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[1] the nearest star to earth is the sun Stars are essentially the building blocks of galaxies and are the source of all the heavier elements. Many other stars are visible to the naked eye at night
Their immense distances from earth make them appear as fixed points of light. A star is a giant sphere of extremely hot, luminous gas (mostly hydrogen and helium) held together by gravity 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. 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.
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. 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. Where do stars come from
Every star forms in a huge cloud of gas and dust Over time, gravity causes the cloud to contract, drawing the gas closer and closer together As more gas accumulates at the center, it becomes denser and pressure increases This causes it to heat up and begin to glow.
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