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The so-called "global polytropic model" is applied to the numerical study ofthe exoplanet systems HD 10180, Kepler-32, Kepler-33, Kepler-102, andKepler-186. We compare computed distances of planets from their host stars withcorresponding observations and discuss some further orbit predictions made bythe model.

Gravitational quantization of exoplanet orbits in HD 10180, Kepler-32, Kepler-33, Kepler-102, and Kepler-186