A laser flash photolysis–resonance fluorescence technique has been employed to study the kinetics of the reaction of chlorine atoms with methyl bromide as a function of temperature (161–697 K) and pressure (20–250 Torr) in nitrogen buffer gas. At T≥213 K, where information available in the literature suggests that hydrogen transfer is the dominant reaction pathway, observed rate coefficients are pressure independent and the following modified Arrhenius expression adequately describes all kinetic data obtained: k 1a=1.02×10 −15 T 1.42 exp(−605/ T) cm 3 molecule −1 s −1. At temperatures in the range 161–177 K, reversible addition of Cl( 2P J ) to CH 3Br is observed, thus allowing rate coefficients and equilibrium constants for CH 3BrCl formation and dissociation to be determined. Second- and third-law analyses of the equilibrium data lead to the following thermochemical parameters for the association reaction (1d): Δ H 298 o=−25.6±2.3 kJ mol −1, Δ H 0 o=−24.0±2.9 kJ mol −1, Δ S 298 K o=−72.3±11.8 J K −1 mol −1. In conjunction with the well-known heats of formation of Cl( 2P J ) and CH 3Br, the above Δ H values lead to the following heats of formation for CH 3BrCl at 298 and 0 K: Δ H f, 298 o=57.6±2.4 kJ mol −1 and Δ H f, 0 o=72.9±3.0 kJ mol −1. Ab initio calculations using density functional theory and G2 theory reproduce the experimental bond strength reasonably well. The DFT calculations predict a CH 3BrCl structure (used in the third-law analysis) where the C–Br–Cl bond angle is 90° and the methyl group adopts a staggered orientation with a pronounced tilt toward chlorine. Ab-initio calculations are also reported which examine the structures and energetics of adducts formed from addition of F atoms and OH radicals to CH 3Br. Structures of CH 3BrF and CH 3BrOH are similar to that of CH 3BrCl, with the F-adduct being the most strongly bound and the OH-adduct being the least strongly bound. Bonding in CH 3Br–X (X=F, Cl, OH) is discussed as are the implications of the new experimental and theoretical results for atmospheric chemistry.