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Dynamos operating in the interiors of rapidly rotating planets and low-massstars might belong to a similar category where rotation plays a vital role. Wequantify this similarity using scaling laws. We analyse direct numericalsimulations of Boussinesq and anelastic spherical shell dynamos. These dynamosrepresent simplified models which span from Earth-like planets to rapidlyrotating low-mass stars. We find that magnetic field and velocity in thesedynamos are related to the available buoyancy power via a simple power lawwhich holds over wide variety of control parameters.

Bridging planets and stars using scaling laws in anelastic spherical shell dynamos