NGC 4414


NGC 4414, also known as the Dusty Spiral Galaxy, is an unbarred spiral galaxy about 62 million light-years away in the constellation Coma Berenices. It was discovered by German-British astronomer William Herschel on 13 March 1785.
NGC 4414 is a flocculent spiral galaxy, with short segments of spiral structure but without the dramatic well-defined spiral arms of a grand design spiral.
The galaxy was imaged by the Hubble Space Telescope in 1995, as part of the HST's main mission to determine the distance to galaxies, and again in 1999 as part of the Hubble Heritage project. It has been part of an ongoing effort to study its Cepheid variable stars. The outer arms appear blue due to the continuing formation of young stars and include a possible luminous blue variable with an absolute magnitude of −10.
NGC 4414 is also an isolated galaxy without signs of past interactions with other galaxies and despite not being a starburst galaxy shows a high density and richness of gas – both atomic and molecular, with the former extending far beyond its optical disk.
NGC 4414 is a member of the Coma I Group, a group of galaxies lying physically close to the Virgo Cluster.

Supernovae

Four supernovae have been observed in NGC 4414:
  • SN 1974G was discovered by Miss W. Burgat on 20 April 1974.
  • SN 2013df was discovered by the Italian Supernovae Search Project on 7 June 2013.
  • SN 2021J was discovered by the Automatic Learning for the Rapid Classification of Events on 1 January 2021.
  • SN 2023hlf was discovered by the Zwicky Transient Facility on 1 May 2023.

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