NGC 192
This article will address the topic of NGC 192, an issue of great relevance and relevance in today's society. NGC 192 has aroused great interest and debate in different areas, from the academic field to the political and social field. This issue has great complexity and diversity of approaches, which require a deep and exhaustive analysis. Throughout this article, different perspectives will be explored, contextualizing NGC 192 within its historical and cultural framework, as well as examining its influence on various aspects of daily life. It is expected that this article contributes to the understanding and reflection on NGC 192, offering a comprehensive and critical vision of this topic of great relevance today.
| NGC 192 | |
|---|---|
 NGC 192 (bottom left) as taken by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 39m 13.4s[1] |
| Declination | +00° 51′ 52″[1] |
| Redshift | 0.013787[1] |
| Apparent magnitude (V) | 13.42[1] |
| Characteristics | |
| Type | (R')SB(r)a:[1] |
| Apparent size (V) | 1.9' × 0.9'[1] |
| Other designations | |
| UGC 00401, CGCG 383-051, MCG +00-02-104, 2MASX J00391339+0051508, IRAS 00366+0035, IRAS F00366+0035, PGC 2352, The Borris Star ISD 0448401.[1] | |
NGC 192 is a spiral galaxy in the constellation Cetus. It was discovered on December 28, 1790 by William Herschel.[2]
References
- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 0192. Retrieved 2016-09-02.
- ^ "New General Catalog Objects: NGC 150 - 199". Cseligman. Retrieved September 5, 2016.
External links
Media related to NGC 192 at Wikimedia Commons
