Stars generate energy through nuclear fusion reactions, where lighter elements like hydrogen are combined to form heavier elements like helium, releasing vast amounts of energy.

During a supernova, the core of a massive star collapses, triggering a powerful explosion that releases a vast amount of energy and heavy elements, enriching the surrounding interstellar medium.

Stars with masses similar to our Sun end their lives as white dwarfs, which are dense remnants of stars that have shed their outer layers and cooled down.

Blue supergiants are the hottest and most luminous stars, characterized by their high surface temperatures and intense radiation output.

The core of a star is the central region where nuclear fusion reactions occur, generating the energy that powers the star.

Main sequence stars, like our Sun, spend the majority of their lives in a stable phase where they fuse hydrogen into helium, maintaining a balance between gravitational collapse and outward pressure.

Stars can lose mass through mass ejection, where material from the star's outer layers is expelled into the surrounding space.

Depending on the mass of the progenitor star, a supernova can leave behind either a black hole or a neutron star.

Red giants are stars that have evolved beyond the main sequence stage and have expanded in size, becoming cooler and redder.

A nova is a sudden and dramatic increase in brightness of a star, caused by a thermonuclear runaway on its surface.

Both white dwarfs and neutron stars are compact remnants of stars that have undergone significant gravitational collapse.

The corona is the outermost layer of a star's atmosphere, characterized by its high temperature and low density.

Pulsars are neutron stars that emit regular pulses of radio waves due to their rapid rotation and strong magnetic fields.

Star formation is the process by which interstellar gas and dust collapse under gravity to form stars.

Massive stars are stars with masses several times that of our Sun, and they have shorter lifespans due to their rapid consumption of fuel.