The importance of NGC 5630 in contemporary society is undeniable. Whether professionally, culturally, personally or politically, NGC 5630 has a significant impact on our lives. As technology advances, NGC 5630 continues to be relevant and its influence becomes increasingly evident. In this article, we will explore the role and importance of NGC 5630 in different contexts, analyzing its evolution over time and its impact on the world today. Additionally, we will examine how NGC 5630 has shaped the way we think, act and relate, and how we can harness its potential to promote change and progress in society.
NGC 5630 | |
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![]() The barred spiral galaxy NGC 5630 | |
Observation data (J2000 epoch) | |
Constellation | Boötes |
Right ascension | 14h 27m 36.5894s[1] |
Declination | +41° 15′ 27.918″[1] |
Redshift | 0.008918[1] |
Heliocentric radial velocity | 2673 ± 2 km/s[1] |
Distance | 135.9 ± 9.5 Mly (41.68 ± 2.92 Mpc)[1] |
Apparent magnitude (V) | 13.0[1] |
Characteristics | |
Type | Sdm?[1] |
Size | ~75,700 ly (23.21 kpc) (estimated)[1] |
Apparent size (V) | 2.2′ × 0.7′[1] |
Other designations | |
HOLM 649A, IRAS 14256+4128, 2MASX J14273658+4115281, UGC 9270, MCG +07-30-014, PGC 51635, CGCG 220-018[1] |
NGC 5630 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 2826 ± 11 km/s, which corresponds to a Hubble distance of 41.68 ± 2.92 Mpc (~136 million light-years).[1] It was discovered by German-British astronomer William Herschel on 9 April 1787.[2]
NGC 5630 is listed as a field galaxy, i.e. one does not belong to a larger galaxy group or cluster and hence is gravitationally alone.[3]
Three supernovae have been observed in NGC 5630:
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