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[1] the nearest star to earth is the sun Throughout the milky way galaxy (and even near the sun itself), astronomers have discovered stars that are well evolved or even approaching extinction, or both, as well as occasional stars that must be very young or still in the process of formation. Many other stars are visible to the naked eye at night
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Their immense distances from earth make them appear as fixed points of light. Stars come in a variety of sizes and colors. Of the tens of billions of trillions of stars in the observable universe, only a very small percentage are visible to the naked eye.
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At the beginning of the end of a star’s life, its core runs out of hydrogen to convert into helium The energy produced by fusion creates pressure inside the star that balances gravity’s tendency to pull matter together, so the core starts to collapse. These large, swelling stars are known as red giants But there are different ways a star’s life can end, and its fate depends on how massive the star is.
The protostar continues to collapse until nuclear fusion begins in its core, leading to the formation of a stable star This stage is known as the main sequence, where the star burns hydrogen into helium. The simplest way to describe a star is that it is a great ball of fire, but it is more complicated than that A star is a giant ball of hydrogen turning into helium through nuclear fusion.
A star’s mass determines its temperature and luminosity, and how it will live and die
The more massive a star is, the hotter it burns, the faster it uses up its fuel, and the shorter its life is. A star is a huge sphere of very hot, glowing gas Stars produce their own light and energy by a process called nuclear fusion Fusion happens when lighter elements are forced to become heavier elements
When this happens, a tremendous amount of energy is created causing the star to heat up and shine
