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Moreover, star - Fusion, Lifecycle, Evolution As the central temperature and density continue to rise, the proton-proton and carbon cycles become active, and the development of the (now genuine) star is stabilized. The star then reaches the main sequence, where it remains for most of its active life. This aspect of The Life Cycle Of A Star Encyclopedia Britannica plays a vital role in practical applications.
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Furthermore, in order to maintain stability, the star burns fuel in its core until it is depleted, causing the core to collapse into, depending on whether the star is low- or high-mass, either a dense white dwarf, a neutron star, or a black hole. This aspect of The Life Cycle Of A Star Encyclopedia Britannica plays a vital role in practical applications.
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Furthermore, stars as massive as this will have luminosities about one million times greater than that of the Sun. A general model of star formation and evolution has been developed, and the major features seem to be established. This aspect of The Life Cycle Of A Star Encyclopedia Britannica plays a vital role in practical applications.
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Furthermore, star - Fusion, Lifecycle, Evolution Britannica. This aspect of The Life Cycle Of A Star Encyclopedia Britannica plays a vital role in practical applications.
Moreover, stars as massive as this will have luminosities about one million times greater than that of the Sun. A general model of star formation and evolution has been developed, and the major features seem to be established. This aspect of The Life Cycle Of A Star Encyclopedia Britannica plays a vital role in practical applications.
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