XIII. The absorption spectra of the vapours of benzene and its homolognes, at different temperatures and pressures, and of solutions of benzene
The absorption spectrum of benzene in a state of vapour and in solution was photographed by W. A. Miller (‘ Phil. Trans.,’ 1862, vol. 152, II., pp. 861-887). It was also photographed by me in 1880 (‘ J. Chem. Soc.,’ 1881, vol. 39, p. 153; 1882, vol. 41 ; 1885, vol. 47, pp. 685-757), with the instrument and by the method described in the ‘ Scientific Proceedings of the Royal Dublin Society ’ in 1881 (vol. iii., p. 93, New Series) and ‘ J. Society of Arts,’ 1885. For these investigations a molecular weight in milligrammes was employed to test the molecular absorption of the hydrocarbon, but the quantity of vapour was too large even at low temperatures, and the temperature, as since ascertained, was in other experiments too high to admit of the numerous absorption bands being observed, although a series of bands had been photographed from very dilute solutions of benzene in alcohol. The continuous rays which accompany the lines in the emission spectrum of the strongly condensed spark of cadmium were found to afford the best source of light in the region of short wavelengths. J. Pauer, in 1897 (‘ Wiedemann’s Annalen,’ vol. 61, p. 363), also used the cadmium spectrum precisely in the same manner for a more complete investigation of benzene and its homologues, but his experiments were not quantitative, although he compared the same substances in the states of vapour, of liquid, and in solution at a temperature of 20° C. He accurately measured 29 different narrow bands characteristic of the spectrum of the vapour of benzene. More recently this work has been repeated by Wilhelm Friederichs (‘ Zeitschrift f. Wissenschaftl. Photographie,’ 1905, vol. 3, p. 154) and by Leonard Grebe ( loc. cit ., 1905, p . 363).