No, it is a red dwarf
A black dwarf is a theoretical stellar remnant that is predicted to form when a white dwarf cools down completely. It is essentially a cold, dark, and compact stellar remnant with no nuclear fusion activity. No black dwarfs are currently known to exist in the Universe due to the immense timescales required for white dwarfs to cool down to become black dwarfs.
A white dwarf doesn't run out of fuel because it no longer undergoes nuclear fusion. Instead, it gradually cools down over billions of years until it becomes a cold, dark object known as a black dwarf. This process takes an extremely long time, so no white dwarfs have had enough time to evolve into black dwarfs yet.
It loses its outer layers because it has expanded to the point where gravity can no longer hold it together. The inner part of the star becomes a white dwarf, called a white dwarf because it is still glowing with the remaining heat of the dead star. It eventually becomes a black dwarf, where it has radiated all its energy out and no longer glows.
A collapsed star after using up its fuel is called a white dwarf, neutron star, or black hole, depending on its mass. White dwarfs are remnants of low to medium mass stars, neutron stars are remnants of massive stars, and black holes are formed when very massive stars collapse.
The Sun is currently a main-sequence star, which means it is in the stable phase of its life cycle where nuclear fusion in its core is converting hydrogen into helium. It will eventually evolve into a white dwarf, not a black dwarf, after exhausting its nuclear fuel.
The remains of a star that has no fuel but still glows faintly are called white dwarfs. White dwarfs are very dense, Earth-sized objects that are formed when a low to medium mass star exhausts its nuclear fuel and sheds its outer layers. The residual heat from the white dwarf's formation causes it to glow faintly for billions of years.
A star that has burned out and no longer has fuel to sustain nuclear fusion in its core is called a white dwarf, not a black dwarf. A white dwarf is the remnant core of a low to medium mass star after its outer layers have been ejected. Over time, a white dwarf will cool down and eventually become a black dwarf, but this process takes billions of years.
A black dwarf is a theoretical stellar remnant that is predicted to form when a white dwarf cools down completely. It is essentially a cold, dark, and compact stellar remnant with no nuclear fusion activity. No black dwarfs are currently known to exist in the Universe due to the immense timescales required for white dwarfs to cool down to become black dwarfs.
No, you cannot. As the name suggests, a "black" dwarf is "black" because it has stopped burning hydrogen/helium for fuel, and is now not producing energy and has cooled to the point that it no longer glows.
The gas being used as a fuel source for white dwarfs is primarily hydrogen. During nuclear fusion reactions in the core of a white dwarf, hydrogen atoms are fused together to form helium, releasing energy in the process.
A star, after using all of it's fuel explodes. We call this a super nova, and after this the star will either become a black dwarf star (or maybe a white dwarf) or it will collapse in on its self creating a black hole.
No. A brown dwarf is a star that has too low a mass to start nuclear fusion. A black dwarf is a former white dwarf, the remnant of a low to medium mass star that ran out of fuel in its core.
It is dead. It becomes a black dwarf, just a rock.
A white dwarf star is a star that has burned off all of its helium and hydrogen fuel, but which is still hot. After it cools off (which would theoretically take hundreds of billions of years), it would become a black dwarf.
First a red giant, then a white dwarf and finally after billions of years a black dwarf. See related questions
A white dwarf doesn't run out of fuel because it no longer undergoes nuclear fusion. Instead, it gradually cools down over billions of years until it becomes a cold, dark object known as a black dwarf. This process takes an extremely long time, so no white dwarfs have had enough time to evolve into black dwarfs yet.
Yes, a mid-sized star can eventually become a white dwarf or a black dwarf. After exhausting its nuclear fuel, the star sheds its outer layers to form a planetary nebula, leaving behind a white dwarf. Over trillions of years, a white dwarf may cool and fade into a black dwarf, although this process would take longer than the current age of the universe.