A supernova occurs when a massive star undergoes gravitational collapse, leading to a sudden and dramatic explosion.

Depending on the mass of the progenitor star, a supernova can result in the formation of a black hole or a neutron star.

Type II supernovae are associated with the death of massive stars with masses greater than 8 solar masses.

The energy released in a supernova primarily comes from the gravitational potential energy of the collapsing core.

Stars with masses similar to our Sun have a lifespan of approximately 10 billion years.

During the Red Giant Phase, a star sheds its outer layers, creating a planetary nebula.

Population III Stars are believed to be the first stars formed in the universe.

Peak Luminosity refers to the maximum brightness reached by a supernova during its outburst.

Hydrogen is the primary element responsible for the characteristic colors observed in a supernova.

Supernova Remnant refers to the expanding shell of material ejected during a supernova.

Type Ia supernovae are associated with the death of white dwarf stars.

Stars with masses in the range of 8-15 solar masses typically undergo a Type II supernova.

Nuclear Fusion is the process by which a star converts hydrogen into helium.

Type III supernovae are associated with the death of massive stars with masses greater than 25 solar masses.

Mass Loss refers to the process by which a star gradually loses mass through stellar winds.