A star can turn into a black hole when it collapses, with some mass being expelled during a nova event, while the remaining mass may form the black hole if it is sufficiently large. Black holes have a mass that is equal to or less than the original star, and from a distance, they behave similarly to stars or planets. The gravitational effects of a black hole become significant only when one approaches it closely, due to the inverse square law of gravity. Mass loss occurs during black hole formation, with energy being released as electromagnetic radiation and gravitational waves, maintaining the total mass-energy balance. Ultimately, the concept of conservation of mass can be understood through the lens of mass-energy equivalence, as mass can be transformed into energy.