What is Emission nebula?
[[Image:M57 The Ring Nebula.JPG|thumb|Planetary nebulae, here represented by the [[Ring Nebula]], are examples of emission nebulae.]] An '''emission nebula''' is a [[cloud]] of [[Plasma (physics)|plasma]] emitting light in many colors. The glowing is caused by a [[star]] being near the nebula. There are many types of emission nebula. [[H II region]]s are caused when stars are forming and are very hot, causing the plasma to heat up. [[Planetary nebula]]e are made when where a dying star has thrown off its outer layers. This causes the core of the star to heat up the plasma. ==General information== A nebula's color depends on what chemicals are in it, and how [[ionization|ionized]] it is. Because most of the universe is made of [[hydrogen]], many emission nebulae appear red. Hydrogen glows red when it is hot. If the nebula is very hot, other types of gas will be heated and the it might also glow blue and green. By looking at which colors are glowing in a nebula, one can figure out what it is made of. Emission nebulae sometimes look like they have dark areas in them. This is because [[interstellar medium|clouds]] of dust block the light when it is traveling between the nebula and the [[Earth]]. ==Related pages== *[[Reflection nebula]] *[[Planetary nebula]] [[Category:Nebulae]]