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I discuss a prospect for mode identification from two-passband photometry offorthcoming BRITE space mission. Examples of photometric diagnostic diagramsare shown for three types of main sequence pulsating variables: $\beta$ Cephei,Slowly Pulsating B-type and $\delta$ Scuti stars. I consider also taking intoaccount the radial velocity data from simultaneous spectroscopy, which can becarried out from the ground. With such observations, much better discriminationof the spherical harmonic degree, $\ell$, can be accomplished and moreconstraints on stellar parameters and input physics can be derived.

Identifying pulsation modes from two-passband photometry