In today's world, NGC 5988 is a topic of great relevance and debate. With the advancement of technology and globalization, NGC 5988 has become a key element in our society, impacting different aspects of daily life. From economics to politics, NGC 5988 has generated discussions and reflections in all areas. This is why it is essential to thoroughly analyze this phenomenon, understand its implications and seek solutions to the challenges it presents. In this article, we will explore different perspectives on NGC 5988, from its origin to its impact today, with the aim of offering a complete and enriching overview of this very relevant topic.
NGC 5988 | |
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![]() The spiral galaxy NGC 5988 | |
Observation data (J2000 epoch) | |
Constellation | Serpens |
Right ascension | 15h 44m 33.8559s[1] |
Declination | +10° 17′ 35.33″[1] |
Redshift | 0.035259[1] |
Heliocentric radial velocity | 10,570 ± 4 km/s[1] |
Distance | 514.6 ± 36.0 Mly (157.78 ± 11.05 Mpc)[1] |
Apparent magnitude (V) | 13.8[1] |
Characteristics | |
Type | Scd[1] |
Size | ~298,900 ly (91.63 kpc) (estimated)[1] |
Apparent size (V) | 1.2′ × 1.0′[1] |
Other designations | |
IRAS F15421+1026, 2MASX J15443383+1017356, UGC 9998, MCG +02-40-012, PGC 55921, CGCG 078-058[1] |
NGC 5988 is a large spiral galaxy in the constellation of Serpens. Its velocity with respect to the cosmic microwave background is 10697 ± 10 km/s, which corresponds to a Hubble distance of 514.6 ± 36.0 Mly (157.78 ± 11.05 Mpc).[1] However, one non-redshift measurement gives a much larger distance of 668.62 Mly (205.000 Mpc).[2] It was discovered by American astronomer Lewis Swift on 17 April 1887.[3]
NGC 5988 is 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.[4]
One supernova has been observed in NGC 5988: SN 2023hbv (type II, mag 19.278) was discovered by ATLAS on 29 April 2023.[5]