Two districts can share a mean and a standard deviation and still look nothing alike: one symmetrical, the other with a long tail of very rich households. Skewness says which way the data lean and kurtosis says how heavy the tails are. This lesson builds both, from the order of the averages to the moment formulas, and ends with the box plot, the quickest way to see a distribution’s shape.
Ashanagar is an invented district. The statistics lessons use it for every worked example, so you meet the same households again as the ideas build: first as a list of numbers, then as a spread, then as a population to sample from.
It has 60 households, each with a monthly income in rupees. Unless a page says otherwise, those 60 are the whole population, and a “sample” means a few of them drawn at random. Where a page needs two variables, it uses a smaller set of 12 households with the head’s years of schooling beside income.
The figures are illustrative, made up once and fixed. They are not official statistics.
The first four lessons gave you two summaries of a data set: where it is centred and how far it spreads. Neither says anything about its shape. Picture the incomes of the sixty Ashanagar households. The mean is ₹28,783 and the median ₹25,000. Most households earn around the median, and then a few earn a good deal more. Draw the histogram and the right-hand side trails off into a long tail; there is no matching tail on the left, because no household earns less than ₹10,500.
That lopsidedness is called skewness. A distribution is symmetrical if its right half is the mirror image of its left (Hyderabad 2018 words it exactly that way). It is positively skewed if the long tail runs to the right, and negatively skewed if it runs to the left. The word describes the tail, not where the bulk of the data sit.
A second feature matters too. Two symmetrical distributions with the same mean and standard deviation can differ in how much of their weight sits in the centre and how much out in the tails. That is kurtosis, and it gets its own section below. Both ideas are about the same question: what does the picture look like when the mean and the standard deviation have already been taken out?
The mean, median and mode respond to a tail in different ways. The mode sits under the highest point of the curve and ignores the tail. The median is the middle value and moves only a little. The mean adds up every value, so it is pulled furthest toward the tail. That gives an order you can read straight off:
| Shape | Long tail | Order of the averages | Skewness |
|---|---|---|---|
| Positively skewed | to the right | mean > median > mode | positive |
| Symmetrical | none | mean = median = mode | zero |
| Negatively skewed | to the left | mean < median < mode | negative |
The order holds for the usual single-peaked shapes. Oddly shaped distributions can break it, but exam questions treat it as the rule.
Try it below. The two sliders set how much weight the curve puts on the left and on the right; the three averages are drawn on it, and three coefficients of skewness (explained in the next section) are worked out beside it. Start with the right-skewed preset, then flip to left-skewed and watch the mean and the mode swap places with the median always between them.
The long tail points right (positive skew). The mean is dragged furthest into the tail, the mode stays under the peak, and the median falls between them: mean > median > mode.
Find the tail. In the usual single-peaked shapes the mean is closer to it than the median is, and the mode is furthest from it. So “mean > median” points to a right tail and “mean < median” to a left one.
The examiners ask the same thing in many forms:
The order of the averages tells you the direction. To say how much, and to compare two distributions measured in different units, you need a coefficient with no units. There are three families, and exams name all of them.
The gap between the mean and the mode grows with the skew. Dividing it by the standard deviation removes the units:
A mode is awkward to find in real data, and it can be several values or none. For a moderately skewed distribution, one that is not too lopsided, there is an empirical relation that lets you drop it: the median sits roughly one third of the way from the mean toward the mode, which gives
With it, the mode can be replaced and Pearson’s second coefficient needs only the mean, median and standard deviation: . For the Ashanagar incomes this gives 3 × (28,783 − 25,000) ÷ 13,366 = 0.85, a clear right skew.
The relation also lets you recover a missing average. If the mean is 28 and the mode 25, the median is (2 × 28 + 25) ÷ 3 = 27 (CUET 2021). A longer chain: a distribution with coefficient of variation 5%, variance 4 and skewness 0.5 has SD = 2, so the mean is 2 ÷ 0.05 = 40, and then 0.5 = (40 − mode) ÷ 2 gives a mode of 39 (JNU 2021).
The quartiles give a measure that ignores the extreme tails altogether. In a symmetrical distribution the median sits exactly halfway between Q1 and Q3. In a right-skewed one it sits closer to Q1. Bowley’s coefficient measures how far off-centre it is:
For the Ashanagar incomes Q1 = ₹20,000, the median ₹25,000 and Q3 = ₹38,375. The median is only 5,000 above Q1 and 13,375 below Q3, so Bowley’s coefficient is (38,375 + 20,000 − 50,000) ÷ 18,375 = 0.46.
Both of those are shortcuts. The statistician’s own measure uses central moments, the average of the deviations from the mean raised to a power:
Older books give β1 = m3² ÷ m2³ as the measure of skewness. It is just γ1 squared, so it loses the sign, and the sign has to be taken from m3 separately. Here is a worked example small enough to do by hand.
The three coefficients live on different scales, so only the sign and the rough size are comparable between them. For the Ashanagar incomes Pearson gives 0.85, Bowley 0.46 and the moment coefficient 0.88: all positive, all agreeing on a right skew. Bowley looks smaller because it uses only the middle half of the data and ignores the tail where the skew lives.
