  The measurement of the epicyclic frequencies is a widely used astrophysical
technique to infer information on a given self-gravitating system and on the
related gravity background. We derive their explicit expressions in static and
spherically symmetric wormhole spacetimes. We discuss how these theoretical
results can be applied to: (1) detect the presence of a wormhole,
distinguishing it by a black hole; (2) reconstruct wormhole solutions through
the fit of the observational data, once we have them. Finally, we discuss the
physical implications of our proposed epicyclic method.
