**Scientific notation** (**standard index notation**) is a concise way of recording numbers by integer powers of ten, that is used to record numbers which are notably large or small. Such notation is used to record physical quantities without including trailing, or leading, zeros.

- 10
^{1}= 10 - 10
^{2}= 100 - 10
^{3}= 1000 - 10
^{6}= 1,000,000 - 10
^{9}= 1,000,000,000 - 10
^{20}= 100,000,000,000,000,000,000

*-n*is equal to 1/10

^{n}or, equivalently 0.

*(n-1 zeros)*1:

- 10
^{-1}= 1/10 = 0.1 - 10
^{-3}= 1/1000 = 0.001 - 10
^{-9}= 1/1,000,000,000 = 0.000000001

^{29}, and a small number such as 0.0000000000234 can be written as 2.34 × 10

^{-11}. For example, the distance to the edge of the observable universe is ~4.6 × 10

^{26}m and the mass of a proton is ~1.67 x 10

^{-27}kg. Most calculators and many computer programs present very large and very small results in scientific notation; the 10 is usually omitted and the letter E for exponent is used; for example: 1.56234 E29. Note that this is not related to the base of the natural logarithm also commonly denoted by

*e*.

Scientific notation is highly useful for quoting physical quantities, as they can only be measured to within certain error limits and so quoting just the digits that are certain (the "significant digits") gives all the information required without wasting space.

If a physical quantity is quoted using scientific notation, it is usually assumed to be accurate to the quoted number of digits of precision - for instance if a figure 1.2340 × 10^{6} metres is quoted, the actual figure is assumed to be between 1,233,950 metres as a lower bound and 1,234,050 metres as an upper bound. However, where precision in such measurements is crucial, much more sophisticated expressions of measurement error must be used.

See also: Orders of magnitude, floating point.