into its share of the spots.
where k is the number of letters used, out of 4 total plate positions (4 distinct letters, 4 distinct numbers available). The bracket shows k and its complement 4−k together on the bottom row, and ₙPᵣ = n! / (n − r)! (both n and r written as subscripts around P).
The letters permutation term is shown as a marble, and the numbers permutation term is shown as a die.
Ignoring the letters/numbers split entirely, all 8 symbols compete equally for each of the 4 positions:
That single count of 1,680 is the same total the five composition cases below add up to (24 + 384 + 864 + 384 + 24 = 1,680) — one combined way to reach it, versus splitting it out case by case.
The same second way as above, scaled up to the fuller 4-letter/4-number pool: pick the actual letters and numbers together as one unordered set, then permute that whole set freely.
where C(4, k) picks which k letters (out of 4) go on the plate and C(4, 4−k) picks which numbers fill the rest — order isn't decided yet, so letters and numbers are already mixed into one group at that step. The last factor, 4!, then permutes that chosen 4-symbol set across all 4 positions.
Choose which specific letters and which specific numbers will appear on the plate (as unordered selections), then arrange all 4 chosen symbols across the 4 positions in one step. Single bin: 4 letters (A–D) and 4 numbers (1–4).
where k is the number of letters used, out of 4 total plate positions, and ₙCᵣ = n! / (r! (n − r)!) (both n and r written as subscripts around C).
The letters combination term is shown as a green marble, and the numbers combination term is shown as a purple die — different colors from Method 1, so the two methods' icons are never confused.
Step 1: Separate the Group A and Group B marbles into bins. Starting bin: yellow, blue, green, purple, and pink marbles. Group A (yellow, blue, green) and Group B (purple, pink) are separated into two bins.
To quickly calculate the number of combinations that satisfy the requirement, separate the bin into two — one for Group A marbles and one for Group B marbles — and calculate the ways as 3C2 and 2C1. In the first bin are the yellow, blue, and green marbles, and the number of combinations is:
This combines the steps of putting the two marbles into two chairs you don't see — 3 choices for the 1st chair and 2 choices for the 2nd chair (3×2) — then dividing out the number of permutations for those two chairs, since we pulled them out and their order doesn't matter.
In the second bin are the purple and pink marbles, and the number of combinations for 2 pick 2 is:
When we cross-multiply these two groups:
The full cross-multiplication tree: each of the 3 possible Group A pairs (yellow-blue, green-yellow, blue-green) is matched against each of the 2 Group B marbles (pink, purple), producing 6 total combined groupings — each shown as a circle containing 2 Group A marbles + 1 Group B marble.
Each of these can also be written as a ratio of permutations:
3 Group A Marbles, 2 Group B Marbles.
If we have 52 cards in a deck and want to play poker, we can first calculate the number of hands there are. This is the combinations of five cards taken at a time. How many hands of 5 cards? Combination of 52 pick 5.
If we then want to determine the probability of three-of-a-kind Aces, we want to look at the 2,598,960 combinations in the sample space, and isolate or separate out all of the combinations where there are three Aces. This is the hand we want: three Aces, two of another kind. There is no order.
To determine the number of combinations, we will separate the Aces into one bin and all of the other cards in a second bin. Now if we want to find the number of hands with 3 Aces and 2 other cards:
In the first bin we have the ace of spades, hearts, diamonds, and clubs, and the number of combinations for 4 pick 3 is:
In the second bin we have the remaining 48 cards in the deck (everything except the 4 Aces), and the number of combinations for 48 pick 2 is:
Cross-multiplying the two bins gives the total number of hands with exactly 3 Aces and 2 other cards:
So out of 2,598,960 possible 5-card hands, 4,512 of them are exactly three-of-a-kind Aces (with two additional non-Ace cards).
Starting from the plain arithmetic mean of a small set of numbers, building up the ideas that later reappear as the mean of a binomial distribution (μ = np). This page is a work in progress — more sections are coming.
Setup: a small list of numbers, e.g. five quiz scores: 6, 7, 7, 8, 9 (out of 10). The mean (average) answers the question “if every value were replaced by the same number, what would that number have to be so the total stays the same?”
Sum the values, divide by how many there are: (6 + 7 + 7 + 8 + 9) / 5 = 37 / 5 = 7.4. Note x̄ (“x-bar”) is the usual symbol for a sample mean; μ is used instead for a population mean or, later, the mean of a probability distribution — same idea, different symbol depending on what's being averaged.
Setup: ten employees at a small company, StartUpYes Inc., each earning one of four distinct salaries.
| Employee | Salary (x) | Freq. | Rel. Freq. f(x) |
|---|---|---|---|
| Clerk #1 | $10,000 | 1 | 1/10 |
| Clerk #2 | $10,000 | 1 | 1/10 |
| Clerk #3 | $10,000 | 1 | 1/10 |
| Clerk #4 | $10,000 | 1 | 1/10 |
| Jr. Executive #1 | $25,000 | 1 | 1/10 |
| Jr. Executive #2 | $25,000 | 1 | 1/10 |
| Sr. Executive #1 | $50,000 | 1 | 1/10 |
| Sr. Executive #2 | $50,000 | 1 | 1/10 |
| Sr. Executive #3 | $50,000 | 1 | 1/10 |
| President | $100,000 | 1 | 1/10 |
The ordinary way to find the mean: add up every salary, divide by how many employees there are.
Now rewrite that same division a different way: instead of adding everything up and dividing by 10 once at the very end, divide each individual salary by 10 first — equivalently, multiply each one by 1/10 — and add those up instead. It's the same arithmetic (multiplication distributes over addition), but now every value is carrying its own share of the division along with it.
Each employee contributes exactly 1/10 — one tenth — of their own salary to the mean. That fraction, 1/10, is that value's relative frequency, written f(x): the share of the whole data set one value represents. Once every value is paired with its own f(x) like this, the mean can be written in general as:
μ = x·f(x) + x·f(x) + x·f(x) + x·f(x) + x·f(x) + x·f(x) + x·f(x) + x·f(x) + x·f(x) + x·f(x) — one term per employee, each one that employee's salary times the fraction of the group they represent.
Sometimes the raw, one-row-per-person data isn't available — only a summary showing how many people fall at each value. That's still enough to find the mean, using the exact same μ = ∑ x·f(x) formula.
| Position | Salary (x) | # of Employees | Relative Freq. f(x) |
|---|---|---|---|
| President | $100,000 | 1 | 1/10 |
| Senior Executive | $50,000 | 3 | 3/10 |
| Junior Executive | $25,000 | 2 | 2/10 |
| Office Clerk | $10,000 | 4 | 4/10 |
Going back to the expanded, one-term-per-employee sum from Method 1, group together every term that shares the same salary — the three $50,000 terms, the two $25,000 terms, and the four $10,000 terms each collapse into one group (color-coded here to match the table above):
Each colored group is just repeated addition, which is multiplication: three copies of 50,000(1/10) is 50,000(3/10), and likewise for the rest. That collapses the 10-term sum down to one term per distinct salary, each now carrying its own relative frequency:
Reading each term as a share of the group: 1 president out of 10 employees is 1/10 — 10%, frequency 0.1 — earning $100,000. Three senior executives out of 10 is 3/10, or 30% (frequency 0.3), earning $50,000. Two junior executives out of 10 is 2/10, or 20% (frequency 0.2), earning $25,000. Four clerks out of 10 is 4/10, or 40% (frequency 0.4), earning $10,000.
Same $34,000 mean as Method 1 — grouping first just means fewer, bigger terms instead of one term per person.
Now that you've seen it both ways — one row per person, and grouped by distinct value — here's a frequency table of your own to work through.
Setup: 12 students took a quiz; here's how many students got each score.
Each row's x and count are given (and x matches the bars above). Fill in f(x) — as a fraction like count/n, or as a decimal — then x·f(x) for that row. Calculate grades every box at once, and once they're all correct it totals the x·f(x) column under the line to show the mean. New Numbers swaps in a fresh data set to try again.
| Score (x) | # of students | f(x) | x·f(x) |
|---|---|---|---|
| 70 | 2 of 12 | ||
| 80 | 4 of 12 | ||
| 90 | 4 of 12 | ||
| 100 | 2 of 12 | ||
| Σ x·f(x) = | — | ||
Everything above found the mean of a fixed, already-given list of numbers. Here's that same μ = ∑ x·f(x) idea applied to a full binomial distribution: X ~ Binomial(n, p), the number of successes in n independent trials, each with success probability p. Drag the sliders (or type exact values) below to see the distribution — and its mean — change.
| x | f(x) | x·f(x) |
|---|---|---|
| 0 | ||
| 1 | ||
| 2 | ||
| 3 | ||
| Σ x·f(x) = | — | |
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| -0.0 | 0.5000 | 0.4960 | 0.4920 | 0.4880 | 0.4840 | 0.4801 | 0.4761 | 0.4721 | 0.4681 | 0.4641 |
| -0.1 | 0.4602 | 0.4562 | 0.4522 | 0.4483 | 0.4443 | 0.4404 | 0.4364 | 0.4325 | 0.4286 | 0.4247 |
| -0.2 | 0.4207 | 0.4168 | 0.4129 | 0.4090 | 0.4052 | 0.4013 | 0.3974 | 0.3936 | 0.3897 | 0.3859 |
| -0.3 | 0.3821 | 0.3783 | 0.3745 | 0.3707 | 0.3669 | 0.3632 | 0.3594 | 0.3557 | 0.3520 | 0.3483 |
| -0.4 | 0.3446 | 0.3409 | 0.3372 | 0.3336 | 0.3300 | 0.3264 | 0.3228 | 0.3192 | 0.3156 | 0.3121 |
| -0.5 | 0.3085 | 0.3050 | 0.3015 | 0.2981 | 0.2946 | 0.2912 | 0.2877 | 0.2843 | 0.2810 | 0.2776 |
| -0.6 | 0.2743 | 0.2709 | 0.2676 | 0.2643 | 0.2611 | 0.2578 | 0.2546 | 0.2514 | 0.2483 | 0.2451 |
| -0.7 | 0.2420 | 0.2389 | 0.2358 | 0.2327 | 0.2296 | 0.2266 | 0.2236 | 0.2206 | 0.2177 | 0.2148 |
| -0.8 | 0.2119 | 0.2090 | 0.2061 | 0.2033 | 0.2005 | 0.1977 | 0.1949 | 0.1922 | 0.1894 | 0.1867 |
| -0.9 | 0.1841 | 0.1814 | 0.1788 | 0.1762 | 0.1736 | 0.1711 | 0.1685 | 0.1660 | 0.1635 | 0.1611 |
| -1.0 | 0.1587 | 0.1562 | 0.1539 | 0.1515 | 0.1492 | 0.1469 | 0.1446 | 0.1423 | 0.1401 | 0.1379 |
| -1.1 | 0.1357 | 0.1335 | 0.1314 | 0.1292 | 0.1271 | 0.1251 | 0.1230 | 0.1210 | 0.1190 | 0.1170 |
| -1.2 | 0.1151 | 0.1131 | 0.1112 | 0.1093 | 0.1075 | 0.1056 | 0.1038 | 0.1020 | 0.1003 | 0.0985 |
| -1.3 | 0.0968 | 0.0951 | 0.0934 | 0.0918 | 0.0901 | 0.0885 | 0.0869 | 0.0853 | 0.0838 | 0.0823 |
| -1.4 | 0.0808 | 0.0793 | 0.0778 | 0.0764 | 0.0749 | 0.0735 | 0.0721 | 0.0708 | 0.0694 | 0.0681 |
| -1.5 | 0.0668 | 0.0655 | 0.0643 | 0.0630 | 0.0618 | 0.0606 | 0.0594 | 0.0582 | 0.0571 | 0.0559 |
| -1.6 | 0.0548 | 0.0537 | 0.0526 | 0.0516 | 0.0505 | 0.0495 | 0.0485 | 0.0475 | 0.0465 | 0.0455 |
| -1.7 | 0.0446 | 0.0436 | 0.0427 | 0.0418 | 0.0409 | 0.0401 | 0.0392 | 0.0384 | 0.0375 | 0.0367 |
| -1.8 | 0.0359 | 0.0351 | 0.0344 | 0.0336 | 0.0329 | 0.0322 | 0.0314 | 0.0307 | 0.0301 | 0.0294 |
| -1.9 | 0.0287 | 0.0281 | 0.0274 | 0.0268 | 0.0262 | 0.0256 | 0.0250 | 0.0244 | 0.0239 | 0.0233 |
| -2.0 | 0.0228 | 0.0222 | 0.0217 | 0.0212 | 0.0207 | 0.0202 | 0.0197 | 0.0192 | 0.0188 | 0.0183 |
| -2.1 | 0.0179 | 0.0174 | 0.0170 | 0.0166 | 0.0162 | 0.0158 | 0.0154 | 0.0150 | 0.0146 | 0.0143 |
| -2.2 | 0.0139 | 0.0136 | 0.0132 | 0.0129 | 0.0125 | 0.0122 | 0.0119 | 0.0116 | 0.0113 | 0.0110 |
| -2.3 | 0.0107 | 0.0104 | 0.0102 | 0.0099 | 0.0096 | 0.0094 | 0.0091 | 0.0089 | 0.0087 | 0.0084 |
| -2.4 | 0.0082 | 0.0080 | 0.0078 | 0.0075 | 0.0073 | 0.0071 | 0.0069 | 0.0068 | 0.0066 | 0.0064 |
| -2.5 | 0.0062 | 0.0060 | 0.0059 | 0.0057 | 0.0055 | 0.0054 | 0.0052 | 0.0051 | 0.0049 | 0.0048 |
| -2.6 | 0.0047 | 0.0045 | 0.0044 | 0.0043 | 0.0041 | 0.0040 | 0.0039 | 0.0038 | 0.0037 | 0.0036 |
| -2.7 | 0.0035 | 0.0034 | 0.0033 | 0.0032 | 0.0031 | 0.0030 | 0.0029 | 0.0028 | 0.0027 | 0.0026 |
| -2.8 | 0.0026 | 0.0025 | 0.0024 | 0.0023 | 0.0023 | 0.0022 | 0.0021 | 0.0021 | 0.0020 | 0.0019 |
| -2.9 | 0.0019 | 0.0018 | 0.0018 | 0.0017 | 0.0016 | 0.0016 | 0.0015 | 0.0015 | 0.0014 | 0.0014 |
| -3.0 | 0.0013 | 0.0013 | 0.0013 | 0.0012 | 0.0012 | 0.0011 | 0.0011 | 0.0011 | 0.0010 | 0.0010 |
| -3.1 | 0.0010 | 0.0009 | 0.0009 | 0.0009 | 0.0008 | 0.0008 | 0.0008 | 0.0008 | 0.0007 | 0.0007 |
| -3.2 | 0.0007 | 0.0007 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0005 | 0.0005 | 0.0005 |
| -3.3 | 0.0005 | 0.0005 | 0.0005 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0003 |
| -3.4 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0002 |
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| 0.0 | 0.5000 | 0.5040 | 0.5080 | 0.5120 | 0.5160 | 0.5199 | 0.5239 | 0.5279 | 0.5319 | 0.5359 |
| 0.1 | 0.5398 | 0.5438 | 0.5478 | 0.5517 | 0.5557 | 0.5596 | 0.5636 | 0.5675 | 0.5714 | 0.5753 |
| 0.2 | 0.5793 | 0.5832 | 0.5871 | 0.5910 | 0.5948 | 0.5987 | 0.6026 | 0.6064 | 0.6103 | 0.6141 |
| 0.3 | 0.6179 | 0.6217 | 0.6255 | 0.6293 | 0.6331 | 0.6368 | 0.6406 | 0.6443 | 0.6480 | 0.6517 |
| 0.4 | 0.6554 | 0.6591 | 0.6628 | 0.6664 | 0.6700 | 0.6736 | 0.6772 | 0.6808 | 0.6844 | 0.6879 |
