This image from the Hubble Space
Telescope shows planetary nebula NGC 7026. Located just beyond the tip of the
tail of the constellation of Cygnus (The Swan), this butterfly-shaped cloud of
glowing gas and dust is the wreckage of a star similar to the sun.
Planetary nebulae, despite their name,
have nothing to do with planets. They are, in fact, a relatively short-lived
phenomenon that occurs at the end of the life of mid-sized stars. As a star’s
nuclear fuel runs out, its outer layers are puffed out, leaving only the hot
core of the star behind. As the gaseous
envelope heats up, the atoms in it are excited, and it lights up like a
fluorescent sign.
Fluorescent lights on Earth get their
bright colors from the gases with which they are filled. Neon signs, famously,
produce a bright red color, while ultraviolet lights (black lights) typically
contain mercury. The same is true for nebulae: their vivid colors are produced
by the mix of gases present in them.
This image was produced by the Wide
Field and Planetary Camera 2 aboard the Hubble Space Telescope. A version of it
was entered into the Hubble’s Hidden Treasures Competition by contestant Linda
Morgan-O’Connor. Hidden Treasures is an initiative to invite astronomy
enthusiasts to search the Hubble archive for stunning images that have never
been seen by the general public.
Image Credit ESA/NASA
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