Limite de Chandrasekhar

The Chandrasekhar Limit calculator is a tool used to determine the maximum mass limit that a white dwarf star can have. This limit is fundamental in astrophysics, as it defines the point beyond which the star collapses into a black hole or a neutron star.

The Chandrasekhar Limit is calculated based on a formula that takes into account the star's mass in relation to the Sun's mass. This formula is simple yet crucial: approximately 1.4 solar masses. When a white dwarf star reaches or exceeds this mass, it can no longer support its own weight and undergoes a collapse.

The importance of the Chandrasekhar Limit lies in its ability to explain the behavior of stars at the end of their lives. It helps astronomers understand how stars evolve and what possible destinations they may have, whether as white dwarfs, neutron stars, or black holes.

Care should be taken when using this calculator, as the accuracy of the result directly depends on the accuracy of the input data. Additionally, it is important to remember that the Chandrasekhar Limit is a theoretical concept that applies to white dwarf stars composed mainly of carbon and oxygen.