M 53 and NGC 5053 in Coma Berenices.
M53 consists of several hundred thousand stars, is approximately 60,000 light-years away, has a diameter of around 200 light-years, and an incredible age of 13.2 billion years.

NGC 5053 mainly consists of old, metal-poor stars. As recently as 1995, it was considered the most metal-poor globular cluster in the Milky Way. The chemical abundances of the stars in NGC 5053 are more similar to those in the dwarf galaxy than to those in the Milky Way halo. Along with the kinematics of the globular cluster, this suggests that NGC 5053 may have been stripped from the Sagittarius Dwarf Galaxy. The star density is very low: 3,500 stars are spread over a diameter of about 160 light-years.There is a tidal bridge connecting M53 with NGC 5053, indicating that the two may have interacted in the past.

Image Details
Date
May 15, 2024
LOCATion
Hannover (Germany)
Sky Quality
Bortle 5
Telescope
Skywatcher 200/1000 @750mm f/3.75
Mount
Skywatcher EQ6-R Pro
Main Camera
ZWO ASI 2600 MC Pro
Gain 100, Offset 18, -10°
Focuser
ZWO EAF
Filter
Baader UV/IR Cut
Exposure
RGB: 189 × 30″ (1h 34' 30'')
Guiding
ZWO ASI 120MM, PHD2
Calibration
Flats, Darks, Darkflats
Software
N.I.N.A., EQMod
Other
Starizona Nexus Reducer & Corrector
Processing
Astropixelprocessor, Photoshop, Pixinsight
  
  
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