Celestial hemisphere:  Southern  ·  Constellation: Pavo (Pav)  ·  Contains:  NGC 6752
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Southern Globular Cluster NGC 6752, Alex Woronow
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Southern Globular Cluster NGC 6752

Getting plate-solving status, please wait...
Southern Globular Cluster NGC 6752, Alex Woronow
Powered byPixInsight

Southern Globular Cluster NGC 6752

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Description

Globular Cluster NGC 6752

OTA: RCOS (14.5” f/8)

Camera: SBIG STXL 11002

Observatory: Heaven’s Mirror, Au

EXPOSURES:

Red: 9 x 600 sec

Blue: 6 x 600

Green: 10 x 600

Lum. 12 x 600

Total exposure: ~6 hours

Image Width: ~1/2 deg

NGC 6752 resides in the Southern sky at a declination of -60 deg. It also lies about 13,000 light-years from us, tagging it as our closest globular cluster. It consists of over 100,000 stars in a sphere about 1.3 light-years in diameter, making it an intermediate density globular cluster.

Globular clusters are spherical concentrations of stars that orbit the galactic center and are dispersed in a broad halo surrounding the galaxy. Globular clusters contain older, redder stars than the galaxy at large, and may represent some of the first stars to be produced in the galaxy. However, the globular clusters’ origins and roles in galactic evolution remain unclear. It does appear clear that globular clusters formed as part of the star formation of the parent galaxy, rather than as a separate galaxy that subsequently underwent captured into their parent galaxies.

(Source: largely Wikipedia)

Processed by Alex Woronow (2019) using PixInsight, Matlab, AuroraHDR, Topaz. Image was photometrically calibrated in PI, and only saturation was subsequently adjusted. Sharpening of luminosity was done largely in Matlab, with some additional tweaks in Aurora and Topaz.

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    Southern Globular Cluster NGC 6752, Alex Woronow
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C

Description: better core resolution

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Southern Globular Cluster NGC 6752, Alex Woronow