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The Ring Nebula

The Ring Nebula is an example of a “planetary nebula”—though these objects have nothing to do with planets.  Through early, low-powered telescopes, their circular shapes resembled planets.  Planetary nebulae are formed when a Sun-like star begins to run out of fuel, inflates to become an enormous Red Giant star, and then blows its outer layers into space.  The shell of gas, expanding and cooling, will eventually dissipate, and all that will be left of the original star is a compact, Earth-sized object known as a White Dwarf—the dead star’s remains.  The Ring Nebula is believed to be about 2300 light years away and about one light year in diameter.  

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