NGC 600 explained

NGC 600
Epoch:J2000
Constellation Name:Cetus
Z:0.006144 ± 0.000003[1]
H Radial V:1842 km/s
Group Cluster:[CHM2007] HDC 81,[2] [T2015] nest 200207[3]
Type:(R')SB(rs)d
Appmag V:12.5±0.1
Appmag B:13.1[4]
Absmag V:-15.69
References:[5]

NGC 600 is an emission-line galaxy[4] in the constellation Cetus. It was discovered by William Herschel on 10 September 1785.[6] The galaxy has a diameter of 70,000 light-years. It is also approximately 90 million light-years from the Milky Way.[1]

See also

Notes and References

  1. Web site: Your NED Search Results. ned.ipac.caltech.edu. 2020-07-21.
  2. [CHM2007] HDC 81. 2020-07-21.
  3. [T2015] nest 200207. 2020-07-21.
  4. NGC 600. 2020-07-21.
  5. Web site: The galaxy NGC 600 - In-The-Sky.org. Dominic. Ford. in-the-sky.org.
  6. Web site: New General Catalogue objects: NGC 600 - 649. Seligman, Courtney. cseligman.com. 2020-07-21.