Normal Distribution Calculator
Find normal distribution probabilities and critical values for any mean and standard deviation, instantly.
๐ What is the Normal Distribution?
The normal distribution (also called the Gaussian distribution or bell curve) is the most important probability distribution in statistics. It describes the spread of a continuous random variable that clusters symmetrically around a central mean, with the probability of values decreasing smoothly as you move away from the center. The shape is completely determined by two parameters: the mean (mu), which controls the center, and the standard deviation (sigma), which controls the spread. A wider bell means higher standard deviation; a narrower, taller bell means lower standard deviation.
The normal distribution appears throughout science, engineering, finance, and social science. Heights and weights in a population, measurement errors in scientific instruments, IQ scores (standardized to mean 100, SD 15), blood pressure readings, exam score distributions, and the daily returns of financial assets are all commonly modeled as approximately normal. More fundamentally, the Central Limit Theorem guarantees that the mean of any sufficiently large sample follows a normal distribution regardless of the underlying population distribution, which is why the normal distribution is central to statistical inference.
A common misconception is that the normal distribution is always the right model. Many real-world distributions have heavier tails (more extreme values) than the normal, including financial returns, income distributions, and many biological measurements. The normal distribution is also bounded by the symmetric bell shape, whereas data like heights, weights, and prices must be positive. Despite these limitations, the normal distribution provides an excellent approximation for many purposes, and its mathematical tractability makes it indispensable in statistics.
This calculator covers the two most common normal distribution computations. The Find Probability mode calculates the area under the normal curve to the left of x (left-tail CDF), to the right of x, between two values, or outside a range. The Find X (Inverse) mode solves the reverse problem: given a probability, find the x value at which the cumulative area equals that probability. This is used for computing percentiles, critical values, and confidence interval boundaries.
๐ Formula
Cumulative distribution function (CDF) giving P(X < x):
Probability density function (PDF, the height of the bell curve at x):