Hydrogen fusion is the main energy source in any star.
Put very simply, four Hydrogen atoms fuse to create Helium. The atomic weight of Helium is slightly less than four Hydrogen atoms the extra mass is released as energy.
Algol is a blue main-sequence star in the constellation Perseus
Polaris - the current North star is a multiple star system., consisting of the main star and smaller companions. The main star Alpha Ursae Minoris is a bright star, a 6 solar mass supergiant and it is a main sequence star. Orbiting very close to this main star is a white dwarf of roughly 1.5 solar masses. This is not a main sequence star. Orbiting further out is the third companion, a 1.39 solar mass star. This is a main sequence star. There are also two more distant components (α UMi C and α UMi D) - Polaris is thought to be part of an open cluster - I do not know if these later two stars are main sequence or not.
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.
Radiant and gravitational Energy.
Unfortunately, it is impossible to tell accurately where a star is on the main sequence.
Nuclear fusion starting with hydrogen.
quasar
by it self, they create & produce their own energy just like the sun
A star's main source of fuel is nuclear fusion, specifically the fusion of hydrogen atoms into helium in its core. This process releases vast amounts of energy in the form of light and heat, which sustains the star's luminosity and temperature.
No, it is not source of any energy as it is a planet not a star.
The energy source is hydrogen undergoing nuclear fusion to helium. The time that lasts depends on the mass of the star but it usually takes a few billion years.
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.
The main source of energy during this stage is gravitational potential energy, as gas in the interstellar cloud collapses under gravity to form a protostar. The energy released from this gravitational collapse heats up the material and initiates the process of star formation.
nuclear fusion
nuclear fusion
The main source of a star's light is nuclear fusion in its core. This process involves the conversion of hydrogen into helium, releasing energy in the form of light and heat. The energy generated by nuclear fusion is what makes stars shine brightly.
The principal source of stellar energy is nuclear fusion, where hydrogen atoms combine to form helium in the core of a star. This process releases immense amounts of energy in the form of light and heat.