It will probably explode as a supernova, leaving either a neutron star or black hole.
When a star exhausts its remaining fuel, it will undergo a series of transformations based on its mass. For example, a massive star will undergo a supernova explosion, leaving behind a neutron star or black hole. A lower-mass star like the Sun will expand into a red giant, shed its outer layers as a planetary nebula, and eventually form a white dwarf.
Yes, eventually the star will run out of fuel. Once it exhausts its hydrogen fuel, it will undergo changes leading to its end of life, such as expanding into a red giant or engaging in a supernova explosion, depending on the star's mass.
A Type II supernova occurs when a massive star with about 8-20 times the mass of the Sun exhausts its nuclear fuel and collapses under its own gravity. The mass required for a Type II supernova is typically around 8 solar masses.
Remnants of low mass stars include white dwarfs, neutron stars, and black holes, depending on the mass of the original star. White dwarfs are remnants of stars similar in mass to our Sun, while neutron stars and black holes are remnants of more massive stars. These remnants are formed after the star exhausts its nuclear fuel and undergoes a supernova explosion.
Low and high mass stars are indirectly related; high mass stars evolve faster and have shorter lifespans compared to low mass stars. This is because high mass stars burn through their fuel at a faster rate due to their higher core temperature and pressure.
When a star exhausts its remaining fuel, it will undergo a series of transformations based on its mass. For example, a massive star will undergo a supernova explosion, leaving behind a neutron star or black hole. A lower-mass star like the Sun will expand into a red giant, shed its outer layers as a planetary nebula, and eventually form a white dwarf.
Yes, eventually the star will run out of fuel. Once it exhausts its hydrogen fuel, it will undergo changes leading to its end of life, such as expanding into a red giant or engaging in a supernova explosion, depending on the star's mass.
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.
It will start using your minerals. Not sure what happens if you run out of those.
What actually happens to the types of stars is that the low mass will turn into a white dwarf and the medium mass will turn into a black dwarf and reproduce a nebula
A star must have a mass several times greater than our Sun's to form a black hole. When the star exhausts its nuclear fuel, it collapses under gravity, leading to a supernova explosion, which can leave behind a black hole if the remnant mass is sufficient.
A Type II supernova occurs when a massive star with about 8-20 times the mass of the Sun exhausts its nuclear fuel and collapses under its own gravity. The mass required for a Type II supernova is typically around 8 solar masses.
A high-mass star will use up its fuel faster than a low-mass one. Depending on the amount of mass that remains at the end of its life, it may convert to a neutron star, or to a black hole.
That is a rigid body mode of high mass that has no oscillation.
Remnants of low mass stars include white dwarfs, neutron stars, and black holes, depending on the mass of the original star. White dwarfs are remnants of stars similar in mass to our Sun, while neutron stars and black holes are remnants of more massive stars. These remnants are formed after the star exhausts its nuclear fuel and undergoes a supernova explosion.
Low and high mass stars are indirectly related; high mass stars evolve faster and have shorter lifespans compared to low mass stars. This is because high mass stars burn through their fuel at a faster rate due to their higher core temperature and pressure.
it changes the delivery of the air and fuel allowed into the engine by the computer it uses more fuel fix it fast