NGC 3293
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| Image of the star cluster NGC 3293 and the surrounding, reddish HII region Gum 30 / RCW 51 with the MPG / ESO 2.2 m telescope . | |
| AladinLite | |
| Constellation | Keel of the ship | 
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Position  equinox : J2000.0  | 
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| Right ascension | 10 h 35 m 48.7 s | 
| declination | -58 ° 13 ′ 28 ″ | 
| Appearance
 
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| classification | I3r | 
| Brightness (visual) | 4.7 likes | 
| Brightness (B-band) | 4.84 likes | 
| Angular expansion | 5 ' | 
| Number of stars | > 1500 | 
| Brightest star | HD 91943; 6.52 mag | 
| Variable stars | > 10; including various β-Cephei variables , e.g. B. V381 Car (HD 92024) | 
| Redness ( excess color E (BV)) | 0.29 ± 0.06 | 
| Physical data
 
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| Affiliation | Milky Way , Carina Complex / Carina OB1 | 
| Radial velocity | −12.3 ± 2.3 km / s | 
| distance | 7600 ly  (2327 pc )  | 
| diameter | 11 ± 1 years | 
| Age | 10 million years | 
| history | |
| Discovered by | Nicolas Louis de Lacaille | 
| Discovery time | 1751 | 
| Catalog names | |
| NGC 3293 • C 1033-579 • OCl 816 • Mel 100 • Cr 224 • Dun 321 • Lund 3276 • ESO 128-SC5 • GC 2144 • h 3276 • Raab 85 | |
NGC 3293 is an open star cluster in the constellation Carina , it is one of the brightest star clusters in the southern sky. It is believed that most, if not all, of the fifty stars formed simultaneously less than 10 million years ago . NGC 3293 is approximately 8,000 light years from the solar system.
It was discovered in 1751 by Nicolas Louis de Lacaille during his stay in South Africa using a tiny telescope with an aperture of 0.5 inches.
literature
- Baume et al .: Photometric study of the young open cluster NGC 3293 . bibcode : 2003A & A ... 402..549B
 
Web links
Commons : NGC3293  - Album containing pictures, videos and audio files