Nowadays, NGC 3501 is a topic of great relevance that arouses wide interest in different areas. Whether in the academic, scientific, social or cultural field, NGC 3501 has managed to capture the attention of experts and the general public. Its multiple facets and implications make it a topic of constant study and debate. In this article, we will explore the different perspectives and reflections around NGC 3501, as well as its impact on current society and its possible future implications.
NGC 3501 | |
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![]() NGC 3501, photographed by the Hubble Space Telescope | |
Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 11h 02m 47.307s[1] |
Declination | +17° 59′ 22.31″[1] |
Redshift | 0.003769[2] |
Heliocentric radial velocity | 1130[2] |
Distance | 77.02 ± 6.06 Mly (23.615 ± 1.857 Mpc)[2] |
Apparent magnitude (B) | 13.8[3] |
Characteristics | |
Type | Scd:[2] |
Size | 89,600 ly (27,480 pc)[2] |
Apparent size (V) | 4.00′ × 0.44′[2] |
Other designations | |
UGC 6116, MCG +03-28-051, PGC 33343 |
NGC 3501 is a spiral galaxy 80 million light years away, located in the constellation Leo. It was discovered on 23 April 1881 by French astronomer Édouard Stephan.[4]
NGC 3501 was imaged by the Hubble Space Telescope in 2014, showing an edge-on spiral galaxy; its companion NGC 3507 is not included in the photograph.[5] It is a member of the NGC 3607 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.[6]