| 0.5 | 0.6915 | 0.6950 | 0.6985 | 0.7019 | 0.7054 | 0.7088 | 0.7123 | 0.7157 | 0.7190 | 0.7224 |
| 0.6 | 0.7257 | 0.7291 | 0.7324 | 0.7357 | 0.7389 | 0.7422 | 0.7454 | 0.7486 | 0.7517 | 0.7549 |
| 0.7 | 0.7580 | 0.7611 | 0.7642 | 0.7673 | 0.7704 | 0.7734 | 0.7764 | 0.7794 | 0.7823 | 0.7852 |
| 0.8 | 0.7881 | 0.7910 | 0.7939 | 0.7967 | 0.7995 | 0.8023 | 0.8051 | 0.8078 | 0.8106 | 0.8133 |
| 0.9 | 0.8159 | 0.8186 | 0.8212 | 0.8238 | 0.8264 | 0.8289 | 0.8315 | 0.8340 | 0.8365 | 0.8389 |
| 1.0 | 0.8413 | 0.8438 | 0.8461 | 0.8485 | 0.8508 | 0.8531 | 0.8554 | 0.8577 | 0.8599 | 0.8621 |
| 1.1 | 0.8643 | 0.8665 | 0.8686 | 0.8708 | 0.8729 | 0.8749 | 0.8770 | 0.8790 | 0.8810 | 0.8830 |
| 1.2 | 0.8849 | 0.8869 | 0.8888 | 0.8907 | 0.8925 | 0.8944 | 0.8962 | 0.8980 | 0.8997 | 0.9015 |
| 1.3 | 0.9032 | 0.9049 | 0.9066 | 0.9082 | 0.9099 | 0.9115 | 0.9131 | 0.9147 | 0.9162 | 0.9177 |
| 1.4 | 0.9192 | 0.9207 | 0.9222 | 0.9236 | 0.9251 | 0.9265 | 0.9279 | 0.9292 | 0.9306 | 0.9319 |
| 1.5 | 0.9332 | 0.9345 | 0.9357 | 0.9370 | 0.9382 | 0.9394 | 0.9406 | 0.9418 | 0.9429 | 0.9441 |
| 1.6 | 0.9452 | 0.9463 | 0.9474 | 0.9484 | 0.9495 | 0.9505 | 0.9515 | 0.9525 | 0.9535 | 0.9545 |
| 1.7 | 0.9554 | 0.9564 | 0.9573 | 0.9582 | 0.9591 | 0.9599 | 0.9608 | 0.9616 | 0.9625 | 0.9633 |
| 1.8 | 0.9641 | 0.9649 | 0.9656 | 0.9664 | 0.9671 | 0.9678 | 0.9686 | 0.9693 | 0.9699 | 0.9706 |
| 1.9 | 0.9713 | 0.9719 | 0.9726 | 0.9732 | 0.9738 | 0.9744 | 0.9750 | 0.9756 | 0.9761 | 0.9767 |
| 2.0 | 0.9772 | 0.9778 | 0.9783 | 0.9788 | 0.9793 | 0.9798 | 0.9803 | 0.9808 | 0.9812 | 0.9817 |
| 2.1 | 0.9821 | 0.9826 | 0.9830 | 0.9834 | 0.9838 | 0.9842 | 0.9846 | 0.9850 | 0.9854 | 0.9857 |
| 2.2 | 0.9861 | 0.9864 | 0.9868 | 0.9871 | 0.9875 | 0.9878 | 0.9881 | 0.9884 | 0.9887 | 0.9890 |
| 2.3 | 0.9893 | 0.9896 | 0.9898 | 0.9901 | 0.9904 | 0.9906 | 0.9909 | 0.9911 | 0.9913 | 0.9916 |
| 2.4 | 0.9918 | 0.9920 | 0.9922 | 0.9925 | 0.9927 | 0.9929 | 0.9931 | 0.9932 | 0.9934 | 0.9936 |
| 2.5 | 0.9938 | 0.9940 | 0.9941 | 0.9943 | 0.9945 | 0.9946 | 0.9948 | 0.9949 | 0.9951 | 0.9952 |
| 2.6 | 0.9953 | 0.9955 | 0.9956 | 0.9957 | 0.9959 | 0.9960 | 0.9961 | 0.9962 | 0.9963 | 0.9964 |
| 2.7 | 0.9965 | 0.9966 | 0.9967 | 0.9968 | 0.9969 | 0.9970 | 0.9971 | 0.9972 | 0.9973 | 0.9974 |
| 2.8 | 0.9974 | 0.9975 | 0.9976 | 0.9977 | 0.9977 | 0.9978 | 0.9979 | 0.9979 | 0.9980 | 0.9981 |
| 2.9 | 0.9981 | 0.9982 | 0.9982 | 0.9983 | 0.9984 | 0.9984 | 0.9985 | 0.9985 | 0.9986 | 0.9986 |
| 3.0 | 0.9987 | 0.9987 | 0.9987 | 0.9988 | 0.9988 | 0.9989 | 0.9989 | 0.9989 | 0.9990 | 0.9990 |
| 3.1 | 0.9990 | 0.9991 | 0.9991 | 0.9991 | 0.9992 | 0.9992 | 0.9992 | 0.9992 | 0.9993 | 0.9993 |
| 3.2 | 0.9993 | 0.9993 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9995 | 0.9995 | 0.9995 |
| 3.3 | 0.9995 | 0.9995 | 0.9995 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9997 |
| 3.4 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9998 |
X ~ Binomial(n, p) — the number of successes in n independent trials, each with success probability p. Drag the sliders (or type exact values) to see the distribution change.
Entries are P(X ≤ k) = ∑j=0k C(n, j) pj(1−p)n−j, laid out the way a statistics textbook's appendix presents them — p running across the columns, k down the rows. This table always shows whatever n and p are set on the chart above — for a small n that's every row from k = 0; for a large n, showing every row would mean paging through hundreds mostly rounding to 0.0000 or 1.0000, so it instead windows down to where the distribution's mass actually falls (mean ± 4 std. dev., the same window the chart's own 🔍 Zoom uses). Every row shown is still the full cumulative sum from k = 0, so the first row displayed already carries everything below it. Click a k below to switch on the cumulative step function on the chart above, up through that k. Textbook tables like this only tabulate p up to 0.50, since larger values are read by symmetry: for p > 0.50, look up 1 − p instead and read k as n − k.
| k \ p | 0.05 | 0.10 | 0.15 | 0.20 | 0.25 | 0.30 | 0.35 | 0.40 | 0.45 | 0.50 | 0.55 | 0.60 | 0.65 | 0.70 | 0.75 | 0.80 | 0.85 | 0.90 | 0.95 | 1.00 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 58 | 1.0000 | 1.0000 | 0.9830 | 0.4197 | 0.0123 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 59 | 1.0000 | 1.0000 | 0.9884 | 0.4770 | 0.0175 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 60 | 1.0000 | 1.0000 | 0.9923 | 0.5345 | 0.0246 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 61 | 1.0000 | 1.0000 | 0.9949 | 0.5910 | 0.0338 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 62 | 1.0000 | 1.0000 | 0.9967 | 0.6455 | 0.0456 | 0.0002 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 63 | 1.0000 | 1.0000 | 0.9979 | 0.6970 | 0.0606 | 0.0003 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 64 | 1.0000 | 1.0000 | 0.9987 | 0.7447 | 0.0790 | 0.0005 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 65 | 1.0000 | 1.0000 | 0.9992 | 0.7879 | 0.1013 | 0.0008 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 66 | 1.0000 | 1.0000 | 0.9995 | 0.8264 | 0.1278 | 0.0012 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 67 | 1.0000 | 1.0000 | 0.9997 | 0.8600 | 0.1586 | 0.0018 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 68 | 1.0000 | 1.0000 | 0.9998 | 0.8888 | 0.1938 | 0.0028 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 69 | 1.0000 | 1.0000 | 0.9999 | 0.9131 | 0.2333 | 0.0042 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 70 | 1.0000 | 1.0000 | 0.9999 | 0.9330 | 0.2767 | 0.0061 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 71 | 1.0000 | 1.0000 | 1.0000 | 0.9492 | 0.3235 | 0.0088 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 72 | 1.0000 | 1.0000 | 1.0000 | 0.9621 | 0.3732 | 0.0125 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 73 | 1.0000 | 1.0000 | 1.0000 | 0.9721 | 0.4250 | 0.0174 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 74 | 1.0000 | 1.0000 | 1.0000 | 0.9798 | 0.4778 | 0.0239 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 75 | 1.0000 | 1.0000 | 1.0000 | 0.9856 | 0.5310 | 0.0322 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 76 | 1.0000 | 1.0000 | 1.0000 | 0.9899 | 0.5834 | 0.0429 | 0.0002 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 77 | 1.0000 | 1.0000 | 1.0000 | 0.9930 | 0.6342 | 0.0561 | 0.0003 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 78 | 1.0000 | 1.0000 | 1.0000 | 0.9953 | 0.6827 | 0.0723 | 0.0005 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 79 | 1.0000 | 1.0000 | 1.0000 | 0.9968 | 0.7281 | 0.0918 | 0.0008 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 80 | 1.0000 | 1.0000 | 1.0000 | 0.9979 | 0.7699 | 0.1149 | 0.0013 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 81 | 1.0000 | 1.0000 | 1.0000 | 0.9986 | 0.8077 | 0.1418 | 0.0019 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 82 | 1.0000 | 1.0000 | 1.0000 | 0.9991 | 0.8414 | 0.1726 | 0.0028 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 83 | 1.0000 | 1.0000 | 1.0000 | 0.9995 | 0.8709 | 0.2072 | 0.0041 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 84 | 1.0000 | 1.0000 | 1.0000 | 0.9997 | 0.8963 | 0.2456 | 0.0059 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 85 | 1.0000 | 1.0000 | 1.0000 | 0.9998 | 0.9178 | 0.2874 | 0.0084 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 86 | 1.0000 | 1.0000 | 1.0000 | 0.9999 | 0.9357 | 0.3321 | 0.0117 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 87 | 1.0000 | 1.0000 | 1.0000 | 0.9999 | 0.9504 | 0.3793 | 0.0161 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 88 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9623 | 0.4283 | 0.0218 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 89 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9717 | 0.4782 | 0.0291 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 90 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9790 | 0.5284 | 0.0384 | 0.0002 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 91 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9847 | 0.5781 | 0.0499 | 0.0003 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 92 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9890 | 0.6264 | 0.0640 | 0.0005 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 93 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9922 | 0.6728 | 0.0810 | 0.0008 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 94 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9945 | 0.7165 | 0.1011 | 0.0012 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 95 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9962 | 0.7572 | 0.1246 | 0.0017 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 96 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9974 | 0.7944 | 0.1517 | 0.0025 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 97 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9983 | 0.8279 | 0.1823 | 0.0037 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 98 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9989 | 0.8577 | 0.2164 | 0.0052 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 99 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9993 | 0.8837 | 0.2539 | 0.0074 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 100 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9995 | 0.9061 | 0.2945 | 0.0102 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 101 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9997 | 0.9251 | 0.3378 | 0.0140 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 102 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9998 | 0.9410 | 0.3832 | 0.0189 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 103 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9999 | 0.9541 | 0.4303 | 0.0252 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 104 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9999 | 0.9648 | 0.4783 | 0.0331 | 0.0002 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 105 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9733 | 0.5265 | 0.0429 | 0.0003 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 106 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9800 | 0.5743 | 0.0550 | 0.0004 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 107 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9852 | 0.6210 | 0.0697 | 0.0006 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 108 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9892 | 0.6659 | 0.0871 | 0.0010 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 109 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9922 | 0.7084 | 0.1075 | 0.0014 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 110 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9945 | 0.7483 | 0.1312 | 0.0021 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 111 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9961 | 0.7850 | 0.1582 | 0.0030 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 112 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9973 | 0.8183 | 0.1886 | 0.0043 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 113 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9982 | 0.8482 | 0.2223 | 0.0061 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 114 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9988 | 0.8746 | 0.2592 | 0.0084 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 115 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9992 | 0.8975 | 0.2990 | 0.0115 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 116 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9995 | 0.9173 | 0.3412 | 0.0155 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 117 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9996 | 0.9340 | 0.3855 | 0.0207 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 118 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9998 | 0.9479 | 0.4314 | 0.0273 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 119 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9999 | 0.9594 | 0.4781 | 0.0356 | 0.0002 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 120 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9999 | 0.9687 | 0.5250 | 0.0458 | 0.0003 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 121 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9999 | 0.9762 | 0.5716 | 0.0582 | 0.0005 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 122 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 0.9821 | 0.6172 | 0.0731 | 0.0007 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
Showing n = 300, the chart's own current n. The highlighted column, p = 0.30, is the closest match to the chart's current success probability (p = 0.300). Rows k = 58 to 122 are shown — where nearly all of n = 300's probability mass falls (mean ± 4 std. dev., the same window the chart's own 🔍 Zoom uses) — every row is still the full cumulative sum from k = 0, so k = 58's own row already includes everything below it. Click a k below to switch on the cumulative step function on the chart, up through that point.
