The life cycle and death cycle of a star
A star can be described as a huge, luminous plasma sphere drawn together by gravity of its own (Burnell & Green, 2004). The star that is closest to the Earth is probably the Sun. The sun acts as the source of the majority of the energy of the planet. A number of other stars are observable from Earth in the nighttime, appearing as a swarm of static luminous points because of their incalculable distance.
All through history, the stars that were most prominent got grouped into asterisms and constellations, and the liveliest stars got proper names. Extensive stars catalogues have been amassed by astronomers therefore providing standardized star designations. (Krumenaker, 2006).
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A star has be described as a huge, luminous plasma sphere drawn together by gravity of its own. A life cycle of a star is influenced by its mass. When the mass is larger, the life cycle is shorter. The mass of a star is influenced by the matter amount that is obtainable in the nebula of the star.
The nebula is the giant gas and dust cloud wherein it is born. Apart from the processes of star birth, they have a main sequence of life and then they eventually die as dwarf, neutron star, or black hole. All this is extensively cover the overhead content of this paper
Burnell, S. J. B., & Green, S. F. (2004). An introduction to the sun and stars. Milton Keynes: Open University.