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Observations of thousands of main sequence stars show that there is definite relationship between their mass and their luminosity. The more massive main sequence stars are hotter and more luminous than the low-mass main sequence stars.
High mass stars are hotter, and are white or blue white. Extremely high mass stars may even shine a pale violet, which is more "blue" than blue white. High mass stars are also much brighter than low mass stars, because they produce much more energy.
The most massive stars are the blue giants, supergiants and hypergiants. Rigel, for example, is the brightest star in the constellation Orion. It has 17 times the mass of the Sun, and gives off 66,000 times the energy of the Sun.
Want to learn more? Evolutionary StageDurationLuminosityMain Sequence1010 years1 LSunRed Giant109 years~2000 LSunHorizontal branch108 years~100 LSunAsymptotic Giant branch107 years~10,000 LSun
The Sun is currently a main sequence star and will remain so for another 4-5 billion years. It will then expand and cool to become a red giant, after which it will shrink and heat up again to become a white dwarf. The white dwarf star will run out of nuclear fuel and slowly cool down over many billions of years.
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Throughout the subsequent billions of years, the Sun's luminosity increased gradually and will continue to increase in the future. Astronomers estimate that the Sun's luminosity will increase by about 6% every billion years.
Which mass star becomes the most luminous? \u200bThe 40 solar mass star has the highest luminosity at 425,402.46 solar luminosities.
Different stages of life cycle of stars are: Giant Gas Cloud. Protostar. T-Tauri Phase.
A smaller star, like the Sun, will gradually cool down and stop glowing. During these changes it will go through the planetary nebula phase, and white dwarf phase. After many thousands of millions of years it will stop glowing and become a black dwarf. A massive star experiences a much more energetic and violent end.
After the supernova, the core will collapse to a single point- a black hole. This will have a very low temperature in the nano-Kelvin region. After the 20Msun star explodes, it will leave behind a hot, dense, spinning core- a neutron star. It will reach its maximum temperature during the Neutron Star stage of its life.

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