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| -0.0 | 0.5000 | 0.4960 | 0.4920 | 0.4880 | 0.4840 | 0.4801 | 0.4761 | 0.4721 | 0.4681 | 0.4641 |
| -0.1 | 0.4602 | 0.4562 | 0.4522 | 0.4483 | 0.4443 | 0.4404 | 0.4364 | 0.4325 | 0.4286 | 0.4247 |
| -0.2 | 0.4207 | 0.4168 | 0.4129 | 0.4090 | 0.4052 | 0.4013 | 0.3974 | 0.3936 | 0.3897 | 0.3859 |
| -0.3 | 0.3821 | 0.3783 | 0.3745 | 0.3707 | 0.3669 | 0.3632 | 0.3594 | 0.3557 | 0.3520 | 0.3483 |
| -0.4 | 0.3446 | 0.3409 | 0.3372 | 0.3336 | 0.3300 | 0.3264 | 0.3228 | 0.3192 | 0.3156 | 0.3121 |
| -0.5 | 0.3085 | 0.3050 | 0.3015 | 0.2981 | 0.2946 | 0.2912 | 0.2877 | 0.2843 | 0.2810 | 0.2776 |
| -0.6 | 0.2743 | 0.2709 | 0.2676 | 0.2643 | 0.2611 | 0.2578 | 0.2546 | 0.2514 | 0.2483 | 0.2451 |
| -0.7 | 0.2420 | 0.2389 | 0.2358 | 0.2327 | 0.2296 | 0.2266 | 0.2236 | 0.2206 | 0.2177 | 0.2148 |
| -0.8 | 0.2119 | 0.2090 | 0.2061 | 0.2033 | 0.2005 | 0.1977 | 0.1949 | 0.1922 | 0.1894 | 0.1867 |
| -0.9 | 0.1841 | 0.1814 | 0.1788 | 0.1762 | 0.1736 | 0.1711 | 0.1685 | 0.1660 | 0.1635 | 0.1611 |
| -1.0 | 0.1587 | 0.1562 | 0.1539 | 0.1515 | 0.1492 | 0.1469 | 0.1446 | 0.1423 | 0.1401 | 0.1379 |
| -1.1 | 0.1357 | 0.1335 | 0.1314 | 0.1292 | 0.1271 | 0.1251 | 0.1230 | 0.1210 | 0.1190 | 0.1170 |
| -1.2 | 0.1151 | 0.1131 | 0.1112 | 0.1093 | 0.1075 | 0.1056 | 0.1038 | 0.1020 | 0.1003 | 0.0985 |
| -1.3 | 0.0968 | 0.0951 | 0.0934 | 0.0918 | 0.0901 | 0.0885 | 0.0869 | 0.0853 | 0.0838 | 0.0823 |
| -1.4 | 0.0808 | 0.0793 | 0.0778 | 0.0764 | 0.0749 | 0.0735 | 0.0721 | 0.0708 | 0.0694 | 0.0681 |
| -1.5 | 0.0668 | 0.0655 | 0.0643 | 0.0630 | 0.0618 | 0.0606 | 0.0594 | 0.0582 | 0.0571 | 0.0559 |
| -1.6 | 0.0548 | 0.0537 | 0.0526 | 0.0516 | 0.0505 | 0.0495 | 0.0485 | 0.0475 | 0.0465 | 0.0455 |
| -1.7 | 0.0446 | 0.0436 | 0.0427 | 0.0418 | 0.0409 | 0.0401 | 0.0392 | 0.0384 | 0.0375 | 0.0367 |
| -1.8 | 0.0359 | 0.0351 | 0.0344 | 0.0336 | 0.0329 | 0.0322 | 0.0314 | 0.0307 | 0.0301 | 0.0294 |
| -1.9 | 0.0287 | 0.0281 | 0.0274 | 0.0268 | 0.0262 | 0.0256 | 0.0250 | 0.0244 | 0.0239 | 0.0233 |
| -2.0 | 0.0228 | 0.0222 | 0.0217 | 0.0212 | 0.0207 | 0.0202 | 0.0197 | 0.0192 | 0.0188 | 0.0183 |
| -2.1 | 0.0179 | 0.0174 | 0.0170 | 0.0166 | 0.0162 | 0.0158 | 0.0154 | 0.0150 | 0.0146 | 0.0143 |
| -2.2 | 0.0139 | 0.0136 | 0.0132 | 0.0129 | 0.0125 | 0.0122 | 0.0119 | 0.0116 | 0.0113 | 0.0110 |
| -2.3 | 0.0107 | 0.0104 | 0.0102 | 0.0099 | 0.0096 | 0.0094 | 0.0091 | 0.0089 | 0.0087 | 0.0084 |
| -2.4 | 0.0082 | 0.0080 | 0.0078 | 0.0075 | 0.0073 | 0.0071 | 0.0069 | 0.0068 | 0.0066 | 0.0064 |
| -2.5 | 0.0062 | 0.0060 | 0.0059 | 0.0057 | 0.0055 | 0.0054 | 0.0052 | 0.0051 | 0.0049 | 0.0048 |
| -2.6 | 0.0047 | 0.0045 | 0.0044 | 0.0043 | 0.0041 | 0.0040 | 0.0039 | 0.0038 | 0.0037 | 0.0036 |
| -2.7 | 0.0035 | 0.0034 | 0.0033 | 0.0032 | 0.0031 | 0.0030 | 0.0029 | 0.0028 | 0.0027 | 0.0026 |
| -2.8 | 0.0026 | 0.0025 | 0.0024 | 0.0023 | 0.0023 | 0.0022 | 0.0021 | 0.0021 | 0.0020 | 0.0019 |
| -2.9 | 0.0019 | 0.0018 | 0.0018 | 0.0017 | 0.0016 | 0.0016 | 0.0015 | 0.0015 | 0.0014 | 0.0014 |
| -3.0 | 0.0013 | 0.0013 | 0.0013 | 0.0012 | 0.0012 | 0.0011 | 0.0011 | 0.0011 | 0.0010 | 0.0010 |
| -3.1 | 0.0010 | 0.0009 | 0.0009 | 0.0009 | 0.0008 | 0.0008 | 0.0008 | 0.0008 | 0.0007 | 0.0007 |
| -3.2 | 0.0007 | 0.0007 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0005 | 0.0005 | 0.0005 |
| -3.3 | 0.0005 | 0.0005 | 0.0005 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0003 |
| -3.4 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0002 |
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| 0.0 | 0.5000 | 0.5040 | 0.5080 | 0.5120 | 0.5160 | 0.5199 | 0.5239 | 0.5279 | 0.5319 | 0.5359 |
| 0.1 | 0.5398 | 0.5438 | 0.5478 | 0.5517 | 0.5557 | 0.5596 | 0.5636 | 0.5675 | 0.5714 | 0.5753 |
| 0.2 | 0.5793 | 0.5832 | 0.5871 | 0.5910 | 0.5948 | 0.5987 | 0.6026 | 0.6064 | 0.6103 | 0.6141 |
| 0.3 | 0.6179 | 0.6217 | 0.6255 | 0.6293 | 0.6331 | 0.6368 | 0.6406 | 0.6443 | 0.6480 | 0.6517 |
| 0.4 | 0.6554 | 0.6591 | 0.6628 | 0.6664 | 0.6700 | 0.6736 | 0.6772 | 0.6808 | 0.6844 | 0.6879 |
| 0.5 | 0.6915 | 0.6950 | 0.6985 | 0.7019 | 0.7054 | 0.7088 | 0.7123 | 0.7157 | 0.7190 | 0.7224 |
| 0.6 | 0.7257 | 0.7291 | 0.7324 | 0.7357 | 0.7389 | 0.7422 | 0.7454 | 0.7486 | 0.7517 | 0.7549 |
| 0.7 | 0.7580 | 0.7611 | 0.7642 | 0.7673 | 0.7704 | 0.7734 | 0.7764 | 0.7794 | 0.7823 | 0.7852 |
| 0.8 | 0.7881 | 0.7910 | 0.7939 | 0.7967 | 0.7995 | 0.8023 | 0.8051 | 0.8078 | 0.8106 | 0.8133 |
| 0.9 | 0.8159 | 0.8186 | 0.8212 | 0.8238 | 0.8264 | 0.8289 | 0.8315 | 0.8340 | 0.8365 | 0.8389 |
| 1.0 | 0.8413 | 0.8438 | 0.8461 | 0.8485 | 0.8508 | 0.8531 | 0.8554 | 0.8577 | 0.8599 | 0.8621 |
| 1.1 | 0.8643 | 0.8665 | 0.8686 | 0.8708 | 0.8729 | 0.8749 | 0.8770 | 0.8790 | 0.8810 | 0.8830 |
| 1.2 | 0.8849 | 0.8869 | 0.8888 | 0.8907 | 0.8925 | 0.8944 | 0.8962 | 0.8980 | 0.8997 | 0.9015 |
| 1.3 | 0.9032 | 0.9049 | 0.9066 | 0.9082 | 0.9099 | 0.9115 | 0.9131 | 0.9147 | 0.9162 | 0.9177 |
| 1.4 | 0.9192 | 0.9207 | 0.9222 | 0.9236 | 0.9251 | 0.9265 | 0.9279 | 0.9292 | 0.9306 | 0.9319 |
| 1.5 | 0.9332 | 0.9345 | 0.9357 | 0.9370 | 0.9382 | 0.9394 | 0.9406 | 0.9418 | 0.9429 | 0.9441 |
| 1.6 | 0.9452 | 0.9463 | 0.9474 | 0.9484 | 0.9495 | 0.9505 | 0.9515 | 0.9525 | 0.9535 | 0.9545 |
| 1.7 | 0.9554 | 0.9564 | 0.9573 | 0.9582 | 0.9591 | 0.9599 | 0.9608 | 0.9616 | 0.9625 | 0.9633 |
| 1.8 | 0.9641 | 0.9649 | 0.9656 | 0.9664 | 0.9671 | 0.9678 | 0.9686 | 0.9693 | 0.9699 | 0.9706 |
| 1.9 | 0.9713 | 0.9719 | 0.9726 | 0.9732 | 0.9738 | 0.9744 | 0.9750 | 0.9756 | 0.9761 | 0.9767 |
| 2.0 | 0.9772 | 0.9778 | 0.9783 | 0.9788 | 0.9793 | 0.9798 | 0.9803 | 0.9808 | 0.9812 | 0.9817 |
| 2.1 | 0.9821 | 0.9826 | 0.9830 | 0.9834 | 0.9838 | 0.9842 | 0.9846 | 0.9850 | 0.9854 | 0.9857 |
| 2.2 | 0.9861 | 0.9864 | 0.9868 | 0.9871 | 0.9875 | 0.9878 | 0.9881 | 0.9884 | 0.9887 | 0.9890 |
| 2.3 | 0.9893 | 0.9896 | 0.9898 | 0.9901 | 0.9904 | 0.9906 | 0.9909 | 0.9911 | 0.9913 | 0.9916 |
| 2.4 | 0.9918 | 0.9920 | 0.9922 | 0.9925 | 0.9927 | 0.9929 | 0.9931 | 0.9932 | 0.9934 | 0.9936 |
| 2.5 | 0.9938 | 0.9940 | 0.9941 | 0.9943 | 0.9945 | 0.9946 | 0.9948 | 0.9949 | 0.9951 | 0.9952 |
| 2.6 | 0.9953 | 0.9955 | 0.9956 | 0.9957 | 0.9959 | 0.9960 | 0.9961 | 0.9962 | 0.9963 | 0.9964 |
| 2.7 | 0.9965 | 0.9966 | 0.9967 | 0.9968 | 0.9969 | 0.9970 | 0.9971 | 0.9972 | 0.9973 | 0.9974 |
| 2.8 | 0.9974 | 0.9975 | 0.9976 | 0.9977 | 0.9977 | 0.9978 | 0.9979 | 0.9979 | 0.9980 | 0.9981 |
| 2.9 | 0.9981 | 0.9982 | 0.9982 | 0.9983 | 0.9984 | 0.9984 | 0.9985 | 0.9985 | 0.9986 | 0.9986 |
| 3.0 | 0.9987 | 0.9987 | 0.9987 | 0.9988 | 0.9988 | 0.9989 | 0.9989 | 0.9989 | 0.9990 | 0.9990 |
| 3.1 | 0.9990 | 0.9991 | 0.9991 | 0.9991 | 0.9992 | 0.9992 | 0.9992 | 0.9992 | 0.9993 | 0.9993 |
| 3.2 | 0.9993 | 0.9993 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9995 | 0.9995 | 0.9995 |
| 3.3 | 0.9995 | 0.9995 | 0.9995 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9997 |
| 3.4 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9998 |
The Z-score was necessary because, when this math was developed, it wasn't possible to actually construct a large binomial or proportional distribution by hand. There had to be a way to get that distribution's mean and standard deviation without ever building it — because building it just wasn't possible.
On the chart, the binomial (or proportional) bars are grayed out because before computers, no one could actually build one of these distributions by hand for anything but a tiny n — there was never a real set of bars to check against. The dashed curve is the ghost standing in for it: shaped exactly like whatever binomial it approximates, even though that binomial itself is never actually drawn. That ghost then gets mapped onto one single, universal standard normal curve, because no matter how a particular bell is stretched or shifted, its own 1, 2, and 3 standard-deviation marks always enclose the same fixed share of the area — converting to z means reading off that one curve instead of a different curve for every n and p.
That ghost only looks like a bell when n is reasonably large and p isn't too close to 0 or 1 — a small binomial loses its own symmetry, and the Gaussian ghost stops resembling it at all. That's exactly what the "np ="/"nq =" rule of thumb next to the Normal curve button is checking for, both needing to clear 5. Fortunately, for small n the exact binomial probabilities could still be worked out by hand, so they were simply tabulated directly in the back of standard textbooks instead. And when n grows very large while p gets very small, the normal approximation breaks down a different way — too skewed for a symmetric bell to fit — which is exactly the gap the Poisson distribution was built to fill.
Here’s where calculus runs out of tricks: this curve has no elementary antiderivative, so there’s no way to integrate it piece by piece by hand. It still has to integrate to exactly 1 from −∞ to +∞ — that’s what fixes its scaling constant — and actually doing that integral takes a trick (squaring it and switching to polar coordinates) that’s a story for another day. So instead of solving it fresh for every problem, the Z-table was built once, by hand, and reused ever since.
All of this only works because variance has one convenient property — it’s additive, so np(1−p) can be found directly without ever constructing the distribution it describes. Rescale that to a proportion and a small paradox falls out: the variance actually shrinks as n grows. A smaller variance means a tighter distribution, which is exactly what lets a bigger sample tell populations apart more precisely.
How many ways can you pick a group from a larger set, when the order the group ends up in doesn't matter? This page builds combinations up from permutations, the way it's usually easiest to see it the first time: start with chairs (order matters), then take the chairs away (order stops mattering) and see exactly what collapses.
Setup: three marbles — blue, green, and yellow — are waiting in the parlor (this page's nickname for it is "the bin") to be seated, one each, into three chairs. Order matters: blue-green-yellow and green-blue-yellow are different outcomes, because a different marble ends up in chair 1. The count of orderings is written 3P3 ("3 pick 3"), read as "the number of permutations of 3 things taken 3 at a time." The capital P is what marks it as a permutation (order-counts) problem; the first number is how many marbles are waiting, the second is how many chairs they're filling.
Drag a marble out of the bin onto the chairs — it seats itself in the next open one, and the bin updates live to show what’s still waiting. Click a seated marble to unseat it (and anyone seated after) and try a different order.
Multiplying the choices at each step (the same "multiply the branches" idea behind every counting tree on this page) gives the total number of orderings:
If three marbles sit down in three chairs, every ordered seating is a permutation — that's everything above. Now pull the chairs out. Once there's nowhere to seat them in order, there is exactly one way for all three marbles to simply be in the room together: order no longer distinguishes anything, since there's no chair 1, chair 2, chair 3 left to disagree about. Three marbles, three chairs, no chairs left over — there is one and only one combination.
This is written 3C3 — the capital C marks it as a combination (order-doesn't-count) problem, read "3 choose 3," or "the number of combinations of 3 things taken 3 at a time." The circle is used as the icon for combinations throughout this site, since a circle (unlike a row of chairs) has no fixed order to it.
One way to see why: there were 6 permutations above. Every one of those 6 is the same three marbles, just rearranged into a different chair order. If we want combinations, we need to divide out exactly that rearranging — the number of ways to permute the 3 chairs themselves, which is 3! = 3 × 2 × 1 = 6.
Setup: now there are five marbles waiting — blue, green, yellow, purple, and pink — but only 2 chairs to fill. nPk notation: n is the number of marbles waiting, k is the number of chairs, and (n−k) is the number of marbles that never get a seat at all.
Order matters here: a purple marble seated next to a green one is a different outcome from a green seated next to a purple. Written as a fraction of factorials — the same 5 × 4 mechanics, just with the unused 3! = 3 × 2 × 1 (the three marbles that never get a seat) multiplied on and then immediately divided back off:
Combinations: once two marbles are in their two chairs, if we no longer care which one sits where — same idea as pulling the chairs out above — we divide by the number of ways to permute just those 2 filled chairs, which is 2! = 2. That turns every matched pair of permutations (say, blue-then-green and green-then-blue) into the single combination "blue and green."
The k! in that denominator is really just the permutations of the k filled chairs — it's doing exactly the same job 3! did for the all-three-seated case above, just for 2 filled chairs instead of 3.
Same 20 permutations as Figure 4, this time as boxes — a box keeps its order, first marble then second, the way a chair does. Drag each box down into its matching circle below. The first box to arrive settles in; drag its reverse-order partner into the same circle and watch it collapse away, since it is not a new combination — just the same two marbles, order removed.
That count of 10 shows up somewhere else familiar, too: it's a number straight out of Pascal's Triangle, the "each number is the sum of the two above it" triangle usually met well before combinations are. Row 5 (5 flips, or 5 marbles) reads 1, 5, 10, 10, 5, 1 — the number of ways to land exactly 0, 1, 2, 3, 4, or 5 heads (or blue marbles) out of 5. The highlighted 10 is exactly 5C2 from Figure 5 above: choosing which 2 of the 5 come up heads (or blue) is the same count as choosing which 2 of the 5 marbles get seated.
What happens when a choice is really two separate choices, made from two separate groups? Say there are 3 men waiting and 2 women waiting, and the task is "seat 2 of the men, in order, and seat 1 of the women." One way to approach it: figure out how each group seats itself on its own, then multiply. That is exactly the multiplication rule from every seating example above — just run once for the men and once for the women.
