Omega Centauri Cluster
Omega Centauri (ω Cen, NGC 5139, or Caldwell 80) is a globular cluster in the constellation of Centaurus that was first identified as a non-stellar object by Edmond Halley in 1677. Located at a distance of 17,090 light-years (5,240 parsecs), it is the largest-known globular cluster in the Milky Way at a diameter of roughly 150 light-years. It is estimated to contain approximately 10 million stars, and a total mass equivalent to 4 million solar masses, making it the most massive-known globular cluster in the Milky Way.
[description from wikipedia]
Details
Telescope:
Takahashi FSQ-106EDX III
Mount:
10Micron GM2000 HPSII
Camera:
QHY600M-PH
Filters:
Astrodon Gen2
Exposure:
LRGB 95:72:62:65 min.
Location:
San Pedro de Atacama — Chile
Author:
© Martin Rusterholz, Astrophotographer