Approximation error

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One commonly distinguishes between the relative error and the absolute error. The absolute error is the magnitude of the difference between the exact value and the approximation. The relative error is the absolute error divided by the magnitude of the exact value. The percent error is the relative error expressed in terms of per 100.

As an example, if the exact value is 50 and the approximation is 49.9, then the absolute error is 0.1 and the relative error is 0.1/50 = 0.002. The percent error would then be 0.002 × 100 = 0.2%. Another example would be if you measured a beaker and read 5mL. The correct reading would have been 6mL. This means that your percent error would be 16.67%.

The relative error is often used to compare approximations of numbers of widely differing size; for example, approximating the number 1,000 with an absolute error of 3 is, in most applications, much worse than approximating the number 1,000,000 with an absolute error of 3; in the first case the relative error is 0.003 and in the second it is only 0.000003.

There are two features of relative error that should be kept in mind. Firstly, relative error is undefined when the true value is zero as it appears in the denominator (see below). Secondly, relative error only makes sense when measured on a ratio scale, (i.e. a scale which has a true meaningful zero), otherwise it would be sensitive to the measurement units . For example, when an absolute error in a temperature measurement given in Celsius is 1° and the true value is 2°C, the relative error is 0.5 and the percent error is 50%. For this same case, when the temperature is given in Kelvin, the same 1° absolute error with the same true value of 275.15° K gives a relative error of 3.63e-3 and a percent error of only 0.363%. Celsius temperature is measured on an interval scale, whereas the Kelvin scale has a true zero and so is a ratio scale.


Given some value v and its approximation vapprox, the absolute error is

\epsilon = |v-v_\text{approx}|\ ,

where the vertical bars denote the absolute value. If v \ne 0, the relative error is

 \eta = \frac{\epsilon}{|v|}
    = \left| \frac{v-v_\text{approx}}{v} \right|
    = \left| 1 - \frac{v_\text{approx}}{v} \right|,

and the percent error is

\delta = 100\times\eta = 100\times\frac{\epsilon}{|v|} = 100\times\left| \frac{v-v_\text{approx}}{v} \right|.

These definitions can be extended to the case when v and v_{\text{approx}} are n-dimensional vectors, by replacing the absolute value with an n-norm.[1]


In most indicating instruments, the accuracy is guaranteed to a certain percentage of full-scale reading. The limits of these deviations from the specified values are known as limiting errors or guarantee errors.[2]

See also[edit]


  1. ^ Golub, Gene; Charles F. Van Loan (1996). Matrix Computations – Third Edition. Baltimore: The Johns Hopkins University Press. p. 53. ISBN 0-8018-5413-X. 
  2. ^ Albert D. Helfrick, Modern Electronic Instrumentation and Measurement Techniques, pg16, ISBN 81-297-0731-4

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