Look closely at the 12 tiles above: they are not 12 different outcomes — they are 6 outcomes, each counted twice. Blue→Green + Purple and Green→Blue + Purple end up seating the exact same 3 people once chairs are involved; only the men’s order got flipped along the way. Build up each tile’s own stack of chairs below it (or press its Auto-fill button) until it reaches 6 of 6 — once both tiles of a redundant pair are complete, every seating in one tile turns out to have an identical twin sitting somewhere in the other. One seating gets circled at a time, but its twin is left unmarked, hiding somewhere in the other tile’s own stack — find it by eye, or hover over any finished seating to hear its own little piano note (a twin pair always plays the same note) and click the one that matches. Guess wrong and it just shakes; find the real twin and it evaporates, leaving the confirmed one behind. Work through all 6 twin pairs (or press either tile’s Auto-match button to watch it happen) to collapse the 12 tiles down to the 6 that actually matter.
Those 12 are not yet real 3-seat rows, though — each one is still "this men-order, next to this woman," not "these 3 people, seated in one line." To knock the wall down, permute all 3 people together: multiply by 3! for the 3 open seats. But that 3! re-permutes the 2 men who were already put in order, and the 1 woman who was (trivially) already in order — so divide those back out, the same correction the License Plate page uses to knock down its own wall between letters and numbers.
Now pick the other way: don't decide an order at all, just decide who’s in. The moment order is off the table, men and women are already mixed together in the same breath — there is no wall to knock down afterward, because nothing was ever separated by order to begin with.
Each circle above already is one merged group — 2 men plus 1 woman, nothing further to list. Once a circle is complete, its own 3 chairs appear right below it: drag its people in to seat them (or press that group’s own Auto-fill button). Filling a set reveals a fresh empty one underneath and resets the circle’s people so you can find a new order — keep going until all 3P3 = 6 orderings stack up for that group, then do the same for the other 5.
Both roads land on the same 36. Method 1 (permutations first) had to pay a 3! ⁄ (2!·1!) toll to knock its wall down after the fact; Method 2 (combinations first) never built a wall, so the only permuting left was the honest kind — seating the 3 already-chosen people, once, at the very end. Looking at an actual seated row, like Figure 2's or Figure 4's tree, is exactly what shows where that missing factor was hiding.
Every worked example above used fixed numbers — 5 marbles into 2 chairs, or all 3 into 3. Pick your own n (marbles waiting) and r (chairs to fill) and this builds the exact same kind of permutation tree, with the exact same drag-into-a-circle collapse, sized to whatever you choose — the tree rebuilds itself the moment you change either number, nothing to press. r is capped to whatever n currently is, since you can't choose more marbles than are waiting. Big combinations get hard to draw legibly, so very large choices of n and r are refused with a note explaining why, rather than attempting to render something unreadable.
That count is also sitting in Pascal's Triangle, beside the tree — row n reads the number of ways to choose 0, 1, 2, … all the way up to n of something out of n options, live as you change n and r.
A narrated, step-by-step walkthrough of the Binomial Distribution Explorer — read (or listen to) the setup below, then start the demo to see the interface come alive one piece at a time.
Each part below narrates a different piece of the Binomial Distribution Explorer, live, using the real controls and chart below — a narrator walks through it step by step, pausing here and there for you to click something yourself. Press any part's button to scroll down and start it; you don't need to go in order, though Parts 2 and 3 pick up the running example Part 1 sets up. You can pause the narration at any time with the button that appears once a part starts.
A coin-toss model, a real bone-marrow-match example, zooming in, and where its probabilities come from.
Draw a sample, run hundreds automatically, and use the histogram button to reveal the individual outcomes behind it.
A bigger, symmetric distribution, the histogram morphing into a bell shape, the normal-curve overlay, and the np/nq rule of thumb.
The binomial distribution isn't an approximation of anything — it predicts the actual result of flipping n coins. Sample from a process with a known probability of success p (the odds of a coin landing heads, say) over a fixed number of trials n (how many times you flip it), repeat that experiment over and over, and the results land exactly on the binomial distribution. That's not just a classroom exercise, either — it's the same math behind calculating the odds of a match for a bone marrow transplant, or how many left-handed people to expect in a small group. It can be built directly, outcome by outcome, with no approximation involved — which is exactly what the chart above is doing.
About 100 years ago, this was done with printed tables: a book of reference tables could reproduce a great many binomial distributions directly, one page per combination of n and p. But once n grew large, working in raw counts became unwieldy, so the scale was often switched to a proportion instead (X/n rather than X). The trouble was that no tables existed for that proportional distribution, and constructing one by hand — the same term-by-term way the binomial tables had been built — simply wasn't possible at that scale.
The only way forward was to invent a stand-in: a smooth, bell-shaped (Gaussian) curve that could approximate the real distribution without ever being it. Call it a ghost — a curve that looks like the distribution but was never actually built from it. Even that ghost wasn't practical on its own, though: a Gaussian curve has no closed-form antiderivative, so it cannot be integrated over an interval by hand, no matter how much calculus you throw at it. The workaround was to rescale every ghost curve's x-axis into Z-units — standard deviations from the mean, using the real standard deviation of the binomial or proportional distribution behind it. Once every ghost is measured this way, they all collapse into the exact same single, standard normal curve. That one curve was integrated by hand exactly once, producing a master reference — the Z-table — reusable for every ghost, for any n and p, because every Gaussian curve obeys the same fixed rule: 68.27% of its area sits within 1 standard deviation of the mean, 95.45% within 2, and 99.73% within 3 — always.
There's just one thing that whole method requires: the standard deviation of the binomial or proportional distribution being approximated.
Here's what most textbooks never say out loud: you can calculate that standard deviation without ever constructing the binomial or proportional distribution at all. That's possible because variance — the standard deviation squared — is linear: it simply adds up across independent trials, so it can be worked out directly from n and p alone, with no need to build the full distribution first. (You'll see exactly how, later in this tool.)
In a standard textbook, that standard deviation quietly becomes a Z-score, where “1” just means “one standard deviation of the binomial or proportional distribution” — which is also the standard deviation of its ghost — mapped onto the one generic bell curve printed in the book. But because the book never shows you the actual ghost, scaled to your specific n and p, you only ever see one fixed, moderately plump curve, and it's easy to assume every distribution looks like that. In reality, the ghost behind any particular binomial or proportional distribution can be very tall and very skinny (a small standard deviation relative to the mean) or short and wide (a large one) — and that difference is exactly what matters when you go on to compare two populations against each other.
Try it yourself. Press the ▶ Sweep n button next to Trials (n) below and watch its effect on the variance as n climbs from 1 to 1000 — the girth of the binomial (or proportional) distribution visibly changes right along with it. That's because variance is linear. Switch the x-axis to k/n first, then press the button again, and you'll see the paradox: instead of growing, the spread narrows. Later in this tool, we'll show that a higher n doesn't just narrow that spread — it also means more accurate predictions.
Take a sample. Press the orange Take 1 sample button and watch the coins show that sample's number of heads — plotted as a dot on the binomial distribution. Then press ▶ Run automatically: as the coin keeps getting tossed, sample after sample, you'll watch those dots build up into the very same shape the mathematical distribution already predicted.
Watch the ghost appear. Turn on the 🔔 Normal curve overlay, then press ▶ Sweep n. Once n is large enough, that curve stops being just an overlay — it becomes the ghost of the binomial distribution itself, and of the proportional distribution too if you're viewing k/n.
Putting the cart before the horse. Set n to 1000 and p to .001, with the x-axis on k (the binomial count view), then turn on the 🔔 Normal curve overlay — watch it not fit. That's the famous np = 1, below the rule-of-thumb minimum of 5, telling you right there that the normal approximation is a poor one here. Now turn on 🌟 Poisson instead: the magenta dots track the binomial very closely, right where a very high n meets a very low p. Again, that's the genius of the mathematicians who worked this out — a binomial distribution like this one, at n = 1000, couldn't have been built by hand, not even back when I was in high school.
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| -0.0 | 0.5000 | 0.4960 | 0.4920 | 0.4880 | 0.4840 | 0.4801 | 0.4761 | 0.4721 | 0.4681 | 0.4641 |
| -0.1 | 0.4602 | 0.4562 | 0.4522 | 0.4483 | 0.4443 | 0.4404 | 0.4364 | 0.4325 | 0.4286 | 0.4247 |
| -0.2 | 0.4207 | 0.4168 | 0.4129 | 0.4090 | 0.4052 | 0.4013 | 0.3974 | 0.3936 | 0.3897 | 0.3859 |
| -0.3 | 0.3821 | 0.3783 | 0.3745 | 0.3707 | 0.3669 | 0.3632 | 0.3594 | 0.3557 | 0.3520 | 0.3483 |
| -0.4 | 0.3446 | 0.3409 | 0.3372 | 0.3336 | 0.3300 | 0.3264 | 0.3228 | 0.3192 | 0.3156 | 0.3121 |
| -0.5 | 0.3085 | 0.3050 | 0.3015 | 0.2981 | 0.2946 | 0.2912 | 0.2877 | 0.2843 | 0.2810 | 0.2776 |
| -0.6 | 0.2743 | 0.2709 | 0.2676 | 0.2643 | 0.2611 | 0.2578 | 0.2546 | 0.2514 | 0.2483 | 0.2451 |
| -0.7 | 0.2420 | 0.2389 | 0.2358 | 0.2327 | 0.2296 | 0.2266 | 0.2236 | 0.2206 | 0.2177 | 0.2148 |
| -0.8 | 0.2119 | 0.2090 | 0.2061 | 0.2033 | 0.2005 | 0.1977 | 0.1949 | 0.1922 | 0.1894 | 0.1867 |
| -0.9 | 0.1841 | 0.1814 | 0.1788 | 0.1762 | 0.1736 | 0.1711 | 0.1685 | 0.1660 | 0.1635 | 0.1611 |
| -1.0 | 0.1587 | 0.1562 | 0.1539 | 0.1515 | 0.1492 | 0.1469 | 0.1446 | 0.1423 | 0.1401 | 0.1379 |
| -1.1 | 0.1357 | 0.1335 | 0.1314 | 0.1292 | 0.1271 | 0.1251 | 0.1230 | 0.1210 | 0.1190 | 0.1170 |
| -1.2 | 0.1151 | 0.1131 | 0.1112 | 0.1093 | 0.1075 | 0.1056 | 0.1038 | 0.1020 | 0.1003 | 0.0985 |
| -1.3 | 0.0968 | 0.0951 | 0.0934 | 0.0918 | 0.0901 | 0.0885 | 0.0869 | 0.0853 | 0.0838 | 0.0823 |
| -1.4 | 0.0808 | 0.0793 | 0.0778 | 0.0764 | 0.0749 | 0.0735 | 0.0721 | 0.0708 | 0.0694 | 0.0681 |
| -1.5 | 0.0668 | 0.0655 | 0.0643 | 0.0630 | 0.0618 | 0.0606 | 0.0594 | 0.0582 | 0.0571 | 0.0559 |
| -1.6 | 0.0548 | 0.0537 | 0.0526 | 0.0516 | 0.0505 | 0.0495 | 0.0485 | 0.0475 | 0.0465 | 0.0455 |
| -1.7 | 0.0446 | 0.0436 | 0.0427 | 0.0418 | 0.0409 | 0.0401 | 0.0392 | 0.0384 | 0.0375 | 0.0367 |
| -1.8 | 0.0359 | 0.0351 | 0.0344 | 0.0336 | 0.0329 | 0.0322 | 0.0314 | 0.0307 | 0.0301 | 0.0294 |
| -1.9 | 0.0287 | 0.0281 | 0.0274 | 0.0268 | 0.0262 | 0.0256 | 0.0250 | 0.0244 | 0.0239 | 0.0233 |
| -2.0 | 0.0228 | 0.0222 | 0.0217 | 0.0212 | 0.0207 | 0.0202 | 0.0197 | 0.0192 | 0.0188 | 0.0183 |
| -2.1 | 0.0179 | 0.0174 | 0.0170 | 0.0166 | 0.0162 | 0.0158 | 0.0154 | 0.0150 | 0.0146 | 0.0143 |
| -2.2 | 0.0139 | 0.0136 | 0.0132 | 0.0129 | 0.0125 | 0.0122 | 0.0119 | 0.0116 | 0.0113 | 0.0110 |
| -2.3 | 0.0107 | 0.0104 | 0.0102 | 0.0099 | 0.0096 | 0.0094 | 0.0091 | 0.0089 | 0.0087 | 0.0084 |
| -2.4 | 0.0082 | 0.0080 | 0.0078 | 0.0075 | 0.0073 | 0.0071 | 0.0069 | 0.0068 | 0.0066 | 0.0064 |
| -2.5 | 0.0062 | 0.0060 | 0.0059 | 0.0057 | 0.0055 | 0.0054 | 0.0052 | 0.0051 | 0.0049 | 0.0048 |
| -2.6 | 0.0047 | 0.0045 | 0.0044 | 0.0043 | 0.0041 | 0.0040 | 0.0039 | 0.0038 | 0.0037 | 0.0036 |
| -2.7 | 0.0035 | 0.0034 | 0.0033 | 0.0032 | 0.0031 | 0.0030 | 0.0029 | 0.0028 | 0.0027 | 0.0026 |
| -2.8 | 0.0026 | 0.0025 | 0.0024 | 0.0023 | 0.0023 | 0.0022 | 0.0021 | 0.0021 | 0.0020 | 0.0019 |
