A Star Is Born

Stars are the most common object in the night sky. They come in different colors and brightness. Grab a pair of binoculars and the number you can see goes from too many to count to more than you thought possible. It seems as though they've always been there, but where did they come from?

Orion Nebula, a stellar nursery (NASA)

Gas and dust in space pulled together by gravity attract more material. More mass has more gravity, so it continues to attract more material, while also collapsing into itself. As it collapses and becomes more dense, it begins to hear up. At some point, what is now considered a core begins to fuse hydrogen atoms into helium. The pressure of the energy radiating from the new star is enough to keep it from collapsing into itself further.
Not all of the gas and dust gets sucked into the star. It will swirl around the star and conceal into planets and asteroids, like what happened here in our solar system. In other systems, multiple stars may form rather than just one like we got stuck with.

Life cycle of a star (NASA)

If a star is massive enough, it will blow itself apart in a supernova. Gas and dust from the exploding star will fly out into space and the process will begin again. This week's information comes from NASA.