red supergiant
A star stops being a main sequence star when it exhausts the hydrogen fuel in its core, leading to changes in its internal structure and a transition to a different phase of stellar evolution, such as becoming a red giant or a white dwarf. This change marks the end of the star's main sequence stage.
Our Sun is currently a main sequence star. It is not a supernova, as supernovae are massive explosions that occur at the end of a star's life cycle, and it is not a white dwarf, which is a type of star that has exhausted its nuclear fuel and collapsed to a very dense state.
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.
The main sequence of a black hole starts with a massive star collapsing under its own gravity to form a singularity, which is a point of infinite density and zero volume. This singularity is surrounded by an event horizon, beyond which not even light can escape, leading to the characteristic black appearance.
When a star "goes off the main-sequence" it generally means the star has run out of hydrogen fuel and is beginning the post-main-sequence or its end of life phase. The main sequence of a star is the time where it is no longer just a proto-star but is burning hydrogen as a primary source of fuel.
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.
red supergiant
A star stops being a main sequence star when it exhausts the hydrogen fuel in its core, leading to changes in its internal structure and a transition to a different phase of stellar evolution, such as becoming a red giant or a white dwarf. This change marks the end of the star's main sequence stage.
The birth line in the Hertzsprung-Russell Diagram represents the path that stars follow as they evolve from protostars to the main sequence. It shows how a star changes in luminosity and temperature as it progresses towards becoming a main sequence star. Stars begin their life on the birth line before settling into the main sequence phase.
Depending on how "low" on the chart it will either be a red dwarf or a PMS (Pre-main sequence) star.
It's the size. A dwarf star has reached the end of the road and has collapsed. It's a little old star and people don't notice it, mostly.
A "main-sequence star" is one that fuses hydrogen into helium. Eventually, the star will run out of this specific type of fuel - in other words, it won't have enough hydrogen (at least, near its core) to continue this process.
the main sequence has a limit at the lower end because as a star's mass decreases, its core temperature and pressure decrease too. This eventually causes the nuclear fusion reactions in the core to stop, leading the star to move off the main sequence.
Alioth is a white star nearing the end of it's main sequence. Hope this helps! (:
Spica is a dual star system, with the two members too close for resolution by the best telescopes. The larger, primary star is a blue-white giant, and does have the potential to end it's life as a supernova. The primary is not a main sequence star. The secondary, about 70% the size of the primary, is a main sequence star, also blue white.
No, Betelgeuse is not a main sequence star. It is a red supergiant star, which is a more evolved stage in the life cycle of a star compared to main sequence stars like the Sun. Betelgeuse is near the end of its life and is expected to go supernova in the relatively near future (on astronomical timescales).