This paper discusses some of the mechanisms whereby fast inertia-gravity waves can be generated spontaneously by slow, balanced atmospheric and oceanic flows. In the small-Rossby-number regime relevant to mid-latitude dynamics, high-accuracy balanced models, which filter out inertia-gravity waves completely, can in principle describe the evolution of suitably initialised flows up to terms that are exponentially small in the Rossby number , i.e, of the form exp(−α/ ) for some α > 0.This suggests that the mechanisms of inertia-gravity-wave generation, which are not captured by these balanced models, are also exponentially weak. This has been confirmed by explicit analytical results obtained for a few highly-simplified models. We review these results and present some of the exponential-asymptotic techniques that have been used in their derivation. We examine both spontaneous-generation mechanisms which generate exponentially small waves from perfectly balanced initial conditions, and unbalanced instability mechanisms which amplify unbalanced initial perturbations of steady flows. The relevance of the results to realistic flows is discussed.2