Calculating the rotation speed of a black hole is challenging due to the inability to observe phenomena inside the event horizon. Theoretical models, such as those involving Kerr black holes, suggest that rotation is linked to conservation of angular momentum. Some theories propose using light emitted from a black hole's surroundings, particularly in x-ray binaries, to estimate its spin. However, skepticism remains regarding the effectiveness of current methods to accurately derive a black hole's intrinsic spin. Overall, while there are promising approaches, definitive measurements of black hole rotation speed remain elusive.