Location & Date	Backyard, Abbott Observatory- Long Island, NY,  June 30, 2022
Telescope	TMB130SS  910mm F/7 APO, Moonlite focuser, Losmandy G11 Gemini Image scale 1.54 arcsec/pixel
Camera	SBIG ST-10XME Baader L,R,G,B filters CCD temp -10°C
Exposures	L- 15 x 3m  Red- 15 x 3m  Green - 15 x 3m  Blue- 15 x 3m  Bin 1x1 per panel
Planning & Acquisition	Sequence Generator Pro
Processing	CCDStack -  Calibration, Debloom, Normalize, Alignment, Combine Adobe PS -  LRGB combine, Color adjustments, Noise reduction, Sharpen, JPEG conversion RC-Astro Star XTerminator Topaz Sharpen

Wikipedia-

  NGC 6791 is an open star cluster in the Lyra constellation. It was discovered by Friedrich August Theodor Winnecke in 1853. At roughly 8 billion years old, and with an iron to hydrogen abundance ratio that is more than twice that of the Sun, it is one of the oldest and most metal-rich clusters in the Milky Way. This is contrary to the typical rule-of-thumb where older means more metal-poor. Compounded with the fact that it has an unusually high population of stars, NGC 6791 is among the most studied clusters in the sky.

  Among the dimmest stars in the cluster are groups of white dwarfs that are 6 billion years old and another group that appear to be 4 billion years old. The ages are out of sync with those of the cluster's normal stars, which are 8 billion years old. This seeming contradiction in age for this cluster has been studied and a solution proposed with age of about 8 billion years.

NGC 6791 position shown relative to our location (Sun) in the Milky Way Galaxy

Age: 8,318 million years

Galatic Longitude: 70

Galatic Latitude: 10.9

Distance from Galatic Plane:3,162 ly above the galatic plane

Above image and info provided by Our Galaxy 3D Atlas application and used with permission by Otherwise