The dragging of inertial frames by an orbiting object implies that the horizon angular velocity of a central black hole in a composed black-hole-orbiting-ring system is no longer related to its angular-momentum by the familiar vacuum functional relation (here are respectively the mass and normalized area of the central spinning black hole). Using a continuity argument, it has recently been revealed that the composed Kerr-ring system is characterized by the universal (that is, spin-{\it independent}) relation , where are respectively the radius of the ring and its orbital angular momentum and is the horizon radius of the central Kerr black hole. This intriguing observation naturally raises the following physically interesting question: Does the physical quantity in a composed black-hole-orbiting-ring system is always characterized by the near-horizon functional relation which is independent of the spin (angular momentum) of the central black hole? In the present compact paper we explore the physical phenomenon of dragging of inertial frames by an orbiting ring in the composed Kerr-Newman-black-hole-orbiting-ring system. In particular, using analytical techniques, we reveal the fact that in this composed two-body (black-hole-ring) system the quantity has an explicit non-trivial functional dependence on the angular momentum of the central spinning black hole.

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