NGC 235

In today's world, NGC 235 has become a topic of great relevance and interest to a wide spectrum of people. Whether due to its impact on society, its historical relevance or its influence in different areas, NGC 235 has captured the attention and curiosity of individuals of all ages and professions. Over the years, NGC 235 has been the subject of debate, analysis and study, generating a large amount of information and opinions about it. In this article, we will explore the different aspects, perspectives and possible implications of NGC 235, addressing its importance from various perspectives and offering a comprehensive view of the topic.

NGC 235
NGC 235
Hubble Space Telescope image of NGC 235
Observation data (J2000 epoch)
ConstellationCetus
Right ascension00h 42m 53.2s[1]
Declination−23° 32′ 36″[1]
Redshift0.022229 [1]
Heliocentric radial velocity6664 km/h [1]
Galactocentric velocity6674 km/h [1]
Distance78.3 ± 5.5 Mpc (255.6 ± 20.9 Mly) [1]
Apparent magnitude (V)14.5 [1]
Characteristics
TypeS0/(r)a? pec [2]
Size120 kly across
Apparent size (V)1.3' x 0.7'
Other designations
ESO 352-IG 066, ESO 012138-3519.7, PGC 5120 [1]

NGC 235 is a lenticular galaxy in the constellation of Cetus. Its companion, PGC 2570, appears in the line of sight of NGC 235, but has no relation with NGC 235. This pair was first discovered by Francis Leavenworth in 1886. Dreyer, the compiler of the catalogue, described the galaxy as "extremely faint, small, round, brighter middle and nucleus".[2]

References

  1. ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 235. Retrieved 2015-09-05.
  2. ^ a b "New General Catalogue Objects: NGC 200-249". Retrieved 2015-09-04.
  • Media related to NGC 235 at Wikimedia Commons