  In this paper, we present a rotating de Rham-Gabadadze-Tolley black hole with
a positive cosmological constant in massive gravity, achieved by applying a
modified Newman-Janis algorithm. The black hole exhibits stable orbits of
constant radii, prompting a numerical study on the behavior of the solutions to
a nonic equation governing the radii of planar orbits around the black hole.
Additionally, we investigate the stability of orbits near the event horizon and
provide a comprehensive analytical examination of the solutions to the angular
equations of motion. This is followed by simulating some spherical particle
orbits around the black hole.
