# Skewness

{{ safesubst:#invoke:Unsubst||$N=Use dmy dates |date=__DATE__ |$B= }} Example distribution with non-zero (positive) skewness. This data is from experiments on wheat grass growth.

In probability theory and statistics, skewness is a measure of the asymmetry of the probability distribution of a real-valued random variable about its mean. The skewness value can be positive or negative, or even undefined.

The qualitative interpretation of the skew is complicated. For a unimodal distribution, negative skew indicates that the tail on the left side of the probability density function is longer or fatter than the right side – it does not distinguish these shapes. Conversely, positive skew indicates that the tail on the right side is longer or fatter than the left side. In cases where one tail is long but the other tail is fat, skewness does not obey a simple rule. For example, a zero value indicates that the tails on both sides of the mean balance out, which is the case both for a symmetric distribution, and for asymmetric distributions where the asymmetries even out, such as one tail being long but thin, and the other being short but fat. Further, in multimodal distributions and discrete distributions, skewness is also difficult to interpret. Importantly, the skewness does not determine the relationship of mean and median.

## Introduction

Consider the two distributions in the figure just below. Within each graph, the bars on the right side of the distribution taper differently than the bars on the left side. These tapering sides are called tails, and they provide a visual means for determining which of the two kinds of skewness a distribution has:

1. Template:Visible anchor: The left tail is longer; the mass of the distribution is concentrated on the right of the figure. The distribution is said to be left-skewed, left-tailed, or skewed to the left.
2. Template:Visible anchor: The right tail is longer; the mass of the distribution is concentrated on the left of the figure. The distribution is said to be right-skewed, right-tailed, or skewed to the right.

Skewness in a data series may be observed not only graphically but by simple inspection of the values. For instance, consider the numeric sequence (49, 50, 51), whose values are evenly distributed around a central value of (50). We can transform this sequence into a negatively skewed distribution by adding a value far below the mean, as in e.g. (40, 49, 50, 51). Similarly, we can make the sequence positively skewed by adding a value far above the mean, as in e.g. (49, 50, 51, 60).

## Relationship of mean and median

The skewness is not strictly connected with the relationship between the mean and median: a distribution with negative skew can have the mean greater than or less than the median, and likewise for positive skew.

In the older notion of nonparametric skew, defined as $(\mu -\nu )/\sigma ,$ where µ is the mean, ν is the median, and σ is the standard deviation, the skewness is defined in terms of this relationship: positive/right nonparametric skew means the mean is greater than (to the right of) the median, while negative/left nonparametric skew means the mean is less than (to the left of) the median. However, the modern definition of skewness and the traditional nonparametric definition do not in general have the same sign: while they agree for some families of distributions, they differ in general, and conflating them is misleading.

If the distribution is symmetric then the mean is equal to the median and the distribution will have zero skewness. If, in addition, the distribution is unimodal, then the mean = median = mode. This is the case of a coin toss or the series 1,2,3,4,... Note, however, that the converse is not true in general, i.e. zero skewness does not imply that the mean is equal to the median.

"Many textbooks," a 2005 article points out, "teach a rule of thumb stating that the mean is right of the median under right skew, and left of the median under left skew. This rule fails with surprising frequency. It can fail in multimodal distributions, or in distributions where one tail is long but the other is heavy. Most commonly, though, the rule fails in discrete distributions where the areas to the left and right of the median are not equal.Template:Clarify Such distributions not only contradict the textbook relationship between mean, median, and skew, they also contradict the textbook interpretation of the median."

## Definition

### Pearson's moment coefficient of skewness

The skewness of a random variable X is the moment coefficient of skewness. It is sometimes referred to as Pearson's moment coefficient of skewness, not to be confused with Pearson's other skewness statistics (see below). It is the third standardized moment. It is denoted γ1 and defined as

$\gamma _{1}=\operatorname {E} {\Big [}{\big (}{\tfrac {X-\mu }{\sigma }}{\big )}^{\!3}\,{\Big ]}={\frac {\mu _{3}}{\sigma ^{3}}}={\frac {\operatorname {E} {\big [}(X-\mu )^{3}{\big ]}}{\ \ \ (\operatorname {E} {\big [}(X-\mu )^{2}{\big ]})^{3/2}}}={\frac {\kappa _{3}}{\kappa _{2}^{3/2}}}\ ,$ where μ3 is the third central moment, μ is the mean, σ is the standard deviation, and E is the expectation operator. The last equality expresses skewness in terms of the ratio of the third cumulant κ3 and the 1.5th power of the second cumulant κ2. This is analogous to the definition of kurtosis as the fourth cumulant normalized by the square of the second cumulant.

