What is a Nebula?

 

Definition of a Nebula:

Hubble Space Telescope image An immense body of highly rarified gas and dust in the interstellar spaces of galaxies. A diffuse nebula, such as the CRAB NEBULA, is irregular in shape and ranges up to 100 light-years in diameter. A bright emission nebula, composed primarily of hydrogen gas ionized by nearby hot blue-white stars, radiates its own light; a bright reflection nebula, located near cooler stars, reflects the starlight. A dark nebula, which neither emits nor reflects light because it is too distant from any star, appears as an empty patch in a field of stars or as a dark cloud obscuring part of a bright nebula in the background. A planetary nebula consists of a well-defined shell of gaseous material that glows from the radiation emitted by the central hot star it surrounds.

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