A planetary nebula is a type of emission nebula consisting of an expanding, glowing shell of ionized gas which was ejected from 'red giant' stars late in their lives.
About 20% of the nebulae are roughly spherical (as might be expected) but the majority are not spherically symmetric - some dramatically so. The mechanisms that produce such a wide variety of shapes and features have not yet been explained.
NOTE: The term “planetary nebula” originally used in the late 1770s, is a misnomer - they are unrelated to planets or exoplanets.
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