| -2.9 | 0.0019 | 0.0018 | 0.0018 | 0.0017 | 0.0016 | 0.0016 | 0.0015 | 0.0015 | 0.0014 | 0.0014 |
| -3.0 | 0.0013 | 0.0013 | 0.0013 | 0.0012 | 0.0012 | 0.0011 | 0.0011 | 0.0011 | 0.0010 | 0.0010 |
| -3.1 | 0.0010 | 0.0009 | 0.0009 | 0.0009 | 0.0008 | 0.0008 | 0.0008 | 0.0008 | 0.0007 | 0.0007 |
| -3.2 | 0.0007 | 0.0007 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0005 | 0.0005 | 0.0005 |
| -3.3 | 0.0005 | 0.0005 | 0.0005 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0003 |
| -3.4 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0002 |
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| 0.0 | 0.5000 | 0.5040 | 0.5080 | 0.5120 | 0.5160 | 0.5199 | 0.5239 | 0.5279 | 0.5319 | 0.5359 |
| 0.1 | 0.5398 | 0.5438 | 0.5478 | 0.5517 | 0.5557 | 0.5596 | 0.5636 | 0.5675 | 0.5714 | 0.5753 |
| 0.2 | 0.5793 | 0.5832 | 0.5871 | 0.5910 | 0.5948 | 0.5987 | 0.6026 | 0.6064 | 0.6103 | 0.6141 |
| 0.3 | 0.6179 | 0.6217 | 0.6255 | 0.6293 | 0.6331 | 0.6368 | 0.6406 | 0.6443 | 0.6480 | 0.6517 |
| 0.4 | 0.6554 | 0.6591 | 0.6628 | 0.6664 | 0.6700 | 0.6736 | 0.6772 | 0.6808 | 0.6844 | 0.6879 |
| 0.5 | 0.6915 | 0.6950 | 0.6985 | 0.7019 | 0.7054 | 0.7088 | 0.7123 | 0.7157 | 0.7190 | 0.7224 |
| 0.6 | 0.7257 | 0.7291 | 0.7324 | 0.7357 | 0.7389 | 0.7422 | 0.7454 | 0.7486 | 0.7517 | 0.7549 |
| 0.7 | 0.7580 | 0.7611 | 0.7642 | 0.7673 | 0.7704 | 0.7734 | 0.7764 | 0.7794 | 0.7823 | 0.7852 |
| 0.8 | 0.7881 | 0.7910 | 0.7939 | 0.7967 | 0.7995 | 0.8023 | 0.8051 | 0.8078 | 0.8106 | 0.8133 |
| 0.9 | 0.8159 | 0.8186 | 0.8212 | 0.8238 | 0.8264 | 0.8289 | 0.8315 | 0.8340 | 0.8365 | 0.8389 |
| 1.0 | 0.8413 | 0.8438 | 0.8461 | 0.8485 | 0.8508 | 0.8531 | 0.8554 | 0.8577 | 0.8599 | 0.8621 |
| 1.1 | 0.8643 | 0.8665 | 0.8686 | 0.8708 | 0.8729 | 0.8749 | 0.8770 | 0.8790 | 0.8810 | 0.8830 |
| 1.2 | 0.8849 | 0.8869 | 0.8888 | 0.8907 | 0.8925 | 0.8944 | 0.8962 | 0.8980 | 0.8997 | 0.9015 |
| 1.3 | 0.9032 | 0.9049 | 0.9066 | 0.9082 | 0.9099 | 0.9115 | 0.9131 | 0.9147 | 0.9162 | 0.9177 |
| 1.4 | 0.9192 | 0.9207 | 0.9222 | 0.9236 | 0.9251 | 0.9265 | 0.9279 | 0.9292 | 0.9306 | 0.9319 |
| 1.5 | 0.9332 | 0.9345 | 0.9357 | 0.9370 | 0.9382 | 0.9394 | 0.9406 | 0.9418 | 0.9429 | 0.9441 |
| 1.6 | 0.9452 | 0.9463 | 0.9474 | 0.9484 | 0.9495 | 0.9505 | 0.9515 | 0.9525 | 0.9535 | 0.9545 |
| 1.7 | 0.9554 | 0.9564 | 0.9573 | 0.9582 | 0.9591 | 0.9599 | 0.9608 | 0.9616 | 0.9625 | 0.9633 |
| 1.8 | 0.9641 | 0.9649 | 0.9656 | 0.9664 | 0.9671 | 0.9678 | 0.9686 | 0.9693 | 0.9699 | 0.9706 |
| 1.9 | 0.9713 | 0.9719 | 0.9726 | 0.9732 | 0.9738 | 0.9744 | 0.9750 | 0.9756 | 0.9761 | 0.9767 |
| 2.0 | 0.9772 | 0.9778 | 0.9783 | 0.9788 | 0.9793 | 0.9798 | 0.9803 | 0.9808 | 0.9812 | 0.9817 |
| 2.1 | 0.9821 | 0.9826 | 0.9830 | 0.9834 | 0.9838 | 0.9842 | 0.9846 | 0.9850 | 0.9854 | 0.9857 |
| 2.2 | 0.9861 | 0.9864 | 0.9868 | 0.9871 | 0.9875 | 0.9878 | 0.9881 | 0.9884 | 0.9887 | 0.9890 |
| 2.3 | 0.9893 | 0.9896 | 0.9898 | 0.9901 | 0.9904 | 0.9906 | 0.9909 | 0.9911 | 0.9913 | 0.9916 |
| 2.4 | 0.9918 | 0.9920 | 0.9922 | 0.9925 | 0.9927 | 0.9929 | 0.9931 | 0.9932 | 0.9934 | 0.9936 |
| 2.5 | 0.9938 | 0.9940 | 0.9941 | 0.9943 | 0.9945 | 0.9946 | 0.9948 | 0.9949 | 0.9951 | 0.9952 |
| 2.6 | 0.9953 | 0.9955 | 0.9956 | 0.9957 | 0.9959 | 0.9960 | 0.9961 | 0.9962 | 0.9963 | 0.9964 |
| 2.7 | 0.9965 | 0.9966 | 0.9967 | 0.9968 | 0.9969 | 0.9970 | 0.9971 | 0.9972 | 0.9973 | 0.9974 |
| 2.8 | 0.9974 | 0.9975 | 0.9976 | 0.9977 | 0.9977 | 0.9978 | 0.9979 | 0.9979 | 0.9980 | 0.9981 |
| 2.9 | 0.9981 | 0.9982 | 0.9982 | 0.9983 | 0.9984 | 0.9984 | 0.9985 | 0.9985 | 0.9986 | 0.9986 |
| 3.0 | 0.9987 | 0.9987 | 0.9987 | 0.9988 | 0.9988 | 0.9989 | 0.9989 | 0.9989 | 0.9990 | 0.9990 |
| 3.1 | 0.9990 | 0.9991 | 0.9991 | 0.9991 | 0.9992 | 0.9992 | 0.9992 | 0.9992 | 0.9993 | 0.9993 |
| 3.2 | 0.9993 | 0.9993 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9995 | 0.9995 | 0.9995 |
| 3.3 | 0.9995 | 0.9995 | 0.9995 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9997 |
| 3.4 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9998 |
| k \ p | 0.05 | 0.10 | 0.15 | 0.20 | 0.25 | 0.30 | 0.35 | 0.40 | 0.45 | 0.50 | 0.55 | 0.60 | 0.65 | 0.70 | 0.75 | 0.80 | 0.85 | 0.90 | 0.95 | 1.00 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 0 | 0.7351 | 0.5314 | 0.3771 | 0.2621 | 0.1780 | 0.1176 | 0.0754 | 0.0467 | 0.0277 | 0.0156 | 0.0083 | 0.0041 | 0.0018 | 0.0007 | 0.0002 | 0.0001 | 0.0000 | 0.0000 | 0.0000 | 0.0000 |
| 1 | 0.9672 | 0.8857 | 0.7765 | 0.6554 | 0.5339 | 0.4202 | 0.3191 | 0.2333 | 0.1636 | 0.1094 | 0.0692 | 0.0410 | 0.0223 | 0.0109 | 0.0046 | 0.0016 | 0.0004 | 0.0001 | 0.0000 | 0.0000 |
| 2 | 0.9978 | 0.9842 | 0.9527 | 0.9011 | 0.8306 | 0.7443 | 0.6471 | 0.5443 | 0.4415 | 0.3438 | 0.2553 | 0.1792 | 0.1174 | 0.0705 | 0.0376 | 0.0170 | 0.0059 | 0.0013 | 0.0001 | 0.0000 |
| 3 | 0.9999 | 0.9987 | 0.9941 | 0.9830 | 0.9624 | 0.9295 | 0.8826 | 0.8208 | 0.7447 | 0.6563 | 0.5585 | 0.4557 | 0.3529 | 0.2557 | 0.1694 | 0.0989 | 0.0473 | 0.0158 | 0.0022 | 0.0000 |
| 4 | 1.0000 | 0.9999 | 0.9996 | 0.9984 | 0.9954 | 0.9891 | 0.9777 | 0.9590 | 0.9308 | 0.8906 | 0.8364 | 0.7667 | 0.6809 | 0.5798 | 0.4661 | 0.3446 | 0.2235 | 0.1143 | 0.0328 | 0.0000 |
| 5 | 1.0000 | 1.0000 | 1.0000 | 0.9999 | 0.9998 | 0.9993 | 0.9982 | 0.9959 | 0.9917 | 0.9844 | 0.9723 | 0.9533 | 0.9246 | 0.8824 | 0.8220 | 0.7379 | 0.6229 | 0.4686 | 0.2649 | 0.0000 |
| 6 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 | 1.0000 |
Showing n = 6, p = 0.05 to 1.00. The highlighted column, p = 0.30, matches the chart's current success probability (p = 0.300). Click a k below to shade its row and highlight that cumulative sum on the chart.
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| -0.0 | 0.5000 | 0.4960 | 0.4920 | 0.4880 | 0.4840 | 0.4801 | 0.4761 | 0.4721 | 0.4681 | 0.4641 |
| -0.1 | 0.4602 | 0.4562 | 0.4522 | 0.4483 | 0.4443 | 0.4404 | 0.4364 | 0.4325 | 0.4286 | 0.4247 |
| -0.2 | 0.4207 | 0.4168 | 0.4129 | 0.4090 | 0.4052 | 0.4013 | 0.3974 | 0.3936 | 0.3897 | 0.3859 |
| -0.3 | 0.3821 | 0.3783 | 0.3745 | 0.3707 | 0.3669 | 0.3632 | 0.3594 | 0.3557 | 0.3520 | 0.3483 |
| -0.4 | 0.3446 | 0.3409 | 0.3372 | 0.3336 | 0.3300 | 0.3264 | 0.3228 | 0.3192 | 0.3156 | 0.3121 |
| -0.5 | 0.3085 | 0.3050 | 0.3015 | 0.2981 | 0.2946 | 0.2912 | 0.2877 | 0.2843 | 0.2810 | 0.2776 |
| -0.6 | 0.2743 | 0.2709 | 0.2676 | 0.2643 | 0.2611 | 0.2578 | 0.2546 | 0.2514 | 0.2483 | 0.2451 |
| -0.7 | 0.2420 | 0.2389 | 0.2358 | 0.2327 | 0.2296 | 0.2266 | 0.2236 | 0.2206 | 0.2177 | 0.2148 |
| -0.8 | 0.2119 | 0.2090 | 0.2061 | 0.2033 | 0.2005 | 0.1977 | 0.1949 | 0.1922 | 0.1894 | 0.1867 |
| -0.9 | 0.1841 | 0.1814 | 0.1788 | 0.1762 | 0.1736 | 0.1711 | 0.1685 | 0.1660 | 0.1635 | 0.1611 |
| -1.0 | 0.1587 | 0.1562 | 0.1539 | 0.1515 | 0.1492 | 0.1469 | 0.1446 | 0.1423 | 0.1401 | 0.1379 |
| -1.1 | 0.1357 | 0.1335 | 0.1314 | 0.1292 | 0.1271 | 0.1251 | 0.1230 | 0.1210 | 0.1190 | 0.1170 |
| -1.2 | 0.1151 | 0.1131 | 0.1112 | 0.1093 | 0.1075 | 0.1056 | 0.1038 | 0.1020 | 0.1003 | 0.0985 |
| -1.3 | 0.0968 | 0.0951 | 0.0934 | 0.0918 | 0.0901 | 0.0885 | 0.0869 | 0.0853 | 0.0838 | 0.0823 |
| -1.4 | 0.0808 | 0.0793 | 0.0778 | 0.0764 | 0.0749 | 0.0735 | 0.0721 | 0.0708 | 0.0694 | 0.0681 |
| -1.5 | 0.0668 | 0.0655 | 0.0643 | 0.0630 | 0.0618 | 0.0606 | 0.0594 | 0.0582 | 0.0571 | 0.0559 |
| -1.6 | 0.0548 | 0.0537 | 0.0526 | 0.0516 | 0.0505 | 0.0495 | 0.0485 | 0.0475 | 0.0465 | 0.0455 |
| -1.7 | 0.0446 | 0.0436 | 0.0427 | 0.0418 | 0.0409 | 0.0401 | 0.0392 | 0.0384 | 0.0375 | 0.0367 |
| -1.8 | 0.0359 | 0.0351 | 0.0344 | 0.0336 | 0.0329 | 0.0322 | 0.0314 | 0.0307 | 0.0301 | 0.0294 |
| -1.9 | 0.0287 | 0.0281 | 0.0274 | 0.0268 | 0.0262 | 0.0256 | 0.0250 | 0.0244 | 0.0239 | 0.0233 |
| -2.0 | 0.0228 | 0.0222 | 0.0217 | 0.0212 | 0.0207 | 0.0202 | 0.0197 | 0.0192 | 0.0188 | 0.0183 |
| -2.1 | 0.0179 | 0.0174 | 0.0170 | 0.0166 | 0.0162 | 0.0158 | 0.0154 | 0.0150 | 0.0146 | 0.0143 |
| -2.2 | 0.0139 | 0.0136 | 0.0132 | 0.0129 | 0.0125 | 0.0122 | 0.0119 | 0.0116 | 0.0113 | 0.0110 |
| -2.3 | 0.0107 | 0.0104 | 0.0102 | 0.0099 | 0.0096 | 0.0094 | 0.0091 | 0.0089 | 0.0087 | 0.0084 |
| -2.4 | 0.0082 | 0.0080 | 0.0078 | 0.0075 | 0.0073 | 0.0071 | 0.0069 | 0.0068 | 0.0066 | 0.0064 |
| -2.5 | 0.0062 | 0.0060 | 0.0059 | 0.0057 | 0.0055 | 0.0054 | 0.0052 | 0.0051 | 0.0049 | 0.0048 |
| -2.6 | 0.0047 | 0.0045 | 0.0044 | 0.0043 | 0.0041 | 0.0040 | 0.0039 | 0.0038 | 0.0037 | 0.0036 |
| -2.7 | 0.0035 | 0.0034 | 0.0033 | 0.0032 | 0.0031 | 0.0030 | 0.0029 | 0.0028 | 0.0027 | 0.0026 |
| -2.8 | 0.0026 | 0.0025 | 0.0024 | 0.0023 | 0.0023 | 0.0022 | 0.0021 | 0.0021 | 0.0020 | 0.0019 |
| -2.9 | 0.0019 | 0.0018 | 0.0018 | 0.0017 | 0.0016 | 0.0016 | 0.0015 | 0.0015 | 0.0014 | 0.0014 |
| -3.0 | 0.0013 | 0.0013 | 0.0013 | 0.0012 | 0.0012 | 0.0011 | 0.0011 | 0.0011 | 0.0010 | 0.0010 |
| -3.1 | 0.0010 | 0.0009 | 0.0009 | 0.0009 | 0.0008 | 0.0008 | 0.0008 | 0.0008 | 0.0007 | 0.0007 |
| -3.2 | 0.0007 | 0.0007 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0006 | 0.0005 | 0.0005 | 0.0005 |
| -3.3 | 0.0005 | 0.0005 | 0.0005 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0004 | 0.0003 |
| -3.4 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0003 | 0.0002 |
| z | 0.00 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
|---|---|---|---|---|---|---|---|---|---|---|
| 0.0 | 0.5000 | 0.5040 | 0.5080 | 0.5120 | 0.5160 | 0.5199 | 0.5239 | 0.5279 | 0.5319 | 0.5359 |
| 0.1 | 0.5398 | 0.5438 | 0.5478 | 0.5517 | 0.5557 | 0.5596 | 0.5636 | 0.5675 | 0.5714 | 0.5753 |
| 0.2 | 0.5793 | 0.5832 | 0.5871 | 0.5910 | 0.5948 | 0.5987 | 0.6026 | 0.6064 | 0.6103 | 0.6141 |
| 0.3 | 0.6179 | 0.6217 | 0.6255 | 0.6293 | 0.6331 | 0.6368 | 0.6406 | 0.6443 | 0.6480 | 0.6517 |
| 0.4 | 0.6554 | 0.6591 | 0.6628 | 0.6664 | 0.6700 | 0.6736 | 0.6772 | 0.6808 | 0.6844 | 0.6879 |
| 0.5 | 0.6915 | 0.6950 | 0.6985 | 0.7019 | 0.7054 | 0.7088 | 0.7123 | 0.7157 | 0.7190 | 0.7224 |
| 0.6 | 0.7257 | 0.7291 | 0.7324 | 0.7357 | 0.7389 | 0.7422 | 0.7454 | 0.7486 | 0.7517 | 0.7549 |
| 0.7 | 0.7580 | 0.7611 | 0.7642 | 0.7673 | 0.7704 | 0.7734 | 0.7764 | 0.7794 | 0.7823 | 0.7852 |
| 0.8 | 0.7881 | 0.7910 | 0.7939 | 0.7967 | 0.7995 | 0.8023 | 0.8051 | 0.8078 | 0.8106 | 0.8133 |
| 0.9 | 0.8159 | 0.8186 | 0.8212 | 0.8238 | 0.8264 | 0.8289 | 0.8315 | 0.8340 | 0.8365 | 0.8389 |
| 1.0 | 0.8413 | 0.8438 | 0.8461 | 0.8485 | 0.8508 | 0.8531 | 0.8554 | 0.8577 | 0.8599 | 0.8621 |
| 1.1 | 0.8643 | 0.8665 | 0.8686 | 0.8708 | 0.8729 | 0.8749 | 0.8770 | 0.8790 | 0.8810 | 0.8830 |
| 1.2 | 0.8849 | 0.8869 | 0.8888 | 0.8907 | 0.8925 | 0.8944 | 0.8962 | 0.8980 | 0.8997 | 0.9015 |
| 1.3 | 0.9032 | 0.9049 | 0.9066 | 0.9082 | 0.9099 | 0.9115 | 0.9131 | 0.9147 | 0.9162 | 0.9177 |
| 1.4 | 0.9192 | 0.9207 | 0.9222 | 0.9236 | 0.9251 | 0.9265 | 0.9279 | 0.9292 | 0.9306 | 0.9319 |
| 1.5 | 0.9332 | 0.9345 | 0.9357 | 0.9370 | 0.9382 | 0.9394 | 0.9406 | 0.9418 | 0.9429 | 0.9441 |
| 1.6 | 0.9452 | 0.9463 | 0.9474 | 0.9484 | 0.9495 | 0.9505 | 0.9515 | 0.9525 | 0.9535 | 0.9545 |
| 1.7 | 0.9554 | 0.9564 | 0.9573 | 0.9582 | 0.9591 | 0.9599 | 0.9608 | 0.9616 | 0.9625 | 0.9633 |
| 1.8 | 0.9641 | 0.9649 | 0.9656 | 0.9664 | 0.9671 | 0.9678 | 0.9686 | 0.9693 | 0.9699 | 0.9706 |
| 1.9 | 0.9713 | 0.9719 | 0.9726 | 0.9732 | 0.9738 | 0.9744 | 0.9750 | 0.9756 | 0.9761 | 0.9767 |
| 2.0 | 0.9772 | 0.9778 | 0.9783 | 0.9788 | 0.9793 | 0.9798 | 0.9803 | 0.9808 | 0.9812 | 0.9817 |
| 2.1 | 0.9821 | 0.9826 | 0.9830 | 0.9834 | 0.9838 | 0.9842 | 0.9846 | 0.9850 | 0.9854 | 0.9857 |
| 2.2 | 0.9861 | 0.9864 | 0.9868 | 0.9871 | 0.9875 | 0.9878 | 0.9881 | 0.9884 | 0.9887 | 0.9890 |
| 2.3 | 0.9893 | 0.9896 | 0.9898 | 0.9901 | 0.9904 | 0.9906 | 0.9909 | 0.9911 | 0.9913 | 0.9916 |
| 2.4 | 0.9918 | 0.9920 | 0.9922 | 0.9925 | 0.9927 | 0.9929 | 0.9931 | 0.9932 | 0.9934 | 0.9936 |
| 2.5 | 0.9938 | 0.9940 | 0.9941 | 0.9943 | 0.9945 | 0.9946 | 0.9948 | 0.9949 | 0.9951 | 0.9952 |
| 2.6 | 0.9953 | 0.9955 | 0.9956 | 0.9957 | 0.9959 | 0.9960 | 0.9961 | 0.9962 | 0.9963 | 0.9964 |
| 2.7 | 0.9965 | 0.9966 | 0.9967 | 0.9968 | 0.9969 | 0.9970 | 0.9971 | 0.9972 | 0.9973 | 0.9974 |
| 2.8 | 0.9974 | 0.9975 | 0.9976 | 0.9977 | 0.9977 | 0.9978 | 0.9979 | 0.9979 | 0.9980 | 0.9981 |
| 2.9 | 0.9981 | 0.9982 | 0.9982 | 0.9983 | 0.9984 | 0.9984 | 0.9985 | 0.9985 | 0.9986 | 0.9986 |
| 3.0 | 0.9987 | 0.9987 | 0.9987 | 0.9988 | 0.9988 | 0.9989 | 0.9989 | 0.9989 | 0.9990 | 0.9990 |
| 3.1 | 0.9990 | 0.9991 | 0.9991 | 0.9991 | 0.9992 | 0.9992 | 0.9992 | 0.9992 | 0.9993 | 0.9993 |
| 3.2 | 0.9993 | 0.9993 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9994 | 0.9995 | 0.9995 | 0.9995 |
| 3.3 | 0.9995 | 0.9995 | 0.9995 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9996 | 0.9997 |
| 3.4 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9997 | 0.9998 |
The Z-score was necessary because, when this math was developed, it wasn't possible to actually construct a large binomial or proportional distribution by hand. There had to be a way to get that distribution's mean and standard deviation without ever building it — because building it just wasn't possible.
