Spectral analysis

1859, 1860 Light and sky instrument

Chemical analysis by light: each element in a flame gives its own set of bright lines, and the same element as a gas absorbs the same lines.

In autumn 1859 the German physicist Gustav Kirchhoff used this to explain Fraunhofer's dark lines (1814) in the solar spectrum, and in 1860 he and the chemist Robert Bunsen published a method of chemical analysis by spectra.

The composition of matter could now be read from its light, including the Sun and the stars: caesium and rubidium were discovered this way in 1860 and 1861. The same work produced Kirchhoff's radiation law and the notion of the black body, whose spectrum forty years later led to the quantum.

Why this date

exact: Kirchhoff's communication on the Fraunhofer lines to the Berlin Academy in autumn 1859; joint paper by Kirchhoff and Bunsen, Chemische Analyse durch Spectralbeobachtungen, Annalen der Physik 1860; predecessor: Fraunhofer's dark lines 1814 (published 1817)

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