NGC 220

In today's article we are going to delve into the exciting world of NGC 220. From its origins to its relevance today, we will explore every facet of this topic/topic/person. We will discover its most relevant aspects, its impact on society and possible future implications. Through a detailed and rigorous analysis, we will delve into its multiple dimensions, examining both its positive aspects and the challenges it presents. NGC 220 is a topic of great relevance today and through this article we will try to offer a global and complete vision that allows the reader to understand its importance and evolution over time. Don't miss this exciting journey through the fascinating world of NGC 220!

NGC 220
NGC 220 (lower right), NGC 222 (middle) and NGC 231 (upper left) with DECam
Observation data (J2000 epoch)
Right ascension00h 40m 29.9s[1]
Declination−73° 24′ 14″[1]
Distance210000 ly
Apparent magnitude (V)14.39[2]
Apparent dimensions (V)1.20′ × 1.20′[2]
Physical characteristics
Mass7.9×103[3] M☉
Estimated age120 Myr[3]
Other designationsESO 029-SC 003.[1]
Associations
ConstellationTucana
See also: Open cluster, List of open clusters

NGC 220 is an open cluster located approximately 210,000 light-years from the Sun in the Small Magellanic Cloud. It is located in the constellation Tucana. It was discovered on August 12, 1834 by John Herschel.[4]

See also

References

  1. ^ a b c "NASA/IPAC Extragalactic Database". Results for NGC 0220. Retrieved 2016-09-02.
  2. ^ a b "NGC 220". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 31 December 2016.
  3. ^ a b Gatto, M.; Ripepi, V.; Bellazzini, M.; Tosi, M.; Cignoni, M.; Tortora, C.; Leccia, S.; Clementini, G.; Grebel, E. K.; Longo, G.; Marconi, M.; Musella, I. (2021). "STEP survey – II. Structural analysis of 170 star clusters in the SMC". Monthly Notices of the Royal Astronomical Society. 507 (3): 3312–3330. arXiv:2108.02791. doi:10.1093/mnras/stab2297.
  4. ^ "New General Catalog Objects: NGC 200 - 249". Cseligman. Retrieved September 10, 2016.