Construct · 1 fields · 4 citations
One name. One construct. A landmark on the map.
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Johannes Rydberg, working from spectral data he presented in 1888 and published in 1890, introduced the constant that now carries his name to express the wavelengths of the bright and dark lines in an element's light spectrum as one formula, generalizing the pattern Johann Balmer had found for hydrogen in 1885. The Rydberg constant, written R with the subscript infinity (R∞), is the fixed number that sets the scale of those spectral lines: in Rydberg's formula the reciprocal of a line's wavelength equals R∞ times the difference of two terms, each of which is one divided by the square of a whole number that labels an electron's energy level. Niels Bohr's 1913 model of the atom derived this constant from more basic quantities, the electron's mass and charge, Planck's constant, and the speed of light, turning an empirical fitting number into a predicted combination of other fundamental constants. Today R∞ is among the most precisely known physical constants, its value fixed by international agreement (the CODATA adjustment) to about a dozen significant figures, which is why the atomic spectra it governs serve as a benchmark test of physical theory. It ties together the observed colors of light emitted by atoms, the ladder of energy levels inside them, and the fundamental constants from which it is built, and it is kept distinct from the related terms Rydberg formula (the equation) and Rydberg atom (a highly excited atom).[1][2][3][4]
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