That's the magic of it: later you'll see how to back into the mean and sigma (standard deviation) without constructing the distribution at all — the same trick you just worked through yourself, above.
Every row counts the outcomes of flipping a coin n times. Read it first as Heads and Tails, then see the exact same numbers fall out of the (a + b)ⁿ expansion below.
Each row is one number of coin flips, n. Row n=5 means 5 flips, and reading left to right, each number in that row tells you how many of the 32 possible outcomes (2⁵) land with a particular split of Heads and Tails.
The first number in row 5 is always 1 — there's exactly one way to get 0 Heads and 5 Tails (every single flip comes up Tails). The next number, 5, is the number of ways to get 1 Head and 4 Tails — the one Head could be the 1st flip, the 2nd, the 3rd, the 4th, or the 5th, so 5 different ways. The next number, 10, is the number of ways to get 2 Heads and 3 Tails. After that the row mirrors itself: another 10 for 3 Heads and 2 Tails, another 5 for 4 Heads and 1 Tail, and a final 1 for 5 Heads and 0 Tails.
Every ball below is labeled in small text at its upper right with that exact split, so row 5 reads 0H,5T · 1H,4T · 2H,3T · 3H,2T · 4H,1T · 5H,0T left to right.
Every row of the triangle is exactly that formula's own n!/(x!(n−x)!) coefficients, one row per n — the expansion above runs the first few terms (x=0,1,2,3), skips ahead, and shows the final x=n term so the whole pattern is visible. Hover any ball to see it three ways, one layer at a time, using the buttons below: 1. Addition rule shows just the two arrows from the pair just above it that add together to make it — Pascal's own shortcut, no formula needed. 2. Formula shows that ball's own n!/(x!(n−x)!), with an arrow pointing from the note to the ball it belongs to. 3. No calculator shows that same formula worked out long-hand, as the cancelled factors.
The addition trick in layer 1 is the whole point of the triangle: once one row is known, the next comes from simple addition instead of working out a fresh factorial ratio for every single value of x. Layers 2 and 3 are what that addition is secretly standing in for — a shortcut around exactly the labor-intensive n!/(x!(n−x)!) calculations, which is why Pascal's Triangle was so valuable long before calculators could do that arithmetic instantly.
Seeing conditional probability as areas of a square, one layer at a time. The physical bucket version of this same idea is over on the "Bayes: Urn" tab.
Let's define our terms:
H₁ = the probability of Heads on the 1st toss
H₂ = the probability of Heads on the second toss
T₁ = the probability of Tails on the 1st toss
T₂ = the probability of Tails on the second toss
Drag to change P(H₁) — P(T₁) adjusts automatically so they always add to 1.
Drag to change P(T₂) — P(H₂) adjusts automatically so they always add to 1. (The slider controls whichever of H₂/T₂ is currently on top — flip and it controls the other one.)
Drag to slide the whole block left or right without changing its width — it's forced to stop the moment it hits the edge of the full sample space (0 or 1).
T₁∩T₂ = T₁ × Chance(T₂|T₁)
T₁ (.50) × Chance(T₂|T₁) (50%) = T₁∩T₂ (.25)
H₁∩T₂ = H₁ × Chance(T₂|H₁)
H₁ (.50) × Chance(T₂|H₁) (50%) = H₁∩T₂ (.25)
T₁∩H₂ = T₁ × Chance(H₂|T₁)
T₁ (.50) × Chance(H₂|T₁) (50%) = T₁∩H₂ (.25)
H₁∩H₂ = H₁ × Chance(H₂|H₁)
H₁ (.50) × Chance(H₂|H₁) (50%) = H₁∩H₂ (.25)
We want the percentage of a Head on the second toss, H₂. We reduce the sample space down to H₁ only — we remove T₁ entirely, since we already know the 1st toss was a Head. It's obvious that getting a Head after getting a Head happens 50% of the time, but because this reduced space is not the complete original sample space, we can't call this a probability — only a percentage, Chance(H₂|H₁).
A new example, same idea as the coin-toss bucket — we'll build this one up the same way, one layer at a time.
Let's define our terms — change any of these and the box below updates:
A statistics textbook usually writes this as P(Test+ | Sick). We write it as a percentage instead — Chance(Test+|Sick) — because P(Sick) is a probability we already know, but P(Sick ∩ Test+) is the probability we're solving for, not one we start with. What we DO start with, for the Sick group specifically, is a rate: out of everyone who's sick, what percentage also tests positive. That's a known percentage, not an unknown probability — so to build the square below, we multiply it by P(Sick): P(Sick ∩ Test+) = Chance(Test+|Sick) × P(Sick).
Chance(Test+|Sick) = Chance(Test+ | given the probability (Sick)) = 95% {all cells of the Sick group that also test positive}
Chance(Test+|Healthy) = Chance(Test+ | given the probability (Healthy)) = 10% {all cells of the Healthy group that also test positive}
P(Test+) = P(Sick ∩ Test+) + P(Healthy ∩ Test+) = the probability that the test is positive
P(Sick ∩ Test+) = Chance(Test+|Sick) × P(Sick) = .95 × .01 = .0095
P(Healthy ∩ Test+) = Chance(Test+|Healthy) × P(Healthy) = .1 × .99 = .099
Zooming out: picture 10,000 people. P(Sick) puts 100 of them Sick and 9,900 Healthy. The two small boxes above are a 100-person sample from each group, painted to match the rates you typed in.
Before area diagrams like the one above, this was usually drawn as two overlapping circles instead -- purely for fun (and for a lesson). Click to see it:
Notice that the circles never move or resize, no matter what you type into P(Sick) or either test rate above -- they can't, since a Venn diagram doesn't encode probability as area or position in the first place. That's exactly the point: it tells you which group a cell belongs to, but there's no way to just look at it and see how much of the population is in each region -- your eyes have nothing to measure. Scroll back up to the square: there, the area itself IS the proportion, so "how much" is something you can actually see, not just calculate.
The physical version of the same idea: an actual bucket of balls you draw from, one trial at a time, then see what is left in the bucket for the next draw.
Set how many red and how many blue balls are really in the bucket — that fixes the true P(R₁) and P(B₁), shown as a decimal next to it. Then drag the slider (also a decimal, like 0.30) to try to match that split with your guess.
Step 1: You may set the number of red and blue balls, or leave them as they are. Then move the slider below to set P(R₁) on the rectangle -- this is Bucket 1's own ratio, fixed before any marble moves.
The purple-ringed "Bucket 1" pail at the start of Case I and the one at the start of Case II are the same bucket — literally a duplicate of "The Bucket — First Trial" above — just kept as two independent copies so dragging a ball for one case never uses up a ball the other case still needs. Drag either color from Case I's own bucket into its target pail, or either color from Case II's own bucket into its target pail — whichever case you drag from first claims that color. A dragged ball leaves that bucket for good, and once a color has come out on one side, that same color is locked out on the other, so you can't claim the same physical ball twice — the other case is still free to draw, just forced into whichever color is left. Case I's target bucket's count boxes are the only ones; Case II's target starts out matching Case I's but only changes from Case II's own drags (re-typing Case I's boxes resets Case II's target to match again).
Seeing conditional probability as areas of a square, one layer at a time. The physical bucket version of this same idea is over on the "Bayes: Urn" tab.
Rename any group below, then set how big each one is -- the other two always adjust so all three keep adding to 100%. Below that, set how likely each group is to support a tax increase.
Drag any slider to change that group's share — the other two adjust automatically so all three always add to 100%. Uncheck a group's box to remove it from the picture entirely -- its slice, its intersection, and its own Bayes line all disappear, and the Bayes puzzle below reworks itself to need only the remaining groups' boxes.
Each of these is independent of the others -- they don't need to add up to anything in particular. ("$↑" is shorthand for "Taxes Increase" above, so each label fits on one line.) Check a group's top box here to show its two brackets above Area A: the outer one spans that group's whole box (100%), the inner one spans just its "taxes increase" slice within that box. Check its lower box, next to "Chance(Taxes Decrease|...)", to show that same pair of brackets above Area B instead, with the inner one now sized to the "taxes decrease" slice -- both are checked by default. The slider itself always stays green for the "increase" share and black for the rest, to scale, never flipping sides. Pick "Chance(Taxes Increase|...)" or "Chance(Taxes Decrease|...)" below a slider to choose which one's result is shown -- the Increase side shows its "= value%" above the green, the Decrease side shows its own "= value%" above the black, one at a time, same size either way.
The base layer is just the three groups, each box sized to P(group). The green overlay inside each box is that same group's own share who support a tax increase.
Solid diagonal = group (blue/red/gold, left to right by default -- renaming a group above doesn't change its color). The green, opposite-sloping overlay inside each box is that same group's own "supports a tax increase" share, not a separate box.
P(D∩$↑) = Chance($↑|Democrat) × P(Democrat) = 0.17
P(R∩$↑) = Chance($↑|Republican) × P(Republican) = 0.17
P($↑∩S) = Chance($↑|Socialist) × P(Socialist) = 0.17
Turning it around with Bayes' Theorem: given that someone supports a tax increase, how likely are they to belong to each group? Every line below divides by the same thing -- the total P($↑), built from the union of all three groups' own intersections with it.
Try building these yourself: drag each box's own green value from the diagram above into any row's three blanks to build that row's own P($↑) -- the top row AND each Chance(...) line's own denominator below each need their own complete set of three (same three chips, reused four times over -- nothing is used up by dragging it). Once a row's three are filled, watch for the gray bar underneath: that's visibly less than the full width above, since this reduced sample space doesn't add up to 1 (which is exactly why the sliders above are labeled "Chance(...)", not "P(...)"). Also drag each line's own green box into its numerator below.
P(Democrat wins AND taxes go up) ∪ P(Republican wins AND taxes go up) ∪ P(Socialist wins AND taxes go up)
The probability that taxes increase
P($↑) = P(D∩$↑) ∪ P(R∩$↑) ∪ P($↑∩S)
Chance(a Democrat | given taxes went up)
P(D∩$↑)/P($↑)
Chance(a Republican | given taxes went up)
P(R∩$↑)/P($↑)
Chance(a Socialist | given taxes went up)
P($↑∩S)/P($↑)
The base layer is just the three groups, each box sized to P(group). The black overlay inside each box is that same group's own share for whom taxes go down -- the green "taxes go up" overlay from Area A is turned off here.
Solid diagonal = group (blue/red/gold, left to right by default -- renaming a group above doesn't change its color). The black, opposite-sloping overlay inside each box is that same group's own "taxes go down" share, not a separate box.
Using the diagrams above, work out each probability yourself and type it in -- as a percentage (6) or a decimal (0.06), either is fine.
Let's define our terms:
H₁ = the probability of Heads on the 1st toss
H₂ = the probability of Heads on the second toss
T₁ = the probability of Tails on the 1st toss
T₂ = the probability of Tails on the second toss
Drag to change P(H₁) — P(T₁) adjusts automatically so they always add to 1.
Drag to change P(T₂) — P(H₂) adjusts automatically so they always add to 1. (The slider controls whichever of H₂/T₂ is currently on top — flip and it controls the other one.)
Drag to slide the whole block left or right without changing its width — it's forced to stop the moment it hits the edge of the full sample space (0 or 1).
We want the percentage of a Head on the second toss, H₂. We reduce the sample space down to H₁ only — we remove T₁ entirely, since we already know the 1st toss was a Head. It's obvious that getting a Head after getting a Head happens 50% of the time, but because this reduced space is not the complete original sample space, we can't call this a probability — only a percentage, Chance(H₂|H₁).
