MONODEUTERATED methane (CHxD) has been discovered recently in the atmosphere of Jupiter by an identification”’ of the lines P(2) through P(12) in its vibration-rotation band at 2200 cm-‘. A quantitative interpretation”’ of the observed spectrum”’ that could lead to an estimate of the abundance of CH,D and of the D/H ratio in the atmosphere of Jupiter requires intensity data at the relevant planetary temperatures for this band. Therefore, we have measured in our laboratory the intensities of J-multiplets between P(12) and R(4) and of the fully blended Q-branch, at lOO”K, lSO”K, 200”K, 250°K and 298°K. EXPERIMENTAL PROCEDURE The experimental apparatus is essentially the same as discussed in Ref. (3) for the 2vX-band of methane. The different spectral region considered in the present paper required the use of an infrared glower, 144 l/mm grating and an InSb detector with which we were able to obtain a spectral resolution ranging between 0.15 cm-’ and 0.2 cm-’ and a signal-to-noise ratio of 200 : 1. The time constant of the lock-in-amplifier was set at 100msec. Several mixtures, with the amount of CH,D in Hz ranging from 0.117 to 4 per cent (by volume), were prepared. The gases were allowed to mix for at least a couple of days in lecture bottles before the mixture was introduced into the absorption cells. The sample of CH,D was supplied by the isotope division of Merck, Sharp and Dohme Canada, Limited, with the following batch analysis: 97.46% of CH,D and 2.54% of CH, with no detectable trace of CH2Dz according to mass analysis by the supplier. With the spectral resolution available to us, it has not been possible to measure the intensities of the individual lines (K-components) of each J-multiplet. The procedure we have adapted for deriving multiplet-intensities, S, (cm-’ atm-‘), from measured equivalent widths is quite similar to that described in our paper”’ on the 2v3-band of methane. Construction of curves-of-growth for blended .I-multiplets required (i) the assumption of theoretical formulae@’ for the relative line strengths, SJK (cm-’ atm-I), of individual lines of a J-multiplet, and (ii) the assumption that all of the lines in the band have the same hydrogen-broadened half-width, Y&,+~~ = (3OO/T)“‘O.O75 cm-’ atm-‘, as the rotational lines in the v3 band of methane.“” On theoretical