Summary: We investigate the motion of a magnetized particle orbiting around a black hole in braneworld immersed in asymptotically uniform magnetic field. The influence of brane parameter on effective potential of the radial motion of magnetized spinning particle around the braneworld black hole using Hamilton-Jacobi formalism is studied. It is found that circular orbits for photons and slowly moving particles may become stable near \(r = 3M\). It was argued that the radii of the innermost stable circular orbits are sensitive on the change of brane parameter. Similar discussion without Weil parameter has been considered by F. de Felice et al. [Classical Quantum Gravity 20, No. 3, 469–489 (2003; Zbl 1025.83015); Classical Quantum Gravity 21, No. 4, 961–973 (2004; Zbl 1052.83028)].