Edge Rewrite
// 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: a254c8b3ee57bd4a

Jump to content

// Workers AI · dad joke modeWhat did NGC 444 say to NGC 445? You're one galaxy ahead.

From Wikipedia, the free encyclopedia

NGC 444
NGC 444
NGC 444 as seen by 2MASS
Observation data (J2000 epoch)
ConstellationPisces
Right ascension01h 15m 49.6s[1]
Declination+31° 04 49[1]
Redshift0.016141[1]
Heliocentric radial velocity4,839 km/s[1]
Distance172.16 ± 23.24 Mly (52.785 ± 7.126 Mpc)[1]
Apparent magnitude (V)15.02[1]
Absolute magnitude (V)-21.11[1]
Characteristics
TypeSd[1]
Apparent size (V)1.9' × 0.4'[1]
Other designations
UGC 810, CGCG 502-015, MCG +05-04-007, 2MASX J01154958+3104488, 2MASXi J0115495+310448, PGC 4561, IC 1658.[1]

NGC 444 is a spiral galaxy of type Sd located in the constellation Pisces. It was first discovered on October 26, 1854 by R. J. Mitchell (and later listed as NGC 444), and was also spotted on October 17, 1903 by Stéphane Javelle (and later listed as IC 1658). It was described by Dreyer as "very faint, much extended 135°, a little brighter middle."[2]

Image taken by SDSS.

References

[edit]
  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 0431. Retrieved September 2, 2016.
  2. "New General Catalog Objects: NGC 400 - 449". Cseligman. Retrieved April 22, 2017.
[edit]
  • Wikimedia Commons logo Media related to NGC 444 at Wikimedia Commons
  • NGC 444 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images