The structure of the near infra-red bands of methane I-General survey, and a new band at 11,050 a
Methane is the most important of the relatively few polyatomic molecules which may be expected to give rise to spectra suitable for investigation in that portion of the near infra-red which is as yet available to photography. To the chemist it is simplest organic molecule, whilst to Ike theoretical physicist the four directed valencies and their symmetry properties are its most interesting features, From a technical point of view its importance lies in Ike fact that its low moment of inertia gives to the bank structure a coarseness which brings it within reach of the diffraction grating. The amount of information which we possess of the spectrum is already fairly considerable. The first to make a resolution of the fine structure was Cooley, who investigated the bands at 7·7 μ and 3·3 μ and the measurements have since been extended, with the usual type of thermojunction infra-red spectrometer, by Ellis, Moorhead, and Norris and Unger. In the photographic infra-red, measurements at wave-lengths shorter than 1 μ have been made by Dennison and Ingram, and Vedder and Mecke. The present series of papers presents measurements made by the writer in the region λ10,000-12,000 A. They thus overlap into part of the region covered by Norris and Unger and include the bands found by them at λ 11,350, λ 11,620, and λ 11,870. The resolving power of the grating is of course far higher than that employed by them, and muck new detail not shown in their curves is now revealed for the first time. The regularities which they abstract from their measurements prove to be spurious, the result merely of the smoothing out of a many-lined spectrum by the use of too low a resolving power.