Rename Crescent Nebula to Cerebrum Nebula

The Issue

Photo of Crescent Nebula by Chuck Ayoub

The Crescent Nebula resembles a brain. So my suggestion is that we rename it to Cerebrum Nebula.

Cerebrum is latin for brain.

A potential different alternative:
If one think of the nebula as a brain, it might be the mind of the universe.

Alternative name would then be: Magno Cerebri Nebula (Big Brain Nebula)


What is the Crescent Nebula?

The Crescent Nebula (also known as NGC 6888, Caldwell 27, Sharpless 105) is an emission nebula in the constellation Cygnus, about 5000 light-years away from Earth. It was discovered by William Herschel in 1792. It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000 to 400,000 years ago. The result of the collision is a shell and two shock waves, one moving outward and one moving inward. The inward moving shock wave heats the stellar wind to X-ray-emitting temperatures.

It is a rather faint object located about 2 degrees SW of Sadr. For most telescopes it requires a UHC or OIII filter to see. Under favorable circumstances a telescope as small as 8 cm (with filter) can see its nebulosity. Larger telescopes (20 cm or more) reveal the crescent or a Euro sign shape which makes some to call it the "Euro sign nebula".

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The Issue

Photo of Crescent Nebula by Chuck Ayoub

The Crescent Nebula resembles a brain. So my suggestion is that we rename it to Cerebrum Nebula.

Cerebrum is latin for brain.

A potential different alternative:
If one think of the nebula as a brain, it might be the mind of the universe.

Alternative name would then be: Magno Cerebri Nebula (Big Brain Nebula)


What is the Crescent Nebula?

The Crescent Nebula (also known as NGC 6888, Caldwell 27, Sharpless 105) is an emission nebula in the constellation Cygnus, about 5000 light-years away from Earth. It was discovered by William Herschel in 1792. It is formed by the fast stellar wind from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000 to 400,000 years ago. The result of the collision is a shell and two shock waves, one moving outward and one moving inward. The inward moving shock wave heats the stellar wind to X-ray-emitting temperatures.

It is a rather faint object located about 2 degrees SW of Sadr. For most telescopes it requires a UHC or OIII filter to see. Under favorable circumstances a telescope as small as 8 cm (with filter) can see its nebulosity. Larger telescopes (20 cm or more) reveal the crescent or a Euro sign shape which makes some to call it the "Euro sign nebula".

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Petition created on March 15, 2020