Omega Centauri (or NGC 5139)
Acquisition Details
- Date Posted: February 9, 2024
- Resolutions: 975x975 , 800x800 , 300x300
- Date: January 8, 2017
- Time:
- Number of frames: 36
- FPS: 1
- Focal length: 1260
- CMI/CMII/CMIII:
Description
Designation:Omega Centauri (? Cen or NGC 5139) 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 15,800 light-years (4,850 pc), it is the largest 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. Omega Centauri is so distinctive from the other galactic globular clusters that it is thought to have an alternate origin as the core remnant of a disrupted dwarf galaxy.
- User details
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- Jim Janusz
- February 29, 2020
- Followers 2
