White dwarfs form when stars like our Sun exhaust their nuclear fuel and shed their outer layers, leaving behind a dense core. According to Newton's third law, the force that expels the outer layers also applies an equal and opposite force inward, causing the core to compress. In some cases, the core becomes extremely dense, forming a white dwarf. These stars can rotate rapidly due to the conservation of angular momentum. Consider a white dwarf with a mass equal to the Sun and a radius of 5.0 × 10³ km. How many revolutions per minute(rpm) would a satellite make if it were orbiting 5.0 × 10² km above the surface?[Mass of sun = 2.0 × 10³⁰ kg]