When the protostar accumulates enough mass and the pressure in the core reaches 10 millions degrees Kelvin. then hydrogen fusion can start and the star starts its main sequence phase.
A Main Sequence star.
nucleur fusion
Right now the sun is a main sequence star. When it uses up the hydrogen in its core it will become a red giant then shed its outer layers to become a white dwarf.
A main sequence star burns hydrogen to helium. Once a main sequence star exhausts all of the hydrogen, it begins to expand and burn helium causing if to become a red giant.
No, Betelgeuse has already past that stage and has become a red supergiant.
A Main Sequence star.
nucleur fusion
Right now the sun is a main sequence star. When it uses up the hydrogen in its core it will become a red giant then shed its outer layers to become a white dwarf.
I actually thought that would be when the star starts fusing hydrogen into helium... But apparently there are other stages between those two.According to Wikipedia, "[The protostar phase] ends when the protostar blows back the infalling gas and is revealed as an optically visible pre-main-sequence star, which later contracts to become a main sequence star."Pre-main sequence means the star is not yet on the main sequence; and that, in turn, basically means that it is not yet fusing hydrogen into helium.
The next step in its life is to become a "red giant" star.
No. Red giants are not on the main sequence.
The next step in its life is to become a "red giant" star.
A main sequence star burns hydrogen to helium. Once a main sequence star exhausts all of the hydrogen, it begins to expand and burn helium causing if to become a red giant.
No, Betelgeuse has already past that stage and has become a red supergiant.
A red main sequence star would be a red dwarf or a branch red giant. To be on the main sequence, you have to have hydrogen nuclear fusion.
The sun is a main sequence star, so 1 AU.
The sun is a main sequence star