NGC 4700 explained

NGC 4700
Credit:ESA/Hubble & NASA
Epoch:J2000
Constellation Name:Virgo[1]
Ra:[2]
Z:0.00480
H Radial V:1435 km/s
Dist Ly:9.013+/-
Type:SB(s)c[3]
Appmag V:14.32
Appmag B:12.7
Size V:3.09 (major axis)
Names:MGC-02-33-013, PGC 43330

NGC 4700 is a spiral galaxy located about 50 million light years away in the constellation of Virgo. NGC 4700 was discovered in March 1786 by the British astronomer William Herschel who noted it as a "very faint nebula". It is a member of the NGC 4699 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.[4]

NGC 4700 was imaged by the Hubble Space Telescope in 2012, showing an abundance of star-forming regions similar to the Orion Nebula.[1]

Notes and References

  1. News: A Galaxy Festooned with Stellar Nurseries. 23 July 2012. ESA/Hubble Picture of the Week.
  2. Web site: Search results for NGC 4700. Astronomical database. SIMBAD. 23 July 2012.
  3. Web site: NED results for object NGC 4700. 15 February 2017. National Aeronautics and Space Administration / Infrared Processing and Analysis Center.
  4. Web site: The Virgo III Groups . Atlas of the Universe . 2010-11-27 .