NGC 195
In this article, we are going to address the issue of NGC 195 from a comprehensive and detailed perspective. NGC 195 is a topic of great relevance and interest today, since it directly impacts people's lives and different aspects of society. Throughout this text, we will analyze the most relevant aspects related to NGC 195, from its origin and history to its impact today. In addition, we will explore different approaches and opinions on NGC 195 with the aim of offering a broad and enriching vision of this fascinating topic.
| NGC 195 | |
|---|---|
 SDSS image of NGC 195 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 39m 35.8s[1] |
| Declination | −09° 11′ 40″[1] |
| Redshift | 0.016368[1] |
| Apparent magnitude (V) | 14.2g[1] |
| Characteristics | |
| Type | (R)SB(r)a?[1] |
| Apparent size (V) | 1.21' × 0.69'[1] |
| Other designations | |
| MCG -02-02-079, 2MASX J00393578-0911400, IRAS 00370-0928, IRAS F00370-0927, PGC 2391.[1] | |
NGC 195 is a spiral galaxy located in the constellation Cetus. It was discovered in 1876 by Wilhelm Tempel.[2]
References
- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 0195. Retrieved 2016-09-02.
- ^ "New General Catalog Objects: NGC 150 - 199". Cseligman. Retrieved September 7, 2016.
External links
Media related to NGC 195 at Wikimedia Commons
