![A nebula (from Latin: “cloud”;[1] pl. nebulae or nebulæ, with ligature or nebulas) is aninterstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any extended astronomical object, including galaxies beyond the Milky Way. TheAndromeda Galaxy, for instance, was referred to as the Andromeda Nebula before galaxies were discovered by Edwin Hubble. Nebulae are often star-forming regions, such as in theEagle Nebula. This nebula is depicted in one of NASA’s most famous images, the “Pillars of Creation”. In these regions the formations of gas, dust, and other materials “clump” together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects.](http://24.media.tumblr.com/tumblr_mbhm6yFi601r8x2ybo1_1280.jpg)
A nebula (from Latin: “cloud”;[1] pl. nebulae or nebulæ, with ligature or nebulas) is aninterstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any extended astronomical object, including galaxies beyond the Milky Way. TheAndromeda Galaxy, for instance, was referred to as the Andromeda Nebula before galaxies were discovered by Edwin Hubble. Nebulae are often star-forming regions, such as in theEagle Nebula. This nebula is depicted in one of NASA’s most famous images, the “Pillars of Creation”. In these regions the formations of gas, dust, and other materials “clump” together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects. 36 notes
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