In today's world, NGC 4273 is a topic that has captured the attention of people from all walks of life. With a significant impact on society, daily life and culture, NGC 4273 has emerged as a crucial topic of conversation today. From its influence on the way we communicate to its impact on the global economy, NGC 4273 has generated passionate debate and a range of divergent opinions. In this article, we will explore in depth the impact of NGC 4273 on our lives, examining its implications on a personal, social and global level.
NGC 4273 | |
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![]() Barred spiral galaxy NGC 4273 | |
Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 12h 19m 56.0407s[1] |
Declination | +05° 20′ 36.497″[1] |
Redshift | 0.007942[1] |
Heliocentric radial velocity | 2381 ± 2 km/s[1] |
Distance | 94.72 ± 4.68 Mly (29.040 ± 1.435 Mpc)[1] |
Group or cluster | NGC 4235 group (LGG 281) |
Apparent magnitude (V) | 11.9[1] |
Characteristics | |
Type | SB(s)c[1] |
Size | ~68,900 ly (21.12 kpc) (estimated)[1] |
Apparent size (V) | 2.3′ × 1.5′[1] |
Other designations | |
IRAS 12173+0537, 2MASX J12195606+0520361, UGC 7380, MCG +01-32-008, PGC 39738, CGCG 042-028[1] |
NGC 4273 is a barred spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 2727 ± 24 km/s, which corresponds to a Hubble distance of 131.2 ± 9.3 Mly (40.23 ± 2.84 Mpc).[1] However, 20 non-redshift measurements give a distance of 94.72 ± 4.68 Mly (29.040 ± 1.435 Mpc).[2] It was discovered by German-British astronomer William Herschel on 17 April 1786.[3]
According to A.M. Garcia, NGC 4273 is one of the galaxies in the NGC 4235 group (also known as LGG 281). This galaxy group contains at least 29 members, of which 18 appear in the New General Catalogue and 4 in the Index Catalogue.[4]
Two supernovae have been observed in NGC 4273: