In massive stars, the core collapses under its own gravity when it runs out of nuclear fuel, leading to a supernova.

Type II supernovae are associated with the collapse of massive stars that have retained their hydrogen envelopes.

Type Ia supernovae result from the thermonuclear explosion of a carbon-oxygen white dwarf, leaving behind a neutron star or black hole.

Type Ia supernovae exhibit a rapid rise in brightness followed by an exponential decay, making them useful as standard candles in cosmology.

Type II supernovae produce neutron stars as remnants when the core of the massive star collapses and undergoes a rapid neutronization process.

Type Ia supernovae are triggered by electron capture in a carbon-oxygen white dwarf, leading to a runaway thermonuclear reaction.

Type Ic supernovae are associated with the collapse of massive stars that have lost their hydrogen and helium envelopes, leaving behind a core that directly collapses to form a black hole.

Type II supernovae exhibit a slow rise in brightness followed by a gradual decline, with a plateau phase due to the interaction of the ejecta with the circumstellar material.

Type II supernovae are responsible for the production of heavy elements through the r-process, which occurs during the rapid neutron capture process in the supernova ejecta.

Supernovae release enormous amounts of energy, typically in the order of 10^44 joules, which is equivalent to the energy output of the Sun over billions of years.

Type Ic supernovae are often associated with the production of gamma-ray bursts, which are the most energetic electromagnetic events in the universe.

Supernova explosions occur on very short timescales, typically lasting for a few seconds, during which the star undergoes a dramatic transformation.

Type Ia supernovae produce Type Ia supernova remnants, which are characterized by their distinct composition and morphology.

Stars in the mass range of 10-25 solar masses typically undergo Type II supernovae when they exhaust their nuclear fuel and undergo core collapse.

Type Ib supernovae produce Type Ib supernova remnants, which are characterized by their lack of hydrogen lines in their spectra.