Edge Rewrite
everything Source code View original
// HTMLRewriter · presentation

This page was redesigned at the edge.

Cloudflare fetched the original article and streamed it through HTMLRewriter to apply an entirely new visual system without rebuilding the source page.

// request.cf · coarse context

A page that knows where it met you.

Only coarse request metadata is shown. This demo does not display or persist visitor IP addresses.

Country
US
Cloudflare location
CMH
Connection
HTTP/2
Language
Not provided

Ray ID: a2321edb1d4eaddf

Jump to content

// Workers AI · dad joke modeWhat did NGC 474 say to NGC 473? You're a galaxy behind.

Coordinates: Sky map 01h 20m 06.6862s, +03° 24′ 55.809″
From Wikipedia, the free encyclopedia
(Redirected from UGC 864)
NGC 474
NGC 474 imaged by the Hubble Space Telescope
Observation data (J2000[1] epoch)
ConstellationPisces[2]
Right ascension01h 20m 06.6862s[1]
Declination+03° 24′ 55.809″[1]
Redshift0.007722[1]
Heliocentric radial velocity2315 km/s ±5 km/s[1]
Galactocentric velocity2398 km/s ±7 km/s[1]
Distance~100 Mly (~31 Mpc)[2]
Apparent magnitude (V)12.37[1]
Characteristics
TypeS0[3]
Size250,000 ly (diameter)[4]
Apparent size (V)7.1′ × 6.3′[1]
Other designations
ZWG 385.71, 2MASX J01200669+0324549, Arp 227, UGC 864, MCG +00-04-085, PGC 4801, CGCG 385-071[1][3]

NGC 474 is a large lenticular galaxy in the constellation Pisces. Its velocity with respect to the cosmic microwave background is 2,001±23 km/s, which corresponds to a Hubble distance of 96.2 ± 6.8 Mly (29.51 ± 2.09 Mpc).[1] Additionally, 13 non-redshift measurements give a similar mean distance of 91.50 ± 6.69 Mly (28.054 ± 2.050 Mpc).[5] It was discovered by German-British astronomer William Herschel on 13 December 1784.[6][7]

NGC 474 is known to possess tidal shells[8] and tidal tails, although their origins remain unclear.[2] One possible explanation is that NGC 474 interacted with a galaxy several billion years ago.[9]

Structure

[edit]

The origins of the spectacular tidal features around NGC 474 have been extensively studied, and some possible explanations have been published. The authors of one study argued that the tidal tails were formed because of a collision with a galaxy 2 billion years ago.[9] The same study also stated that NGC 474 is absorbing gas from its neighbor, NGC 470, since the ancient collision.[9] In another model, the tidal shells can be explained by a gas-rich spiral galaxy colliding with NGC 474 twice, before finally merging.[8] NGC 474 is moving away from the Sun at a rate of 2412 km/s due to dark energy.[10]

NGC 474's (right) tidal tails and shell-like structures may be from collision(s) with another galaxy. A neighboring spiral galaxy, NGC 470, is on the left.

Supernova

[edit]

One supernova has been observed in NGC 474: SN 2017fgc (Type Ia, mag. 17.3239) was discovered by the Distance Less Than 40 Mpc Survey (DLT40) on 11 July 2017.[11] It was located at a considerable distance (~18.90±0.01 kpc)[12] from the galactic nucleus.[13]

See also

[edit]

Further reading

[edit]

References

[edit]
  1. 1 2 3 4 5 6 7 8 9 10 "Results for object NGC 0474". NASA/IPAC Extragalactic Database. Retrieved 2026-07-12.
  2. 1 2 3 Schirmer, Mischa. "NGC 474". Archived from the original on 2011-06-29. Retrieved 2011-02-26.
  3. 1 2 "Revised NGC Data for NGC 474". The Interactive NGC Catalog Online. Retrieved 2011-02-26.
  4. ↑ "Galaxy NGC 474". NASA Astronomy Picture of the Day. Retrieved 2018-02-07.
  5. ↑ "Distance Results for NGC 0474". NASA/IPAC Extragalactic Database. NASA. Retrieved 12 July 2026.
  6. ↑ Herschel, William (1786). "Catalogue of One Thousand New Nebulae and Clusters of Stars" (PDF). Philosophical Transactions of the Royal Society of London. 76: 457–499. Bibcode:1786RSPT...76..457H. doi:10.1098/rstl.1786.0027.
  7. ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 474". Celestial Atlas. Retrieved 12 July 2026.
  8. 1 2 Bílek, Michal; Fensch, Jérémy; Ebrová, Ivana; Nagesh, Srikanth T.; Famaey, Benoit; Duc, Pierre-Alain; Kroupa, Pavel (2022). "Origin of the spectacular tidal shells of galaxy NGC 474". Astronomy & Astrophysics. 660: A28. arXiv:2111.14886. Bibcode:2022A&A...660A..28B. doi:10.1051/0004-6361/202141709. S2CID 244729604.
  9. 1 2 3 Alabi, A.B.; Anna, F-M.; Forbes, D.A.; Romanowsky, A.J.; Brodie, J.P. (September 2020). "NGC 474 as viewed with KCWI: diagnosing a shell galaxy". Monthly Notices of the Royal Astronomical Society. 497 (1): 626–631. arXiv:2007.01870. doi:10.1093/mnras/staa1992.
  10. ↑ Guide, Universe. "NGC 474 - Facts about the Galaxy in Pisces". Universe Guide. Retrieved 2022-05-20.
  11. ↑ "SN 2017fgc". Transient Name Server. IAU. Retrieved 18 March 2026.
  12. ↑ Zeng, Xiangyun; et al. (2021). "SN 2017fgc: A Fast-expanding Type Ia Supernova Exploded in Massive Shell Galaxy NGC 474". The Astrophysical Journal. 919 (1): 49. arXiv:2106.12164. Bibcode:2021ApJ...919...49Z. doi:10.3847/1538-4357/ac0e9c.
  13. ↑ King, Bob (2017-07-26). "Sky Surprises: New Comet ASASSN1, Nova in Scutum, and Supernova in Pisces!". Sky & Telescope.
[edit]
  • Wikimedia Commons logo Media related to NGC 474 at Wikimedia Commons
  • Galaxy NGC 474: Cosmic Blender, NASA Astronomy Picture of the Day (8 October 2007)
  • Shell Galaxies in Pisces, NASA Astronomy Picture of the Day (27 February 2011)
  • Galaxy NGC 474: Shells and Star Streams, NASA Astronomy Picture of the Day (5 January 2014)
  • Galaxy NGC 474: Shells and Star Streams, NASA Astronomy Picture of the Day (6 February 2018)
  • Galaxy NGC 474: Shells and Star Streams, NASA Astronomy Picture of the Day (July 12, 2026)
Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_474&oldid=1364446150"