NGC 444 explained

NGC 444
Upright:1.35
Epoch:J2000
Ra:[1]
Constellation Name:Pisces
Z:0.016141
H Radial V:4,839 km/s
Dist Ly:52.785+/-
Type:Sd
Appmag V:15.02
Absmag V:-21.11
Size V:1.9' × 0.4'
Names:UGC 810, CGCG 502-015, MCG +05-04-007, 2MASX J01154958+3104488, 2MASXi J0115495+310448, PGC 4561, IC 1658.

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]

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 0431 . September 2, 2016.
  2. Web site: New General Catalog Objects: NGC 400 - 449. Cseligman. April 22, 2017.