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NGC 5988

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Galaxy in the constellation Serpens

NGC 5988
The spiral galaxy NGC 5988
Observation data (J2000 epoch)
ConstellationSerpens
Right ascension15 44 33.8559
Declination+10° 17′ 35.33″
Redshift0.035259
Heliocentric radial velocity10,570 ± 4 km/s
Distance514.6 ± 36.0 Mly (157.78 ± 11.05 Mpc)
Apparent magnitude (V)13.8
Characteristics
TypeScd
Size~298,900 ly (91.63 kpc) (estimated)
Apparent size (V)1.2′ × 1.0′
Other designations
IRAS F15421+1026, 2MASX J15443383+1017356, UGC 9998, MCG +02-40-012, PGC 55921, CGCG 078-058

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). However, one non-redshift measurement gives a much larger distance of 668.62 Mly (205.000 Mpc). It was discovered by American astronomer Lewis Swift on 17 April 1887.

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.

One supernova has been observed in NGC 5988: SN 2023hbv (type II, mag 19.278) was discovered by ATLAS on 29 April 2023.

See also

References

  1. ^ "Results for object NGC 5988". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 3 August 2024.
  2. "Distance Results for NGC 5988". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 14 December 2024.
  3. Seligman, Courtney. "New General Catalogue Objects: NGC 5988". Celestial Atlas. Retrieved 14 December 2024.
  4. "NGC 5988". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 15 December 2024.
  5. "SN 2023hbv". Transient Name Server. IAU. Retrieved 15 December 2024.

External links

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