Share to: share facebook share twitter share wa share telegram print page

NGC 3455

NGC 3455
NGC 3455 spiral galaxy taken by Hubble Space Telescope.
Observation data (J2000 epoch)
ConstellationLeo
Right ascension10h 54m 31.066s[1]
Declination+17° 17′ 04.59″[1]
Redshift0.003730[1]
Heliocentric radial velocity1117[1]
Distance65 million ly
Apparent magnitude (B)13.1[1]
Characteristics
TypeSABb[1]
Other designations
MCG+03-28-031, Z 95-62, [M98c] 105151.6+173308, IRAS 10518+1733, PSCz Q10518+1733, Z 1051.9+1733, [T76] 25B, KPG 257b, QDOT B1051512+173306, [BEC2010] HRS 30, LEDA 32767, UGC 6028, [CHM2007] HDC 632 J105431.06+1717045, 2MASX J10543106+1717045, UZC J105431.1+171704, [CHM2007] LDC 778 J105431.06+1717045

NGC 3455 is an intermediate spiral galaxy located 65 million light-years away in the constellation of Leo.[2] It is a member of the NGC 3370 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.[3]

References

  1. ^ a b c d e f "Object query : NGC 3455". Astronomical Database. SIMBAD. Retrieved 16 April 2014.
  2. ^ "Galaxies spiralling around Leo". ESA/Hubble Picture of the Week. Retrieved 16 April 2014.
  3. ^ "The Leo III Groups". Atlas of the Universe. Archived from the original on July 22, 2012. Retrieved 2010-11-27.
  • Media related to NGC 3455 at Wikimedia Commons



Stub icon

This spiral galaxy article is a stub. You can help Wikipedia by expanding it.
Kembali kehalaman sebelumnya