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Credit & Copyright: Marco Lorenzi  
(Glittering Lights)  
  
  
Explanation:
Fantastic shapes  
lurk in clouds of glowing hydrogen gas in  
NGC 6188.  
  
The  
emission nebula is found near the edge of a  
large molecular cloud, unseen at visible wavelengths,  
in the southern  
constellation  
Ara, about 4,000 light-years away.  
  
Massive, young  
stars of the embedded Ara  
OB1 association  
were formed in that region only a few million years ago,  
sculpting the dark shapes and  
powering the nebular glow with  
stellar winds and intense ultraviolet radiation.  
  
The recent  
star  
formation itself was likely triggered by  
winds and supernova explosions, from  previous generations of massive  
stars, that swept up and compressed the molecular gas.  
  
Joining NGC 6188 on  
this  
cosmic canvas  
is rare emission nebula NGC 6164,  
also created by one of the region's massive O-type stars.  
  
Similar in appearance to many  
planetary nebulae, NGC 6164's striking,  
symmetric gaseous shroud and faint halo surround  
its bright central star at the upper right.  
  
The field of view spans about two full Moons, corresponding to  
70 light years at the estimated distance  
of NGC 6188.  
  
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: emission nebula - OB association - star formation
Publications with words: emission nebula - OB association - star formation
See also:
- APOD: 2025 September 19 Á The NGC 6914 Complex
- APOD: 2025 September 10 Á The Great Lacerta Nebula
- APOD: 2025 July 21 Á Cats Paw Nebula from Webb Space Telescope
- APOD: 2025 July 16 Á The Rosette Nebula from DECam
- APOD: 2025 July 10 Á Lynds Dark Nebula 1251
- APOD: 2025 July 5 Á Ou4: The Giant Squid Nebula
- APOD: 2025 June 26 Á The Seagull Nebula
