NGC 1910
In today's world, NGC 1910 has become an increasingly relevant topic. Whether due to its impact on society, its influence on popular culture or its importance in the scientific field, NGC 1910 has generated great interest in various areas. Over the years, NGC 1910 and its implications in different contexts have been widely discussed. In this article, we will cover in detail all the relevant aspects of NGC 1910, exploring its origins, its evolution over time and its current relevance. Additionally, we will analyze the future prospects of NGC 1910 and its possible impact on the modern world.
| NGC 1910 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Right ascension | 5h 18m 42.5s[1] |
| Declination | −69° 14′ 12.1″[1] |
| Distance | 160,000 ly (50,000 pc) |
| Apparent magnitude (V) | 11.2 [2] |
| Apparent dimensions (V) | 1.54′ (arcmin.)[1] |
| Physical characteristics | |
| Radius | 71.675 (21.975 pc)[note 1] |
| Other designations | NGC 1910, ESO 56-SC99 |
| Associations | |
| Constellation | Dorado |
NGC 1910, or LH-41, is an OB association in the Large Magellanic Cloud.
Location
NGC 1910's right ascension is 5h 18m 42.5s and its declination is -69° 14′ 12.1″.[3] Its angular size is 1.54 arcminutes.[1]
N119
The cluster has an associated HII region called N119.
Stars
NGC 1910 contains several stars including S Doradus, LH41-1042, LMC195-1, and R85.
See also
Notes and references
- ^ Calculated based on size and distance
- ^ a b c d "SIMBAD search results for NGC 1910". Astronomical Database. Retrieved 17 November 2016.
- ^ "Revised NGC Data for NGC 1910". Retrieved 11 December 2016.
- ^ "NED results for object NGC 1910". Retrieved 11 December 2016.
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