NGC 1983
In this article we will explore the fascinating history of NGC 1983, analyzing its evolution over time and its relevance in contemporary society. From its origins to its impact today, NGC 1983 has played a crucial role in various fields, influencing people, communities and cultures around the world. Through a multidisciplinary approach, we will examine the highlights of NGC 1983, from its contributions in the past to its future implications, offering a comprehensive look that will allow readers to fully understand the importance of NGC 1983 today.
| NGC 1983 | |
|---|---|
 The open cluster NGC 1983 through the Hubble Space Telescope Credit: NASA/ESA | |
| Observation data (J2000.0 epoch) | |
| Right ascension | 05h 27m 44.2s[1] |
| Declination | −68° 59′ 10″[1] |
| Apparent magnitude (V) | 9.9[2] |
| Apparent dimensions (V) | 1.0[3] |
| Physical characteristics | |
| Other designations | ESO 56-SC133 |
| Associations | |
| Constellation | Dorado |
NGC 1983 (also known as ESO 56-SC133) is an open cluster associated with an emission nebula which is located in the Dorado constellation and part of the Large Magellanic Cloud. It was discovered by John Herschel on 11 November 1836.[4] It has an apparent magnitude of 9.9 [2] and its size is 1.0 arc minutes.[3]
References
- ^ a b "NED results for object NGC 1983 *". NED. Retrieved 27 November 2017.
- ^ a b "Object: NGC 1983 (*)". SEDS. Retrieved 27 November 2017.
- ^ a b "NGC 1983 -- Cluster of Stars". SIMBAD. Retrieved 27 November 2017.
- ^ "NGC 1983 (in the Large Magellanic Cloud)". seligman. Retrieved 27 November 2017.
External links
Media related to NGC 1983 at Wikimedia Commons
 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |