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Gray models, which replace spectrally-resolved opacities with a wavelengthindependent mean opacity, are currently seeing wide and diverse application. Inthis brief review, we discuss both the history of gray techniques as well asrecent applications of gray models, with an emphasis on planetary atmospheres.Methods and results for generating mean opacities are summarized. We presentexamples where gray radiative transfer tools are incorporated intothree-dimensional atmospheric circulation models. Gray techniques are alsouseful for problems in comparative climatology, and we inter-compare resultsfrom several generalized gray models as applied to the computation ofconvective fluxes in planetary atmospheres. Finally, we provide examples wherefuture progress can be made in the development of gray models.

Completely Colorblind: Advances in Gray Techniques and Applications to Planets Near and Far