The math to calculate the chance of a Head on the second toss given a Head on the 1st toss is expressed Chance(H₂|H₁).
P(H₁) × Chance(H₂|H₁) = P(H₁∩H₂)
P(H₁) (.5) × Chance(H₂|H₁) (50%) = P(H₁∩H₂) (.25)
This is the same as P(H₁) × P(H₂) = P(H₁∩H₂) = .25
You can just multiply without the conditioning because the outcome of the second flip is not influenced by the 1st toss — this is called independence. We will show next that when the chance of the second flip changes based on the 1st flip, there is no independence and you cannot multiply.
Two trees, a measuring tape, and the question every variance formula answers: how do you measure spread without the pluses and minuses cancelling out? This page works through MAD vs. variance, derives σ² = npq by hand for 3 coin flips, and shows why the count’s variance grows with n while the proportion’s variance shrinks.
Variance measures how wide a distribution is.
The smaller the spread, the easier it is to tell two results apart, and the better the decisions we can make.
The shadow on the ground is where the two distributions overlap. We can shrink the shadow by shrinking the variance, and the way to do that is to take a bigger sample (a larger n).
Two groups each take a test. Both groups average 50, but one group is spread out and the other is not. A good measure of spread should tell them apart. We divide by 3 (the whole group, n) every time, not n − 1.
Absolute value and squaring both get rid of the minus signs, so both fix the cancelling problem from the first method.
The squared version is the one statistics is built on, for these reasons:
Every coin flip adds the same amount of variance, pq. So the variance is linear in n:
and for the proportion:
This means we can calculate the variance without doing the math of building the distribution. With just n and p, we get the spread of the binomial and of the proportional distribution, without ever having the actual distribution in hand.
Before computers, building a large binomial by hand would have been impossible.
So we use this to construct a ghost of the distribution, and work with the ghost without ever constructing the real distribution in the first place.
Squaring changes the units to points², which is hard to picture. Taking the square root at the end brings the answer back to points, the same unit as the test scores.
The variance is the average squared distance from the mean, written E[(X − μ)²]. Weighting each squared distance by its probability f(x) gives the general formula. For our three test scores, each score has f(x) = ⅓, so multiplying by f(x) and adding is the same as dividing by 3.
Sum over every value x: its squared distance from the mean, times its probability.
= (x² − 2μx + μ²) f(x)Expand the square: (x − μ)² = x² − 2μx + μ².
= x² f(x) − 2μx f(x) + μ² f(x)Multiply each term by f(x) and split the one sum into three sums.
= x² f(x) − 2μ x f(x)this is μ + μ² f(x)this is 12μ and μ² are the same for every x, so they move outside the sums. Σ x f(x) is the definition of the mean, E(X) = μ. Σ f(x) adds up every probability, which is always 1.
= E(X²) − 2μ·μ + μ²·1Σ x² f(x) is the average of the squared scores, E(X²).
= E(X²) − 2μ² + μ²Below is the long, laborious work of finding the standard deviation for just 3 tosses of a coin. I actually did this myself by hand.
Now imagine doing this for 1000 flips: 1001 terms, each with its own Pascal's triangle number. By hand, that would not be possible.
When we show you binomial and proportional distributions with very large n, it is the computer doing this math.
Many textbooks never show the proportional distributions at all, and they skip the shadow we talked about. So when students do the calculations, they have no picture of what is going on. They are pushing numbers without a visual understanding, and without appreciating the genius of the mathematicians who figured out how to do the math without doing the math.
Flip a coin 3 times and let X be the number of heads. Each flip lands heads with probability p and tails with probability q = 1 − p. The number of ways to get each X comes from row 3 of Pascal's triangle: 1, 3, 3, 1.
Press the Next step button again and again to show the math one step at a time, with each step explained.
Do this one on paper, the same way as the 3 flips above. Let X be the number of heads in 2 flips. The number of ways now comes from row 2 of Pascal's triangle: 1, 2, 1.
Again, I actually did the one above. This one is just two flips — use a real piece of paper and try it yourself.
Work out this formula:
For a count of successes k, the variance is npq and the SD is √(npq). For the proportion k/n, divide the count by n, which divides the variance by n²: pq/n, and the SD becomes √(pq/n). Each measure has its own chart because their scales are so different. Use the x-axis slider to zoom in on small n, and drag across any chart to read off a value.
The count spreads out as n grows: 4 times as many trials gives twice the SD. The proportion does the opposite and tightens: 4 times as many trials gives half the SD. That is why raising n makes trees A and B skinnier, so a smaller gap between their p values stops overlapping, and why the two trees in the Variance Paradox grow in opposite directions.
Twice the proportion's SD is the familiar margin of error: at p = 0.50 and n = 1,000 it works out to about ±3.16% — the same "plus or minus 3 points" a poll of a thousand people is usually quoted at. p = 0.50 is the worst case (pq is largest there, so that orange curve is as wide as the margin ever gets); the purple curve starts at p = 0.20 instead, where pq is smaller, so it sits narrower than the fixed curve at the same n — move its p slider and watch it shift. The x-axis slider is deliberately non-linear: its first half covers n = 100 to 1,000, the next quarter covers 1,000 to 10,000, and the last quarter covers 10,000 to 100,000, so there's far more room to land precisely on the smaller n values where the curves move fastest. One dashed line now reads both curves at once — drag anywhere on the chart to move it — independent of the four charts above. The y-axis zooms in on its own as that dashed line moves out: it always snaps to the smallest "nice" scale that comfortably fits the curves right where the line sits, so the margin keeps shrinking into view — roughly 100% near the start, down around 10% by n = 200, about 4% by n = 1,000, and finer still out past 10,000 — with no button to click.
Above, we said the variance is our enemy: the wider the spread, the harder it is to tell two results apart. For a count of heads, the variance keeps growing, because variance is additive: every flip adds pq, so σ² = npq.
Now convert the binomial to a proportional distribution. We still use the same additive variance, but dividing by n² turns it into pq/n, and the variance paradoxically narrows as n grows.
Move the n slider to see the effect: the count tree on the left widens while the proportion tree on the right narrows.
Each dot is one experiment's z-score. Chance alone would usually put 2 or 3 of the 7 outside the dark band.
Seven F2 experiments, each expected to follow Binomial(n, p = 0.75). Every result lands close to 3 : 1, closer than chance usually allows.
| Trait | Dominant | Recessive | Total (n) | Ratio | Expected dominant | Off by | Binomial SD | z-score |
|---|
Flower color: Mendel scored seed-coat color (grey-brown vs white), which goes with purple vs white flowers.
Each experiment is a weighted coin: within ±1 SD with p ≈ 0.683. The count is Binomial(7, 0.683). Mendel got 7 of 7, which happens about 6.9% of the time.
Landing close to 3 : 1 is one question. Leaning the same direction every time is a different one: if someone were nudging borderline counts toward the expected ratio, results would land above expectation more often than below (or vice versa) more than chance allows. This is the sign test — each experiment is a coin flip again, but now "heads" means the observed count landed above its expected value, not that it landed close to it.
The 0.75 ratio isn't an assumption — it falls straight out of a monohybrid cross: one gene, two versions, complete dominance. Seed shape is the clearest example.
The gene has two alleles. R = round (dominant), r = wrinkled (recessive). Every pea plant carries two copies, one from each parent. A plant with at least one R looks round; only rr looks wrinkled.
Mendel's cross. He started with a true-breeding round plant (RR) and a true-breeding wrinkled plant (rr). Every first-generation offspring (F1) got one R and one r, so all were Rr and all looked round — the wrinkled trait seemed to vanish. He then let the F1 plants self-pollinate (Rr × Rr), and the 3 : 1 ratio shows up in that second generation (F2) — the generation every count on this page comes from.
| R (½) | r (½) | |
|---|---|---|
| R (½) | RR — round | Rr — round |
| r (½) | Rr — round | rr — wrinkled |
RR: ¼ round · Rr: ½ round (two boxes) · rr: ¼ wrinkled. Round = ¼ + ½ = ¾ = 0.75; wrinkled = ¼ = 0.25 — the 3 : 1 ratio.
Why this is binomial. Each F2 seed is an independent draw of one allele from each parent, which gives the four conditions a binomial model needs: two outcomes (dominant-looking or recessive-looking), a constant probability (every seed has the same 0.75 chance of looking dominant), independence (one seed's result doesn't affect the next), and a fixed number of trials (the seeds Mendel counted). So the number of round seeds out of 7,324 follows Binomial(n = 7,324, p = 0.75) — the same kind of curve drawn above for every trait on this page.
When you wouldn't expect 0.75. Several things can shift the ratio away from 3 : 1: incomplete dominance, where the heterozygote (Rr) looks different from RR — a red × white cross giving pink offspring produces 1 : 2 : 1 instead; a dihybrid cross tracking two genes at once, which gives 9 : 3 : 3 : 1; linked genes sitting close together on the same chromosome, which don't sort independently; and lethal alleles, where rr offspring die before they can be counted, shifting the surviving ratio. Mendel happened to pick seven traits that each behave as a single gene with complete dominance — a real part of why his results were so clean, even before the question of whether they were too clean.
The chi-square distribution comes out of a repeated-sampling experiment, the same way the binomial emerged when you flipped coins over and over. Each simulation below builds the curve from scratch, then uses it to make a decision.
Start with a population that is normally distributed and has a known standard deviation σ. Then repeat this recipe thousands of times:
The histogram that builds up is the chi-square distribution. It can't go below zero because it's a sum of squares, so it's lopsided with a long right tail.
Its shape depends on the degrees of freedom, n − 1. One is lost because distances are measured from the sample's mean instead of the true mean. Small df gives a very skewed curve; large df gives something close to a bell. The curve's average always equals its df.
In the top chart, each new sample appears at its own mean x̄, then slides over to sit on μ. Once both bells share a center, the only difference left is width, and width is what the statistic measures.
The Graph menu switches the histogram between three versions of the same comparison: the chi-square, the variance ratio (s²/σ² or σ̂²/σ²), and the SD ratio (s/σ or σ̂/σ). Switching doesn't take new samples. It redraws the same samples on a different scale, so the shape stays the same and only the numbers on the axis change. A sample that's far out on one scale is far out on all three, so they lead to the same decisions. The first one is used in practice because it matches the standard chi-square table for every sample size.
A sample bell narrower than the population bell gives a statistic below the df. A wider one gives a statistic above it. Sliding x̄ over to μ doesn't change any of the distances, which is why the mean never enters the statistic.
Changing μ or σ keeps the balls already in the histogram, so you can build half the pile with σ = 5 and the rest with σ = 30 and see one smooth curve. Changing n switches to a different curve, so each n keeps its own pile: move n away and back and its balls are still there. Try changing the mean. Nothing in the histogram changes, because the statistic only measures spread. Changing σ doesn't change it either, since dividing by σ² cancels it out. Only n changes the shape.
The sample SD can be computed two ways. s divides the sum of squares by n − 1; a TI-84 calculator shows it as Sx. σ̂ ("sigma hat") divides by n; a TI-84 shows it as σx. Both lead to the same chi-square, because (n − 1)·s² and n·σ̂² both equal the sum of squares. The s and σ̂ buttons choose which one the variance and SD ratios use.
Getting s: enter the data in L1, then STAT → CALC → 1-Var Stats. Use Sx (divides by n − 1) for everything on this page; σx divides by n.
Chi-square areas: 2nd → DISTR → χ²cdf(lower, upper, df). For example χ²cdf(0, 2.70, 9) ≈ 0.025 and χ²cdf(19.02, 1E99, 9) ≈ 0.025, which confirms the two critical values for n = 10.
Critical values: if your model has no inverse chi-square function, read χ²L and χ²R from a chi-square table (row df = n − 1), or use Excel =CHISQ.INV.RT(0.975, df) and =CHISQ.INV.RT(0.025, df).
Interval for σ: lower limit = Sx·√((n−1)/χ²R), upper limit = Sx·√((n−1)/χ²L).
Simulation 1 could place every ball because it knew σ. In real life you get one sample and σ is unknown. You still get an interval for σ in four steps: compute s, look up two chi-square numbers for df = n − 1, multiply s by √((n − 1) ÷ each number), and report the range. Those two table numbers never involve σ, because the chi-square curve is the same for every population. Simulation 1b does exactly that, then repeats it many times so you can check that about 95% of the intervals catch the hidden σ. The chart at the bottom shows where the two multipliers come from.
The chi-square chart. The curve and its two red critical values depend only on n and the confidence level, never on σ. Your ssample sits at the mean of the curve (gold notch), the spot where σ would equal s. Each red line turns into a multiplier, σ ÷ s = √(df ÷ χ²): the top green bar shows the two multipliers (Lmult, Umult), and the bar under it multiplies them by your s to give the lower and upper limits.
The drop. Each new sample's bar slides down onto a real σ scale and flips, because a bigger σ sits on the left of the χ² chart but on the right of a σ scale. There the true σ (dashed blue line) stays put while the intervals move. Optional: drag the ball to see where any other value of σ would place your sample; it turns red past a critical value.
The interval list. Every sample's interval for σ, newest on top. With σ hidden they are gray, because nobody knows σ; with it shown, each turns green if it caught σ or red if it missed. About 95% should be green, even though each was built without knowing σ. The gold notch on each bar is that sample's s; at small n it sits left of center (the interval reaches farther above s than below), and it moves toward the middle as n grows. Click any interval to load that sample; the chart shows it too, and a red one's small dot lands in a red tail.
Now the curve becomes a yardstick. Someone claims "this population's standard deviation is σ₀." That's the null hypothesis, H₀. The rejection rule:
Population A matches the claim. Population B has a different standard deviation. Every sample from both is scored against A's σ₀.
The other possible mistake is missing a real difference. When one of B's samples lands between the cutoffs, the test fails to reject a claim that's false for B. That's a Type II error, and its rate is 1 − power. After each round, the simulation names the outcome for each sample.
The top chart works like Simulation 1. Population A's bell (the claim, σ₀) stays fixed. Each new sample appears as a dashed bell at its own mean, then slides over to sit on A's mean, so you can compare its width with the claimed σ₀. Use Show A and Show B to hide either population's samples.
Things to try: move B's mean and notice nothing changes, since this test only sees spread. Raise n toward 100 and watch B's rejection rate climb toward 100%. Set B's σ below A's and its values pile into the left tail, which is why this test checks both tails.
Two related tests: to compare means, use a t-test. To compare two samples' variances without a claimed σ₀, divide one sample variance by the other. That ratio follows an F distribution, which is built from two chi-squares. Part 4 simulates it.
One caution: this variance test assumes the population really is normal, and more data doesn't fix that.
Chi-square isn't limited to measurements like height and weight. Its most common use is with counts, including the binomial.
Flip a coin m times and count heads. If the claim is that P(heads) = p₀, you expect m·p₀ heads and m·(1 − p₀) tails. Compare what you observed to what you expected, category by category:
With two categories this is exactly a squared z-score for the binomial, (X − m·p₀)² / (m·p₀(1 − p₀)). Because the binomial looks normal once m is large enough, the statistic follows a chi-square curve with df = categories − 1 = 1.
The rejection rule only uses the right tail here. Too many heads and too few heads both square into a large positive number, so "far from expected" always means "large χ²". Reject the claim when χ² is above the cutoff (3.84 for α = 0.05).
The approximation needs enough data: every expected count should be at least about 5. Set m small and you'll see the histogram turn spiky and pull away from the curve, because a handful of flips can only produce a few possible values.
Latest round of flips. Filled part is heads; the red tick marks the expected number of heads under the claim.
With more categories, such as the six faces of a die, the same formula sums six terms and the df becomes 6 − 1 = 5.
Parts 2 and 3 checked one sample against a claimed value. The F test has no claimed value. You take a sample from each of two populations, X and Y, and ask whether their standard deviations are the same.
