At the end of the red giant phase, a star undergoes significant changes depending on its mass. For low to intermediate-mass stars, the outer layers are expelled, forming a planetary nebula, while the core contracts and ultimately becomes a white dwarf. In more massive stars, nuclear fusion continues to create heavier elements until an iron core forms, leading to a supernova explosion. This explosion can leave behind a neutron star or a black hole, depending on the initial mass of the star.
Yes Star spend most of their life span as a main sequence star. A star end will depend on its size in life the end of a start can be a red giant to supernova, a white dwarf, pulsar, or black hole.
After a red giant phase, a star will undergo further evolutionary stages depending on its mass. A low-mass star like the Sun will evolve into a planetary nebula and then eventually into a white dwarf. A high-mass star will undergo a supernova explosion, leading to the formation of a neutron star or black hole.
the examples are Mu Cephei or Garnet Sidus
A dwarf star is denser than a giant star. Dwarf stars have a higher density due to their smaller size and higher mass compared to giant stars. Giant stars have larger volumes and lower densities as they have expanded and become less dense towards the end of their life cycle.
Beta Piscium is a binary star system located in the constellation of Pisces. It consists of a giant star and a white dwarf star. The giant star is classified as a K-type giant, which means it is an orange star that is nearing the end of its life cycle.
super giant.
Nothing usually happens in a binary systems when a star becomes a giant except when two stars are orbiting each other and the one star become a giant it will contract and expand due to the nuclear fusion and it will interact with the other star and will cause a phenomena known as a nova.
Yes Star spend most of their life span as a main sequence star. A star end will depend on its size in life the end of a start can be a red giant to supernova, a white dwarf, pulsar, or black hole.
A red giant.
A star become a red giant when the core contracts, the temperature increases and the outer layers of the star begin to expand. By the end of this phase, the star can be 10 to 100 times it diameter. When the temperature in the core reaches 100 000 000°C, the helium start fusing into carbon. Because the star has expanded to such an enormous size, that the outer layer are much cooler than when the star was a main sequence star. It therefore appears red, earning the name of red giant.
After a red giant phase, a star will undergo further evolutionary stages depending on its mass. A low-mass star like the Sun will evolve into a planetary nebula and then eventually into a white dwarf. A high-mass star will undergo a supernova explosion, leading to the formation of a neutron star or black hole.
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A blue giant star goes through multiple stages during its life cycle: formation from a collapsing nebula, main sequence where it fuses hydrogen into helium, red giant phase where it expands and fuses heavier elements, and finally, depending on its mass, it may end as a supernova or a black hole.
the examples are Mu Cephei or Garnet Sidus
red giant
The three stages in star life cycles that are the same for most stars are the main sequence, red giant (or supergiant) phase, and the final stage, which can lead to either a white dwarf, neutron star, or black hole, depending on the star's mass. During the main sequence, stars fuse hydrogen into helium. In the red giant phase, they expand and begin fusing heavier elements. Finally, the end stage varies based on mass, leading to different remnants after the star exhausts its nuclear fuel.
Before a star becomes a red giant, it goes through the stage of being a main sequence star, where nuclear fusion in its core converts hydrogen into helium, releasing energy in the form of light and heat.