NGC 355

In this article, we will explore everything related to NGC 355. From its historical origin to its impact on current society, passing through its main characteristics and relevant applications today. NGC 355 has been the subject of great interest and debate in recent years, which has motivated researchers, experts and enthusiasts to further study it. Through this article, we hope to shed light on the most relevant aspects of NGC 355, providing our readers with a complete and up-to-date view of this intriguing and important topic.

NGC 355
SDSS image of NGC 355
Observation data (J2000 epoch)
ConstellationCetus
Right ascension01h 03m 07.0s[1]
Declination−06° 19′ 26″[1]
Redshift0.024217[1]
Heliocentric radial velocity7,260 km/s[1]
Apparent magnitude (V)16.0b[1]
Characteristics
TypeSB0[1]
Apparent size (V)1.0' × 0.4'[1]
Other designations
MCG -01-03-077, 2MASX J01030695-0619252, 2MASXi J0103069-061925, 6dF J0103070-061926, PGC 3753.[1]

NGC 355 is a lenticular galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "extremely faint, very small."[2]

NGC 355 with the other galaxies (SDSS)

References

  1. ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 0355. Retrieved September 2, 2016.
  2. ^ "New General Catalog Objects: NGC 350 - 399". Cseligman. Retrieved November 12, 2016.
  • Media related to NGC 355 at Wikimedia Commons