The skewness is also sometimes denoted Skew[X].

The formula expressing skewness in terms of the non-central moment E[X3] can be expressed by expanding the previous formula,

{\begin{aligned}\gamma _{1}&=\operatorname {E} {\bigg [}{\Big (}{\frac {X-\mu }{\sigma }}{\Big )}^{\!3}\,{\bigg ]}\\&={\frac {\operatorname {E} [X^{3}]-3\mu \operatorname {E} [X^{2}]+3\mu ^{2}\operatorname {E} [X]-\mu ^{3}}{\sigma ^{3}}}\\&={\frac {\operatorname {E} [X^{3}]-3\mu (\operatorname {E} [X^{2}]-\mu \operatorname {E} [X])-\mu ^{3}}{\sigma ^{3}}}\\&={\frac {\operatorname {E} [X^{3}]-3\mu \sigma ^{2}-\mu ^{3}}{\sigma ^{3}}}\ .\end{aligned}} ### Properties

Skewness can be infinite, as when

$\Pr \left[X>x\right]=x^{-3}{\mbox{ for }}x>1,\ \Pr[X<1]=0$ or undefined, as when

$\Pr[Xx]=(1+x)^{-3}/2{\mbox{ for positive }}x.$ In this latter example, the third cumulant is undefined. One can also have distributions such as

$\Pr \left[X>x\right]=x^{-2}{\mbox{ for }}x>1,\ \Pr[X<1]=0$ where both the second and third cumulants are infinite, so the skewness is again undefined.

If Y is the sum of n independent and identically distributed random variables, all with the distribution of X, then the third cumulant of Y is n times that of X and the second cumulant of Y is n times that of X, so ${\mbox{Skew}}[Y]={\mbox{Skew}}[X]/{\sqrt {n}}$ . This shows that the skewness of the sum is smaller, as it approaches a Gaussian distribution in accordance with the central limit theorem.

### Sample skewness

For a sample of n values, a natural method of moments estimator of the population skewness is

$b_{1}={\frac {m_{3}}{s^{3}}}={\frac {{\tfrac {1}{n}}\sum _{i=1}^{n}(x_{i}-{\overline {x}})^{3}}{\left[{\tfrac {1}{n-1}}\sum _{i=1}^{n}(x_{i}-{\overline {x}})^{2}\right]^{3/2}}}\ ,$ where ${\overline {x}}$ is the sample mean, s is the sample standard deviation, and the numerator m3 is the sample third central moment.

Another common definition of the sample skewness is

$G_{1}={\frac {k_{3}}{k_{2}^{3/2}}}={\frac {n^{2}}{(n-1)(n-2)}}\;{\frac {m_{3}}{s^{3}}},$ where $k_{3}$ is the unique symmetric unbiased estimator of the third cumulant and $k_{2}=s^{2}$ is the symmetric unbiased estimator of the second cumulant (i.e. the variance).

In general, the ratios $b_{1}$ and $G_{1}$ are both biased estimators of the population skewness $\gamma _{1}$ ; their expected values can even have the opposite sign from the true skewness. (For instance a mixed distribution consisting of very thin Gaussians centred at −99, 0.5, and 2 with weights 0.01, 0.66, and 0.33 has a skewness of about −9.77, but in a sample of 3, $G_{1}$ has an expected value of about 0.32, since usually all three samples are in the positive-valued part of the distribution, which is skewed the other way.) Nevertheless, $b_{1}$ and $G_{1}$ each have obviously the correct expected value of zero for any symmetric distribution with a finite third moment, including a normal distribution.

The variance of the skewness of a random sample of size n from a normal distribution is

$\operatorname {var} (G_{1})={\frac {6n(n-1)}{(n-2)(n+1)(n+3)}}.$ An approximate alternative is 6/n but this is inaccurate for small samples.

In normal samples, $b_{1}$ has the smaller variance of the two estimators, with

$\operatorname {var} (b_{1})<\operatorname {var} \left({\frac {m_{3}}{m_{2}^{3/2}}}\right)<\operatorname {var} (G_{1}),$ where m2 in the denominator is the (biased) sample second central moment.

