Towards the end of its life, a star with a size similar to ours will expand to a red giant star as the core contracts and heats up and the hydrogen fuel supply is consumed. It will eventually lose the outer layers and all that will be left is a core, a white dwarf reminant that will slowly cool over millions of years.
A sunlike star goes through the following stages in its life cycle: nebula, protostar, main sequence star, red giant, planetary nebula, and finally white dwarf. During the main sequence stage, the star fuses hydrogen into helium in its core, releasing energy. Once it exhausts its hydrogen fuel, it expands into a red giant before shedding its outer layers to form a planetary nebula. The remaining core becomes a white dwarf, cooling down over billions of years.
The main sequence stage of a sunlike star typically lasts for about 10 billion years. It is during this stage that the star fuses hydrogen into helium in its core, maintaining a balance between the force of gravity pulling in and the energy produced by nuclear fusion pushing out.
The core is necessary for a star's existence, it's the engine that keeps it from collapsing. When this engine runs out of fuel or its fuel vanishes, gravity overcomes and contracts the star until matter from the radiative zone is compressed enough to start fusing hydrogen again to counterbalance gravity.
the answer is white dwarf
If the sun had 10 times its current mass, it would burn through its fuel faster and evolve into a red supergiant star. When it runs out of fuel, it may go through a supernova explosion, leaving behind a dense core called a neutron star or potentially collapsing into a black hole.
A sunlike star goes through the following stages in its life cycle: nebula, protostar, main sequence star, red giant, planetary nebula, and finally white dwarf. During the main sequence stage, the star fuses hydrogen into helium in its core, releasing energy. Once it exhausts its hydrogen fuel, it expands into a red giant before shedding its outer layers to form a planetary nebula. The remaining core becomes a white dwarf, cooling down over billions of years.
The main sequence stage of a sunlike star typically lasts for about 10 billion years. It is during this stage that the star fuses hydrogen into helium in its core, maintaining a balance between the force of gravity pulling in and the energy produced by nuclear fusion pushing out.
The core is necessary for a star's existence, it's the engine that keeps it from collapsing. When this engine runs out of fuel or its fuel vanishes, gravity overcomes and contracts the star until matter from the radiative zone is compressed enough to start fusing hydrogen again to counterbalance gravity.
the answer is white dwarf
A star's core consists mostly of hydrogen. As the star ages, the amount of helium, carbon and other elements in the core increases as they are the result "ash" resulting from the consumption of the hydrogen fuel.
A red giant forms when a star runs out of hydrogen fuel at its core and starts fusing hydrogen in a shell around the core the core. This causes the star to expand and cool.
red giant
The next step in its life is to become a "red giant" star.
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
The next step in its life is to become a "red giant" star.
A star with an iron core is typically a red supergiant star that has exhausted its nuclear fuel and is in the final stages of its life cycle. The iron core forms when the star's fusion processes can no longer generate enough energy to counteract gravitational collapse, leading to a supernova explosion.
Yes, if the star is massive enough when the core collapses a supernova explosion happens.