NGC772, AlBroxton

NGC772

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Description

NGC772 (also known as Arp 78) is an unbarred spiral galaxy approximately 130 million light-years away in the constellation Aries. It is notable for possessing a single elongated outer spiral arm, which has likely arisen due to tidal interactions with nearby galaxies. At around 100,000 light years in diameter, NGC772 rivals the Milky Way Galaxy in size and is surrounded by several satellite galaxies including the dwarf elliptical, NGC770. Two supernovae (SN 2003 hl & SN 2003 iq) have been observed in NGC772. In a distance of some 130 Mio LY the galaxy appears rather bright at 10m3 in the night skies for a visual observer. The apparent size of 772 measures about 7.2 by 4.3 arc minutes which makes it a worthwhile target in a moderate telescope. Discovered on 27th of November 1785 by William Herschel 2 Supernovas have been observed ever since - photographically of course. These 2 SN showed up in 2003 - the image cannot reveal any sign of those SNs - too much time has passed meanwhile, and the remnants cannot be observed from earth any longer.

What makes that elliptical galaxy NGC 770 really special is its counter rotating core, which was described by professional astronomers in June 2005.

Comments

Revisions

  • NGC772, AlBroxton
    Original
  • NGC772, AlBroxton
    B
  • NGC772, AlBroxton
    C
  • Final
    NGC772, AlBroxton
    D

Histogram

NGC772, AlBroxton

In these collections

Allen Broxton
Galaxies