The first four raw moments of distribution are 2, 136, 320, and 40,000, The coefficient of skewness is:
To find the coefficient of skewness from raw moments, we first need to convert the raw moments into central moments. Central moments are moments about the mean, and they are directly used in formulas for measures like skewness and kurtosis.
Raw moments (denoted by \( \mu'_k \)) are moments taken about the origin (zero). The first raw moment \( \mu'_1 \) is the mean of the distribution.
Central moments (denoted by \( \mu_k \)) are moments taken about the mean. The first central moment \( \mu_1 \) is always zero. The second central moment \( \mu_2 \) is the variance. The third central moment \( \mu_3 \) is related to skewness, and the fourth central moment \( \mu_4 \) is related to kurtosis.
The first four raw moments of the distribution are given as:
We use the following formulas to convert raw moments to central moments:
Let's calculate the central moments:
So, the calculated central moments are \( \mu_2 = 132 \), \( \mu_3 = -480 \), and \( \mu_4 = 40656 \).
The coefficient of skewness based on moments is often represented by \( \beta_1 \) or \( \gamma_1 \). Karl Pearson's Beta coefficient of skewness is given by:
\[ \beta_1 = \dfrac{\mu_3^2}{\mu_2^3} \]This measure indicates the degree of asymmetry of the distribution. A value of 0 indicates symmetry, a positive value indicates positive skew (tail to the right), and a negative value is not possible for \( \beta_1 \) because \( \mu_3 \) is squared.
Karl Pearson's Gamma coefficient of skewness is given by \( \gamma_1 = \sqrt{\beta_1} = \dfrac{\mu_3}{(\sqrt{\mu_2})^3} = \dfrac{\mu_3}{\mu_2^{3/2}} \). This measure retains the sign of \( \mu_3 \) and thus indicates the direction of skewness.
Looking at the options provided, they are in the form of \( \mu_3^2 / \mu_2^3 \) or similar structure, suggesting we should calculate \( \beta_1 \).
Using our calculated central moments \( \mu_2 = 132 \) and \( \mu_3 = -480 \):
\[ \beta_1 = \dfrac{(-480)^2}{(132)^3} \]Let's compare our result with the given options:
| Option | Expression | Matches Calculation? |
|---|---|---|
| 1 | \( \dfrac{40656}{(132)^2} \) | No (Uses \( \mu_4 \) and \( \mu_2^2 \)) |
| 2 | \( \dfrac{(40656)^2}{(132)^3} \) | No (Uses \( \mu_4^2 \) and \( \mu_2^3 \)) |
| 3 | \( \dfrac{-480}{(132)^2} \) | No (Uses \( \mu_3 \) and \( \mu_2^2 \)) |
| 4 | \( \dfrac{(-480)^2}{(132)^3} \) | Yes (Matches \( \mu_3^2 / \mu_2^3 \)) |
Our calculated value for the coefficient of skewness \( \beta_1 \) is \( \dfrac{(-480)^2}{(132)^3} \), which matches Option 4.
| Concept | Notation | Definition/Formula (Central Moments from Raw) |
|---|---|---|
| First Raw Moment (Mean) | \( \mu'_1 \) | Given |
| Second Raw Moment | \( \mu'_2 \) | Given |
| Third Raw Moment | \( \mu'_3 \) | Given |
| Fourth Raw Moment | \( \mu'_4 \) | Given |
| First Central Moment | \( \mu_1 \) | \( 0 \) |
| Second Central Moment (Variance) | \( \mu_2 \) | \( \mu'_2 - (\mu'_1)^2 \) |
| Third Central Moment | \( \mu_3 \) | \( \mu'_3 - 3\mu'_2\mu'_1 + 2(\mu'_1)^3 \) |
| Fourth Central Moment | \( \mu_4 \) | \( \mu'_4 - 4\mu'_3\mu'_1 + 6\mu'_2(\mu'_1)^2 - 3(\mu'_1)^4 \) |
| Beta Coefficient of Skewness | \( \beta_1 \) | \( \dfrac{\mu_3^2}{\mu_2^3} \) |
| Gamma Coefficient of Skewness | \( \gamma_1 \) | \( \dfrac{\mu_3}{\sqrt{\mu_2^3}} \) |
Skewness is a measure of the asymmetry in a probability distribution. A distribution is symmetric if it looks the same on both sides of the mean. If the distribution is skewed, the data is spread out more on one side of the mean than the other.
Moments are fundamental descriptive statistics used to characterize the shape and properties of a distribution. Raw moments and central moments are commonly used, but moments about any arbitrary point can also be calculated.
The third central moment \( \mu_3 \) directly measures the asymmetry. If \( \mu_3 > 0 \), the distribution is positively skewed. If \( \mu_3 < 0 \), it's negatively skewed. If \( \mu_3 = 0 \), it's symmetric.
The coefficient \( \beta_1 = \mu_3^2 / \mu_2^3 \) is a pure number, independent of the units of the variable, making it useful for comparing the degree of skewness across different distributions. Its square root, \( \gamma_1 \), is also unit-free and its sign matches the sign of \( \mu_3 \).
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