NGC 413
NGC 413 is a topic that has captured the attention of people around the world. Since its emergence, it has generated great interest and debate in different areas, whether in politics, culture, science or society in general. This topic has been the subject of research and analysis by experts and academics, with the aim of understanding its impact and implications. Furthermore, it has aroused the interest of the general population, generating conversations and reflections on different platforms and discussion spaces. In this article we will explore NGC 413 in detail, analyzing its most relevant aspects and offering a broad and varied perspective on this topic.
| NGC 413 | |
|---|---|
 NGC 413 as seen by the SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 12m 31.4s[1] |
| Declination | −02° 47′ 36″[1] |
| Redshift | 0.019403[1] |
| Heliocentric radial velocity | 5,817 km/s[1] |
| Distance | 235.00 ± 32.98 Mly (72.050 ± 10.112 Mpc)[1] |
| Apparent magnitude (V) | 15.06[1] |
| Absolute magnitude (V) | -21.36[1] |
| Characteristics | |
| Type | SB(r)c[1] |
| Apparent size (V) | 1.1' × 0.7'[1] |
| Other designations | |
| MCG -01-04-013, 2MASX J01123140-0247361, 6dF J0112313-024736, PGC 4347.[1] | |
NGC 413 is a spiral galaxy of type SB(r)c located in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. It was described by Dreyer as "extremely faint, pretty small, very little extended."[2]
Image gallery
References
External links
Media related to NGC 413 at Wikimedia Commons
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