The adjusted Fisher-Pearson standardized moment coefficient $G_{1}$ is the version found in Excel and several statistical packages including Minitab, SAS and SPSS.

## Applications

Skewness has benefits in many areas. Many models assume normal distribution; i.e., data are symmetric about the mean. The normal distribution has a skewness of zero. But in reality, data points may not be perfectly symmetric. So, an understanding of the skewness of the dataset indicates whether deviations from the mean are going to be positive or negative.

D'Agostino's K-squared test is a goodness-of-fit normality test based on sample skewness and sample kurtosis.

## Other measures of skewness

Other measures of skewness have been used, including simpler calculations suggested by Karl Pearson (not to be confused with Pearson's moment coefficient of skewness, see above). These other measures are:

### Pearson mode skewness

The Pearson mode skewness is defined by

### Pearson's first skewness coefficient

The Pearson's first skewness coefficient is defined by

### Pearson's second skewness coefficient

The Pearson's median or Pearson's second skewness coefficient is defined by

The latter is a simple multiple of the nonparametric skew.

### Other

Starting from a standard cumulant expansion around a Normal distribution, one can actually show that skewness = 6 (meanmedian) / standard deviation ( 1 + kurtosis / 8) + O(skewness2).{{ safesubst:#invoke:Unsubst||date=__DATE__ |$B= {{#invoke:Category handler|main}}{{#invoke:Category handler|main}}[citation needed] }} One should keep in mind that above given equalities often don't hold even approximately and these empirical formulas are abandoned nowadays.{{ safesubst:#invoke:Unsubst||date=__DATE__ |$B= {{#invoke:Category handler|main}}{{#invoke:Category handler|main}}[citation needed] }} There is no guarantee that these will be the same sign as each other or as the ordinary definition of skewness.

### Quantile based measures

A skewness function

$\gamma (u)={\frac {F^{-1}(u)+F^{-1}(1-u)-2F^{-1}(1/2)}{F^{-1}(u)-F^{-1}(1-u)}}$ can be defined, where F is the cumulative distribution function. This leads to a corresponding overall measure of skewness defined as the supremum of this over the range 1/2 ≤ u < 1. Another measure can be obtained by integrating the numerator and denominator of this expression. The function γ(u) satisfies -1 ≤ γ(u) ≤ 1 and is well defined without requiring the existence of any moments of the distribution.

Galton's measure of skewness is γ(u) evaluated at u = 3 / 4. Other names for this same quantity are the Bowley Skewness, the Yule-Kendall index and the quartile skewness.

Kelley's measure of skewness uses u = 0.1.{{ safesubst:#invoke:Unsubst||date=__DATE__ |\$B= {{#invoke:Category handler|main}}{{#invoke:Category handler|main}}[citation needed] }}

### L-moments

Use of L-moments in place of moments provides a measure of skewness known as the L-skewness.

### Distance skewness

A value of skewness equal to zero does not imply that the probability distribution is symmetric. Thus there is a need for another measure of asymmetry which has this property: such a measure was introduced in 2000. It is called distance skewness and denoted by dSkew. If X is a random variable which takes values in the d-dimensional Euclidean space, X has finite expectation, X' is an independent identically distributed copy of X and $\|\cdot \|$ denotes the norm in the Euclidean space then a simple measure of asymmetry is

dSkew (X) := 1 - E||X-X'|| / E||X + X'|| if X is not 0 with probability one,

and dSkew (X):= 0 for X = 0 (with probability 1). Distance skewness is always between 0 and 1, equals 0 if and only if X is diagonally symmetric (X and -X has the same probability distribution) and equals 1 if and only if X is a nonzero constant with probability one. Thus there is a simple consistent statistical test of diagonal symmetry based on the sample distance skewness:

dSkewn(X):= 1- ∑i,j ||xi – xj|| / ∑i,j||xi + xj||.

### Groeneveld & Meeden’s coefficient

Groeneveld & Meeden have suggested, as an alternative measure of skewness,

$\mathrm {skew} (X)={\frac {(\mu -\nu )}{E(|X-\nu |)}}$ where μ is the mean, ν is the median, |…| is the absolute value and E() is the expectation operator.