Red Supergiant:
A red supergiant is a massive star in the late stages of its life. After it has exhausted its nuclear fuel, the star undergoes significant changes, causing it to expand to a massive size. Red supergiants are much larger than the original main-sequence star they once were. They have relatively low surface temperatures, which causes them to emit a reddish hue. These stars are crucial in the process of nucleosynthesis, as they produce heavy elements that enrich the universe. Eventually, red supergiants will undergo a supernova explosion, resulting in either a neutron star or a black hole.
Black Hole:
A black hole is a region in space where gravity is so intense that nothing, not even light, can escape its gravitational pull. Black holes form from the remnants of massive stars after a supernova explosion. When the core of a massive star collapses under its own gravitational force, it creates an incredibly dense point in space known as a singularity. The region around the singularity, called the event horizon, marks the boundary beyond which nothing can escape the black hole's gravitational grasp. Black holes have a profound influence on their surroundings, distorting space and time, and are among the most mysterious objects in the universe.
White Dwarf:
A white dwarf is the remnant of a low- to medium-mass star that has exhausted its nuclear fuel. As the star's core contracts, its outer layers are expelled into space in a planetary nebula. What remains is a dense and compact stellar remnant, composed primarily of electron-degenerate matter. White dwarfs are relatively small in size but incredibly dense, with a mass comparable to that of the Sun but compressed into a sphere about the size of Earth. Over time, white dwarfs cool down and fade, eventually becoming a cold, dark object known as a black dwarf.
Planetary Nebula:
A planetary nebula is a shell of glowing gas and dust formed from the outer layers of a low-mass star that has shed its outer envelope during the later stages of its evolution. As the star exhausts its nuclear fuel, it expands and loses mass, and the outer layers drift away into space, creating a beautiful and colorful nebula. Despite the name, planetary nebulas have no connection to planets; the term originated from early astronomers who observed them through telescopes and thought they resembled the disks of distant planets. Planetary nebulas play a role in enriching the interstellar medium with heavy elements, which will become the building blocks of future stars and planets.
I hope this helped!
~~~Harsha~~~