NGC 4475

Wikipedia

NGC 4475
NGC 4475 imaged by SDSS
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 29m 47.5825s[1]
Declination+27° 14 36.039[1]
Redshift0.024660±0.000005[1]
Heliocentric radial velocity7,393±1 km/s[1]
Distance327.60 ± 10.87 Mly (100.442 ± 3.334 Mpc)[1]
Apparent magnitude (V)14.3g[1]
Characteristics
TypeSAbc[1]
Size~190,600 ly (58.43 kpc) (estimated)[1]
Apparent size (V)1.65′ × 0.87′[1]
Other designations
UGC 7632, MCG +05-30-008, PGC 41225, CGCG 159-008[1]

NGC 4475 is a spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 7,681±20 km/s, which corresponds to a Hubble distance of 369.5 ± 25.9 Mly (113.29 ± 7.94 Mpc).[1] However, 12 non-redshift measurements give a closer mean distance of 327.60 ± 10.87 Mly (100.442 ± 3.334 Mpc).[2] It was discovered by German-British astronomer William Herschel on 11 April 1785.[3][4]

Supernovae

Two supernovae have been observed in NGC 4475:

See also

References

  1. 1 2 3 4 5 6 7 8 9 10 11 "Results for object NGC 4475". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 27 August 2025.
  2. "Distance Results for NGC 4475". NASA/IPAC Extragalactic Database. NASA. Retrieved 27 August 2025.
  3. Herschel, William (1789). "Catalogue of a Second Thousand of New Nebulae and Clusters of Stars; with a Few Introductory Remarks on the Construction of the Heavens". Philosophical Transactions of the Royal Society of London. 79: 212–255. Bibcode:1789RSPT...79..212H. doi:10.1098/rstl.1789.0021.
  4. Seligman, Courtney. "New General Catalogue Objects: NGC 4475". Celestial Atlas. Retrieved 27 August 2025.
  5. "SN 2021acnd". Transient Name Server. IAU. Retrieved 27 August 2025.
  6. "SN 2025nat". Transient Name Server. IAU. Retrieved 27 August 2025.
  • Media related to NGC 4475 at Wikimedia Commons
  • NGC 4475 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images