Most stars will become white dwarf stars.
A "high mass" star will become a neutron star or a black hole, after exploding as a supernova.
It will probably explode as a supernova, leaving either a neutron star or black hole.
When a Star runs out of fuel, it will expand into what is known as a "Red Giant". Massive stars will become "Red Supergiants". This phase will last until the star exhausts its remaining fuel. At this point, the pressure of the nuclear reaction is not strong enough to equalize the force of gravity and the star will collapse. Go to related link to read more about Stars... ;)
The sun will eventually exhaust its hydrogen fuel and will undergo a transformation into a red giant star. This will happen in about 5 billion years. After that, it will shed its outer layers and become a white dwarf.
The sun has around 5 billion years left before it exhausts its nuclear fuel and starts to evolve into a red giant star. This phase will mark the end of its stable life cycle and the beginning of a transformation that will eventually lead to the formation of a planetary nebula.
A star becomes a white dwarf after it exhausts its fuel and undergoes fusion reactions that lead to its outer layers being expelled as a planetary nebula. The remaining core collapses and becomes a dense, Earth-sized white dwarf composed mostly of electron-degenerate matter.
It will probably explode as a supernova, leaving either a neutron star or black hole.
When a Star runs out of fuel, it will expand into what is known as a "Red Giant". Massive stars will become "Red Supergiants". This phase will last until the star exhausts its remaining fuel. At this point, the pressure of the nuclear reaction is not strong enough to equalize the force of gravity and the star will collapse. Go to related link to read more about Stars... ;)
When its original source of fuel has run out for instance our sun runs on hydrogen, after the depletion of the original fuel is gone the suns core condenses creating helium were the star expands to great measures were it gets to a size were its limited supply of helium runs out either collapsing into a black hole or a dwarf star
As a star ages and runs out of fuel in its core, it can expand in size as it transitions into a red giant. During this phase, fusion reactions occur in the outer layers of the star, causing it to expand and cool. This expansion happens when the star exhausts its hydrogen fuel and begins fusing helium in its core.
The sun will eventually exhaust its hydrogen fuel and will undergo a transformation into a red giant star. This will happen in about 5 billion years. After that, it will shed its outer layers and become a white dwarf.
The sun has around 5 billion years left before it exhausts its nuclear fuel and starts to evolve into a red giant star. This phase will mark the end of its stable life cycle and the beginning of a transformation that will eventually lead to the formation of a planetary nebula.
Yes, massive blue stars can eventually collapse and form black holes at the end of their lives. When a blue star exhausts its nuclear fuel, it undergoes a supernova explosion and if the remaining core is massive enough, it can collapse into a black hole due to gravitational forces.
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 white dwarf is a remnant of a low mass star. It is formed when a star with a mass less than 8 times that of the Sun exhausts its nuclear fuel and sheds its outer layers, leaving behind a hot, dense core.
A star becomes a white dwarf after it exhausts its fuel and undergoes fusion reactions that lead to its outer layers being expelled as a planetary nebula. The remaining core collapses and becomes a dense, Earth-sized white dwarf composed mostly of electron-degenerate matter.
A star shines due to nuclear fusion in its core, where hydrogen atoms combine to form helium, releasing energy in the process. This energy radiates outwards, providing the star with heat and light. This process can last for billions of years until the star exhausts its nuclear fuel.
Yes, a star can fade out over time as it exhausts its nuclear fuel and enters the later stages of its life cycle. This can happen gradually as the star cools and dims, or it can occur more suddenly in the event of a stellar explosion such as a supernova.