M 3
Globular Cluster
M 3 (also NGC 5272) is a globular cluster of stars in the northern constellation of Canes Venatici.

It was discovered on May 3, 1764 and was the first Messier object to be discovered by Charles Messier himself. Messier originally mistook the object for a nebula without stars. This mistake was corrected after the stars were resolved by William Herschel around 1784. Since then, it has become one of the best-studied globular clusters.

This cluster is one of the largest and brightest, and is made up of around 500,000 stars. It is estimated to be 11.4 billion years old and 32,600 light-years (10.0 kpc) away from Earth. Messier 3 is quite isolated as it is 31.6 kly (9.7 kpc) above the Galactic plane and roughly 38.8 kly (11.9 kpc) from the center of the Milky Way. It contains 274 known variable stars, by far the most found in any globular cluster.

Image Details
Date
May 14, 2022 & May 27, 2023
LOCATion
Hannover (Germany)
Sky Quality
Bortle 5
Telescope
Skywatcher 200/1000 f/5
Mount
Skywatcher EQ6-R Pro
Main Camera
ZWO ASI 2600 MC Pro
Gain 100, Offset 18, -10°
Exposure
658 x 30' (5h 29′)
Guiding
ZWO ASI 120 MM, PHD2
Calibration
Flats, Darks, Darkflats
Software
N.I.N.A., EQMod
Processing
Astropixelprocessor, Photoshop, Pixinsight
  
  
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