In this article, we will explore the topic of NGC 540 in depth, with the aim of providing a broad and detailed vision of this topic that is so relevant today. We will analyze its origin, its impact on society, its implications in different areas, as well as future trends and perspectives related to NGC 540. Through a multidisciplinary approach, we will approach this topic from different angles to offer our readers a complete and balanced understanding. This article is proposed as a comprehensive guide for all those interested in acquiring solid and up-to-date knowledge about NGC 540, and it is expected that it will be useful both for specialists in the field and for those approaching this topic for the first time.
| NGC 540 | |
|---|---|
NGC 540 imaged by the Sloan Digital Sky Survey | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 27m 08.90558s[1] |
| Declination | −20° 02′ 11.7187″[1] |
| Redshift | 0.033700±0.000213[2] |
| Heliocentric radial velocity | 10,103±89 km/s[3] |
| Characteristics | |
| Type | SB(s)0:[2] |
| Apparent size (V) | 2.5 × 2.0 arcmin[2] |
| Other designations | |
| LEDA 5410, PGC 5410, SGC 012444-2017.7 | |
NGC 540 is a barred lenticular galaxy in the constellation Cetus. It is estimated to be 451 million light years from the Milky Way and has a diameter of approximately 120,000 light years.[citation needed] The object was discovered on October 15, 1885, by the American astronomer Francis Preserved Leavenworth.[4][5][6]
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