Nowadays, NGC 7124 is a topic on everyone's lips. Whether due to its relevance in today's society, its impact on the economy or its influence on culture, NGC 7124 has captured the attention of a large number of people around the world. From its origins to its evolution today, NGC 7124 has played a fundamental role in various aspects of daily life. In this article, we will explore in depth what NGC 7124 is all about, its different ramifications, and its importance in today's world. Through detailed analysis, we hope to shed light on this very relevant topic and provide a more complete view of NGC 7124 for our readers.
NGC 7124 | |
---|---|
![]() The spiral galaxy NGC 7124 | |
Observation data (J2000 epoch) | |
Constellation | Indus |
Right ascension | 21h 48m 05.3679s[1] |
Declination | −50° 33′ 53.979″[1] |
Redshift | 0.017251[1] |
Heliocentric radial velocity | 5172 ± 8 km/s[1] |
Distance | 240.0 ± 16.8 Mly (73.57 ± 5.16 Mpc)[1] |
Apparent magnitude (V) | 12.3[1] |
Characteristics | |
Type | SB(rs)bc[1] |
Size | ~206,200 ly (63.21 kpc) (estimated)[1] |
Apparent size (V) | 2.8′ × 1.1′[1] |
Other designations | |
IRAS 21447-5047, 2MASX J21480540-5033549, PGC 67375, ESO 237- G 002[1] |
NGC 7124 is a large spiral galaxy in the constellation of Indus. Its velocity with respect to the cosmic microwave background is 4988 ± 15 km/s, which corresponds to a Hubble distance of 240.0 ± 16.8 Mly (73.57 ± 5.16 Mpc).[1] However, nine non-redshift measurements give a much closer distance of 191.56 ± 4.26 Mly (58.733 ± 1.306 Mpc).[2] It was discovered by British astronomer John Herschel on 8 July 1834.[3]
NGC 7124 is classified as a LINER galaxy, i.e. it has a type of nucleus that is defined by its spectral line emission which has weakly ionized or neutral atoms, while the spectral line emission from strongly ionized atoms is relatively weak.[1]
One supernova has been observed in NGC 7124: SN 2023pwl (type Ia, mag 16.7) was discovered by ATLAS on 19 August 2023.[4]