Take the fourth power of the deviations and a value far from the mean counts enormously: twice as far out counts sixteen times as much. The fourth moment is therefore a measure of how much of the spread comes from the extreme values in the tails. Divided by the standard deviation to the fourth, it gives the coefficient of kurtosis, β2. For the normal curve it equals 3, and that value is the yardstick:
| Name | β₂ | Excess γ₂ = β₂ − 3 | Shape compared with the normal |
|---|---|---|---|
| Leptokurtic | > 3 | positive | higher peak, heavier tails |
| Mesokurtic | = 3 | zero | the normal curve itself |
| Platykurtic | < 3 | negative | flatter top, lighter tails |
The test is the same however it is written: β2 < 3 or γ2 < 0 means platykurtic (UGC NET 2025), and kurtosis defined as m4 ÷ σ4 − 3 is positive for a leptokurtic distribution (JAM 2026). If you are given the moments directly, just divide: with a fourth moment of 16 and a variance of 2, β2 = 16 ÷ 2² = 4 (CUET 2023).
The picture below shows three symmetric curves that have exactly the same mean and standard deviation. Everything that differs between them is kurtosis. Select one to highlight it and compare the share of the distribution lying more than two standard deviations from the mean.
| Shape | β₂ | Excess β₂ − 3 | Peak height | Share beyond ±2 SD |
|---|---|---|---|---|
| Platykurtic (uniform) | 1.8 | −1.2 | 0.289 | 0% |
| Mesokurtic (normal) | 3 | 0 | 0.399 | 4.55% |
| Leptokurtic (Laplace) | 6 | +3 | 0.707 | 5.91% |
All three have mean 0 and standard deviation 1, so mean and variance cannot tell them apart. The Laplace has the tallest peak and the most mass beyond two standard deviations: weight moved out of the shoulders into the centre and the tails. The uniform has no tail at all past 1.73 SD.
Two points to hold on to. First, kurtosis is mostly about the tails. “Peakedness” is the usual one-word summary, but the number is driven by how far the rare extreme values go. Second, skewness and kurtosis are separate properties: a distribution can be skewed without unusual tails, or have heavy tails and still be symmetrical, so the two can exist individually (Hyderabad 2016).
The quickest picture of a distribution’s shape is the box plot, built from the five-number summary: the minimum, Q1, the median, Q3 and the maximum. The box runs from Q1 to Q3 with a line at the median, so it holds the middle half of the data. Whiskers run out from it toward the extremes.
Whiskers stop short of values that are unusually far out. The standard rule is Tukey’s fences: any value more than 1.5 × IQR beyond a quartile is flagged as an outlier and drawn as a separate point, and the whisker ends at the most extreme value still inside the fences.
For Ashanagar, Q1 = 20,000, Q3 = 38,375 and the IQR is 18,375, so the upper fence is 38,375 + 27,562.5 = ₹65,937.50. Exactly one household, the one on ₹72,000, lies beyond it; the next highest, ₹58,500, is inside. The lower fence is negative, so nothing can fall below it.
The slider below changes only that richest household’s income. Watch which summaries respond. The median and the interquartile range cannot, because they depend on position, not size. The mean and the standard deviation follow the household wherever it goes.
The upper fence is Q3 + 1.5 × IQR = 38,375 + 1.5 × 18,375 = ₹65,938. ₹72,000 lies beyond it, so the household is drawn as an outlier.
The box also shows skew. In a symmetrical distribution the median is in the middle of the box and the two whiskers are about equal. If the median is close to Q1 and the upper half of the box and the upper whisker are much longer, the distribution is right-skewed. A boxplot with the median near the first quartile and a much wider upper half is exactly that picture, and the answer in DSE 2016 is right-skewed. Bowley’s coefficient is this same comparison, written as a number.
One caution on quartiles: this lesson uses the (n + 1)p rule, which puts Q1 at the (n + 1) ÷ 4-th value. Spreadsheets and statistics packages offer several other rules and can differ in the last digit on a small sample. For the sixty incomes this rule gives Q3 = ₹38,375, while the spreadsheet function QUARTILE.INC gives ₹38,125. If an exam names a rule, use that one.
| Measure | Formula | Range | Needs | Best used when |
|---|---|---|---|---|
| Pearson, first | (x̄ − mode) ÷ σ | no fixed limit | a clear single mode | The mode is well defined |
| Pearson, second | 3(x̄ − median) ÷ σ | within ±3 | mean, median, SD | Moderately skewed data, no clear mode |
| Bowley | (Q₃ + Q₁ − 2M) ÷ (Q₃ − Q₁) | −1 to +1 | the quartiles | Open-ended classes, extreme values |
| Moment | m₃ ÷ σ³ | unbounded | every value | Theory, and a precise number from full data |
Definitions, one-step arithmetic and which-measure questions. Most CUET and Hyderabad questions sit here.
Grouped data, combined means, effects of shifting and scaling, and statement questions, up to JNU level.
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