NGC 1992
In today's world, NGC 1992 has become a topic of great relevance and interest to a wide range of people. Whether due to its impact on society, its relevance in the workplace or its influence on popular culture, NGC 1992 has acquired a prominent place in the public conversation. As we delve into this article, we will explore the various facets of NGC 1992 and examine its importance in different contexts. From its impact on the global economy to its role in the evolution of technology, NGC 1992 continues to be a highly relevant topic in the modern world. Through detailed analysis, we will attempt to shed light on the complexities and nuances surrounding NGC 1992, in hopes of providing a deeper and more complete understanding of this phenomenon.
| 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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