Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  21 eta Cyg  ·  B144  ·  Sh2-101  ·  The star ηCyg
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Sh2-101 Tulip Nebula #1, Molly Wakeling
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Sh2-101 Tulip Nebula #1

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Sh2-101 Tulip Nebula #1, Molly Wakeling
Powered byPixInsight

Sh2-101 Tulip Nebula #1

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Description

The Tulip Nebula!
Also listed in the Sharpless catalog as Sh2-101, this emission nebula lies about 6,000 lightyears away in the constellation of Cygnus, the Swan.  Cygnus is high above our heads in the Northern Hemisphere in the summertime, and is easily found by locating its two brightest stars, Deneb and Sadr, which form the body of the Swan.  

Just to the right of the Tulip itself are two bright stars, the lower of which is a binary companion to one of the first suspected black holes.  It was discovered from a rocket-launched X-ray detector in 1964 and is named Cygnus X-1.  It's one of the brightest X-ray sources yet seen.  The black hole is about 21.2 solar masses and has an event horizon of about 300 km (186 miles).  It pulls material off the stellar wind of the companion star, forming an accretion disk that gets superheated to millions of degrees, which is the source of the X-rays.  

Narrowband imaging saves the day under light-polluted skies!  This was captured from my backyard in Dayton, OH, which is about Bortle 7 on the light pollution scale.  Not only was I able to get a nice bright Tulip, but I picked up a lot of the fluffy hydrogen gas clouds in the background that suffuse the Cygnus region.  This particular filter, the Optolong L-eXtreme, captures a small sliver of the color spectrum around hydrogen-alpha and oxygen-III emission (red and blue in color, respectively).

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Sh2-101 Tulip Nebula #1, Molly Wakeling