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Dates:July 30, 2020 , July 31, 2020
Frames:
Astronomik Blue: 127x60" -20C bin 1x1
Astronomik Green: 114x60" -20C bin 1x1
Astronomik Red: 134x60" -20C bin 1x1
Integration: 6.2 hours
Darks: ~50
Flats: ~50
Bias: ~100
Avg. Moon age: 11.06 days
Avg. Moon phase: 85.06%
Astrometry.net job: 3754243
RA center: 19h 10' 53"
DEC center: -59° 59' 11"
Pixel scale: 1.317 arcsec/pixel
Orientation: -87.193 degrees
Field radius: 0.659 degrees
Resolution: 2812x2250
Locations: Glanmire Home Observatory, Bathurst, NSW, Australia
Data source: Backyard
It seems quite appropriate that this very bright globular cluster is located in the constellation of Pavo - the Peacock. The bright scattering of stars look like the fine display of a peacock's tail when it is trying to impress a prospective mate. This globular cluster does a very fine job of that as well.
According to Wikipedia, NGC6752 is the fourth brightest globular cluster after Omega Centauri, 47 Tucanae and Messier 22. I already have images of Omega Centauri and 47 Tucanae so now I'm going to have to grab some data on Messier 22.
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