Messier 92 or or NGC 6341 

About Messier 92

Messier 92 (M92), is a stunning globular cluster located in the northern constellation Hercules. Here are some fascinating details about this celestial gem:

Discovery and Brightness:

M92 was first discovered by astronomer Johann Elert Bode in 1777. It is one of the brightest globular clusters in the Milky Way. Under good observing conditions, it is visible to the naked eye.

Composition and Age:
M92 is very tightly packed with stars, containing approximately 330,000 stars in total. It belongs to a group of metal-poor clusters, meaning it has low metallicity (elements heavier than hydrogen and helium). As one of the oldest star clusters in the Milky Way, M92’s age is almost the same as the age of the Universe.

Messier 92

Learn more

science.nasa.gov | en.wikipedia.org | messier-objects.com

Photo Capture Info:

Total Integration time: 1 hours, 49 minutes

Optical Equipment Used:

Computerized Equipment and Software:

Photo Capture Info:

Total Integration time: 1 hours, 49 minutes

Optical Equipment Used:

Computerized Equipment and Software:

Mythology:


Hercules, also known as Heracles in Greek mythology, is a legendary figure celebrated for his strength and numerous far-ranging adventures. Here are some key aspects of his mythological background:

!Hercules battles Achelous1

PixInsight Processing Details

Processing on the Luminance Channel