NGC 1992
In this article we are going to analyze in detail NGC 1992, a topic that has aroused great interest in contemporary society. From its origins to its impact today, NGC 1992 has been the subject of debate and research in different areas. Over the years, NGC 1992 has influenced the way we perceive the world around us and has played a crucial role in the evolution of various areas of knowledge. Through this article, we will seek to understand the meaning, importance and implications of NGC 1992, as well as its relevance in the current context. We will break down its different facets, explore its multiple applications and analyze its impact on society.
| NGC 1992 | |
|---|---|
 The lenticular galaxy NGC 1992 | |
| Observation data (J2000.0 epoch) | |
| Constellation | Columba |
| Right ascension | 05h 34m 31.8s[1] |
| Declination | −30° 53′ 49″[1] |
| Redshift | 0.035361 +/- 0.000150[2] |
| Heliocentric radial velocity | 10601 +/- 45[2] |
| Distance | 473 million |
| Apparent magnitude (V) | 13.8[3] |
| Apparent magnitude (B) | 14.65 [2] |
| Characteristics | |
| Type | SA0/a?(rs) |
| Apparent size (V) | 1.0 x 0.7 arc minutes[2] |
| Other designations | |
| ESO 423- G 023, AM 0532-305, 2MASX J05343177-3053492, PGC 017466 [2] | |
NGC 1992 (also known as PGC 17466) is a lenticular galaxy located in the Columba constellation. It was discovered by John Herschel on November 19, 1835.[4] It is about 473 million light years from the Milky Way, Its apparent magnitude is 14.65 and its size is 1.0 x 0.7 arc minutes.[2]
References
- ^ a b "Galaxy NGC 1992". DSO. Archived from the original on 1 December 2017. Retrieved 22 November 2017.
- ^ a b c d e f "NGC 1992". NED. Retrieved 22 November 2017.
- ^ "Object: NGC 1992 (*)". SEDS. Retrieved 22 November 2017.
- ^ "NGC 1992". cseligman. Retrieved 22 November 2017.
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