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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…
History, Observation history & Properties
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omega centauri cluster stars globular core galaxy black hole clusters milky way dwarf mass center disrupted object solar masses ngc
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Omega Centauri | Apparent dimensions (V) | 36′.3 | 1.00 | infobox |
| Omega Centauri | Apparent magnitude (V) | 3.9 | 1.00 | infobox |
| Omega Centauri | Class | VIII | 1.00 | infobox |
| Omega Centauri | Constellation | Centaurus | 1.00 | infobox |
| Omega Centauri | Declination | −47° 28′ 46.1″ | 1.00 | infobox |
| Omega Centauri | Distance | 15.8 ± 1.1 kly (4.84 ± 0.34 kpc) | 1.00 | infobox |
| Omega Centauri | Estimated age | 11.52 Gyr | 1.00 | infobox |
| Omega Centauri | Mass | (4.05±0.1)×106 M☉ | 1.00 | infobox |
| Omega Centauri | Metallicity | [Fe/H] = –1.35 dex | 1.00 | infobox |
| Omega Centauri | Other designations | NGC 5139, GCl 24, ω Centauri, Caldwell 80, Mel 118 | 1.00 | infobox |
| Omega Centauri | Radius | 86 ± 6 ly | 1.00 | infobox |
| Omega Centauri | Right ascension | 13h 26m 47.28s | 1.00 | infobox |
| Omega Centauri | is a | core of a dwarf galaxy that was disrupted and absorbed by the Milky Way | 0.90 | text |
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