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[1] the nearest star to earth is the sun Main sequence stars make up around 90% of the universe’s stellar population. Many other stars are visible to the naked eye at night
Their immense distances from earth make them appear as fixed points of light. Scientists call a star that is fusing hydrogen to helium in its core a main sequence star Of the tens of billions of trillions of stars in the observable universe, only a very small percentage are visible to the naked eye.
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. How does a star work How do they form, live, and eventually die Learn more about these distant objects and their major importance in the universe.
In a very broad sense, a star is simply one of those twinkling points of light you can see in the night sky But that’s not terribly satisfying in either lexicological or physical terms. 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 Stars come in a variety of sizes and colors. 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.
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.
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