If the two populations really have the same spread, their sample variances should be similar, so F should land near 1. A ratio far above 1 or far below 1 is evidence that the spreads differ.
From Part 1, (n_X − 1)·s_X² / σ_X² follows a chi-square curve with n_X − 1 df, and the same is true for Y. Divide each one by its own df and take the ratio:
If σ_X = σ_Y, the two σ's cancel, and what's left is just s_X² ÷ s_Y². So when the spreads are equal, F follows an F distribution with two df numbers: n_X − 1 for the top and n_Y − 1 for the bottom. The order matters; swapping X and Y swaps the df.
The two sample sizes don't need to match. Each one just sets its own df.
Things to try: set the two SDs equal, and the rejection rate settles near α; every rejection is then a false alarm. Make the SDs different, and the rejection rate becomes the test's power. Raise both sample sizes and power climbs. Change either mean, and nothing happens.
One caution: the F test is very sensitive to non-normal data, even more than the variance test in Part 2. With skewed or heavy-tailed data, statisticians usually switch to Levene's test.
Is a filling machine's volume more variable than the spec allows? Is a lab instrument as precise as claimed? How volatile is an asset compared with a benchmark? This is Part 2. Comparing two machines or two methods with each other is the F test in Part 4.
Is a die fair? Do genetic crosses match Mendel's 3:1 ratio? Do binomial counts match a claimed p? This is Part 3, extended to any number of categories.
Does a treatment's success rate differ by group? Do survey answers depend on age? Counts in a table are compared with what independence predicts. This is what most people mean by "a chi-square test."
Both tests reject null hypotheses. Each one rejects a different null hypothesis, so you choose by the question you're asking.
| Your question | Null hypothesis | Test | On this page |
|---|---|---|---|
| Does one population's spread match a claimed value? | σ = σ₀ | Chi-square | Simulation 2 |
| Do counts match expected proportions, like a fair coin or die? | The proportions are as claimed | Chi-square | Simulation 3 |
| Are two categorical variables related, like treatment and outcome? | They're independent | Chi-square | Not simulated |
| Do two populations have the same spread? | σ_X = σ_Y | F | Simulation 4 |
| Do three or more groups have the same mean? | All means are equal | F (ANOVA) | Simulation 15 |
| Does a regression model explain anything? | All slopes are zero | F | Not simulated |
Chi-square compares one thing to a fixed benchmark you already know, like a claimed σ or the expected counts. F compares two estimated variances to each other, with no benchmark known in advance. ANOVA works this way too: it compares the variation between group means to the variation within groups.
The rejection rule is the same for both. Compute the statistic, find the cutoff that leaves α in the tail (α/2 in each tail for a two-sided test), and reject the null hypothesis if the statistic lands past it. They just use different curves to set the cutoff.
Questions that came up while working through the simulations, with the answers.
No. Two similar-looking formulas are easy to mix up.
The population variance uses f(x): σ² = Σ (x − μ)²·f(x). You list every possible value and weight each by its probability. For continuous data the sum becomes an integral.
The sample sum of squares, Σ (xᵢ − x̄)², doesn't. Each value you actually drew counts once, and common values show up more often in the sample, so the weighting is already built in. If you roll a die six times and get 2, 2, 5, 3, 2, 4, the value 2 gets added three times, which is the same as weighting it by 3/6.
Dividing the sample sum by n − 1 gives s², which estimates σ². The chi-square statistic divides the sample sum by the true σ², so it asks how this sample's spread compares with the population's.
Distances are measured from x̄, not μ, which is why df = n − 1. Using the true μ would also give a chi-square curve, with df = n.
Take an example with n = 4 and σ = 10:
In the bottom chart, the blue bars are a histogram of every statistic so far, scaled so the total area is 1. The black curve is the theoretical chi-square curve, drawn from its formula. The triangle under the axis marks the current sample. One value adds one tally to one bar; the shape only appears once many samples pile up.
Neither. Each sample is compared to the claim, not to the other sample.
In real life you'd have one sample and wouldn't know whether the claim is true. A shows what samples look like when the claim is true; B shows what they look like when it's false.
Each number is checked against the red cutoffs on its own. The sample sizes match only so both histograms can share one curve; different sizes would each need their own df and cutoffs. To compare two populations' spreads directly, use the F test in Part 4.
You are comparing the sample to the population. The statistic just uses variances and multiplies by n − 1:
With s² = 44.33 and σ² = 100, s²/σ² = 0.443: the sample's variance is about 44% of the population's. Multiplying by n − 1 = 3 gives 1.33.
Multiplying by n − 1 is what makes the result match the standard chi-square curve, which is defined as a sum of squared z-scores. Variances are used instead of SDs because squares are what add up. s/σ works too, but its distribution (the chi distribution) is messier to work with.
| Quantity | Typical value | Distribution |
|---|---|---|
| s / σ | near 1 | Chi (rarely used) |
| s² / σ² | near 1 | Chi-square ÷ df |
| (n − 1)·s² / σ² | near n − 1 | Chi-square (the standard table) |
All three rank samples the same way, so they lead to the same decisions. The Graph menu in Simulation 1 switches between them.
It's built only from positive pieces. Each distance is squared, so a point 5 below the mean and a point 5 above it both add 25. σ² is positive, and so is the df. A sum of squares divided by positive numbers can't go below zero. It would only equal zero if every value in the sample were identical, which essentially never happens with continuous data.
That's why the curve starts at zero and is squeezed against it. Too little spread shows up near zero; too much shows up far to the right.
Neither is more correct. One is the other divided by a fixed number, so they always lead to the same decision. They're useful for different things.
Chi-square matches the standard tables and software, so it's what you use to get cutoffs and p-values. Its average is the df and its variance is 2 × df.
Chi-square ÷ df is easier to read: it's centered at 1 for any sample size, so 0.44 means "the sample variance is 44% of the claimed variance." Its spread shrinks as df grows (variance 2 ÷ df), showing that bigger samples estimate the variance more precisely. In Simulation 1, choose s²/σ² and drag n from 4 to 100 to watch it tighten around 1.
No. Because of the long right tail, the peak, median, and mean sit in different places:
| Feature | Where it sits | Example: n = 4, df = 3 |
|---|---|---|
| Peak (most common value) | df − 2 (zero for df 1 or 2) | 1 |
| Median | about df − ⅔ | about 2.37 |
| Mean | df | 3 |
In Simulation 1, df = n − 1. With large samples the curve becomes nearly symmetric and all three crowd together; at df = 99 they're about 97, 98.3, and 99.
The divided version is still used where it helps interpretation: the F test is a ratio of two of them, and scientists report a "reduced chi-square" near 1 as a sign of good fit. The convention: calculate with chi-square, interpret with chi-square ÷ df.
Three coffee populations whose means start equal (all the same, hidden), each with the bean σ = 23.74 mg. Every round draws three samples. Then it does what a tempting shortcut does: it picks the two samples whose means are farthest apart and runs a two-sample test on just those two. Because you picked the most extreme pair after looking, that test rejects H₀ far more often than α, even though nothing is different. The same three samples are also run through a one-way ANOVA, which tests all three at once and keeps the error rate at α.
Yes, ANOVA compares sample means. The question is whether three or more groups come from populations with the same mean. The null hypothesis is μ₁ = μ₂ = μ₃, and the alternative is that at least one mean is different.
The surprise is how it does it. Despite the name, analysis of variance answers a question about means by comparing two variances, and the comparison is an F test.
When the null hypothesis is true, both are estimates of the same σ², so F lands near 1. When the means differ, MSB is inflated and F gets large. That's why ANOVA only rejects in the right tail: means that differ can only push F up.
The chi-square connects here too. SSB/σ² follows a chi-square with k − 1 df, and SSW/σ² follows one with N − k df. Divide each by its df, take the ratio, and σ² cancels, which gives the F distribution from Part 4.
ANOVA assumes each population is normal and that all groups share the same σ. With only two groups, ANOVA's F equals the square of the two-sample t statistic, so the two tests agree.
| Calculation | Result |
|---|
Picture a bell centered at the grand mean with SD = √MSW, the pooled spread of single values. Individual values from all three groups should mostly fall inside it. But that bell is the wrong yardstick for group means, because a mean of n values varies less than a single value. Its bell has SD = √(MSW ÷ n), the standard error.
If all three populations share one mean, the three sample means should scatter about as much as that narrow bell says. If one mean sits far out in its tail, that's a sign of a real difference. ANOVA makes this exact comparison, using all three means at once:
That equals MSB ÷ MSW, since MSB = n × (variance of the group means). Eyeballing whether each mean is within 2 standard errors is a helpful picture, but it isn't the test itself: checking groups one at a time raises the chance of a false alarm. The F test combines all the means into one number with a controlled α.
Things to try: set all three means equal, and the rejection rate settles near α, with every rejection a Type I error. Spread the means apart and watch the red segments grow, MSB rise, and the histogram slide right. Raise σ with the means held fixed, and the groups overlap more, so the test has a harder time telling them apart. Raise n, and it gets easier.
The same ANOVA rounds tested two ways. The pooled test estimates σ from all three groups (more degrees of freedom); the not-pooled test uses Group 1’s variance alone (fewer degrees of freedom, so a higher cutoff). Watch how often each one catches a real difference.
Denominator uses only Group 1’s variance s1² instead of MSW: Fnot pooled = MSB ÷ s1² = [(√MSB ÷ √n) ÷ (s1 ÷ √n)]². Fewer degrees of freedom (10 − 1 = 9 df) means a higher cutoff.
| Test | Denominator | df | F this round | Cutoff | Decision |
|---|
| Calculation | Result |
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The same repeated-sampling idea, now for means instead of counts: build the sampling distribution of x̄ from a real population, estimate its spread, and use it for confidence intervals and two-sample tests.
A rebuild of the original Flash lab. The population is the 1,231 coffee beans we weighed (mg). Work through it in order: Display the population as raw counts, Normalize it so the area is 100%, take samples to build the sampling distribution of x̄, use Estimate SD and the slider to find σx̄ = σ ÷ √n, then sample from an unknown population and move the handles to find its p-value.
A real, finite population: the 1,231 coffee beans we weighed, μ = 128.45 mg on average with σ = 23.74 mg. Switch to “Simulated normal” to set μ, σ and the population size yourself. Display shows raw counts of beans per bin. Normalize divides each count by N × bin width so the total area is 100% and the bars match the normal curve f(x). Each sample draws n beans without replacement (blue); its mean x̄ drops into the sampling distribution below, which narrows to σ ÷ √n.
| Calculation | Result |
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The same population, but now we pretend σ is unknown. Each sample estimates the sampling distribution with its own s ÷ √n, and that curve slides over to μ so you can compare the shapes. A larger n gives narrower, more consistent curves; “Apply t” shows the t shape with n − 1 df.
| Calculation | Result |
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A rebuild of the "Coffee σ vs s" Flash lab, using the same 1,231 beans. Each column samples the population at its own n. Each sample's bell, with SD = s, appears at x̄ (gold), slides onto μ, and then drops and shrinks to SD = s ÷ √n (green) on top of the true sampling distribution σ ÷ √n (brown). The counts show how often s comes out below σ, which is why a z interval built from s is too narrow and the t interval is needed, especially at small n.
A copy of the sampling-distribution simulation to build confidence intervals on. It runs separately from Simulations 6 and 7.
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A rebuild of the "Coffee CI z vs t" Flash lab. The population (our 1,231 beans) starts hidden, as it would be in a real study. Each sample's bell (SD = s) appears at x̄ and drops into the lower chart, shrinking to SD = s ÷ √n. The shaded part is x̄ ± z*·s/√n. Apply t stretches that interval to x̄ ± t*·s/√n. Run many samples, count how often each interval misses μ, then Reveal the population to check.
Step one, with no testing yet. Two coffee populations (the beans shifted to the means you choose, σ = 23.74 mg each). Every round samples both, subtracts the sample means, and drops the difference onto the lower chart. Over many rounds the differences build a bell centered at μ₁ − μ₂ with standard deviation σ√(1/n₁ + 1/n₂). The next part adds cutoffs, confidence intervals and errors to this same bell.
The same bell as Part 14, now with testing layered on: the ±1.96·SE cutoffs from 0, the rejection zone, each round’s confidence interval, the verdict and the type of error. Both coffee populations are shown (the 1,231 beans shifted to the means you choose, σ = 23.74 mg each). Each round samples n₁ beans from population 1 and n₂ from population 2, subtracts the sample means, and drops x̄₁ − x̄₂ onto the lower chart. Repeat it many times and the differences pile up into a bell centered at μ₁ − μ₂ with standard deviation σ√(1/n₁ + 1/n₂). That bell is the curve Part 16 uses for its intervals and tests.
Two populations of coffee beans whose means you set, then hide. Both are the 1,231 weighed beans shifted to the chosen mean, so both have the same σ = 23.74 mg as the bean population. Each round samples n₁ beans from population 1 and n₂ from population 2, then estimates μ₁ − μ₂ with x̄₁ − x̄₂ ± z*·σ√(1/n₁ + 1/n₂), using the known bean σ. For comparison it also shows the pooled t interval you would use if σ were unknown, and tests H₀: μ₁ = μ₂.
Three parts: build the best-fit line from the runs and rises in the data, read the line through a worked example and a replicated-data simulation, then test whether the line is more than noise.
Graph 1 builds the best-fit line from a few points, one step at a time: runs, rises, Sxx, Sxy, the slope, the line ŷ, the misses, SSE, MSE and SE(b).
Graph 2 follows the noise as a chain of arrows: the misses add up to SSE, then MSE, then √MSE, and the runs add up to √Sxx.
A few easy points so you can do it by hand. Some points share the same x, just like the replicated dots in the Regression tab. Pick a set, then press Next to add one idea at a time.
Each dot's miss from the line becomes an arrow. Every new arrow turns a right angle, so by Pythagoras the distance from the start grows as √(sum of the squared misses). At the end that distance is √SSE.
Every sample gives a slightly different line. Graph 1 shows the bells and the SE at each x, and compares confidence intervals with the truth. Graph 2 splits the wobble into shift (sliding up and down) and tilt (rocking around x̄) and puts them back together, with the newest sample's dots. Graph 3 repeats the sample many times, piles up the slopes, and checks how often the CIs catch the truth.
True population (button, off at first) = brown bells filled with evenly spread population dots at each x; the middle of each bell is the true mean μ. While it is on, the sample's own dots are hidden.
Black dashed line = a reveal of the unknown population line. You never see this in real life.
Blue line = the regression line ŷ, this sample's estimate of the unknown line.
Magenta = x̄ and ȳ (the regression line always passes through them); black long-dash = the true ȳ.
Brackets at each x: brown on the right = the truth (± σ, thick ± σ÷√n); teal and blue on the left = this sample (thick ± SE, ± √MSE).
Dotted teal = ± t·SE, the 95% CI: ✓ = it reaches the unknown line, ✗ = it misses. Teal fan = the CI for the slope; a red dashed ȳ line means it includes slope 0.
Each sample's line differs from the true line in two separate ways. Left: only its up-or-down shift (same slope as the true line). Right: only its tilt around the center. Add the two and you get the real line (bottom panel).
Same true line and same noise as the graph in the Testing tab. Each sample draws fresh dots from the same populations and fits a new line. Old lines stay light gray, so you can watch the wobble build up.
Each sample starts from the true line. First it slides up or down (the shift), then it turns around its new center (the tilt), and lands on the line that sample really fits. Old lines stay gray.
Regression uses the same idea as ANOVA: split the spread of y into a part we can explain and a leftover part that is just noise.
When we have several y values at each x, we can measure the noise first, with no line at all: compare each y with the mean of its own x and pool those squared distances. That is SSW again, called pure error in regression, and it estimates σ².
Then we fit the best-fit line: the one line that makes the squared vertical distances from the points to the line as small as possible.
This is the last step: with the slope, the noise and the wobble in hand (the Building and Regression tabs), this graph tests how well the line fits the data.