NGC 6356

In this article, we will address the topic of NGC 6356, exploring its many facets and its relevance today. NGC 6356 is a topic that has aroused interest and curiosity over time, sparks debate and opinion in various areas and has left its mark on society. Along these lines, we will analyze different perspectives on NGC 6356, delving into its origins, evolution and impact on contemporary culture. From its impact on daily life to its implications in the professional field, NGC 6356 is a vital topic that deserves to be explored in detail and that encourages us to reflect on its influence on our lives.

NGC 6356
NGC 6356 as seen through the Hubble Space Telescope
Observation data (J2000 epoch)
ClassII
ConstellationOphiuchus
Right ascension17h 23m 35.0s
Declination−17° 48′ 47″
Apparent magnitude (V)8.2
Apparent dimensions (V)10.00
Physical characteristics
Absolute magnitude-8.51
Metallicity = -0.4[1] dex
Other designationsGCL 62 and ESO 588-SC1
See also: Globular cluster, List of globular clusters

NGC 6356 is a globular cluster located in the constellation Ophiuchus. It is designated as a II in the Shapley–Sawyer Concentration Class and was discovered by the German-born British astronomer William Herschel on 18 June 1784. The star cluster is more dense and bright towards the middle. NGC 6356 is located 80' north east of the brighter NGC 6333. It is at a distance of 49,600 light years away from Earth.[2][3][4][5][6]

The cluster is relatively metal-rich and therefore has a large amount of interstellar dust in its core.[1]

See also

References

  1. ^ a b Dust in the core of the metal-rich globular cluster NGC 6356
  2. ^ "Object No. 1 - NGC 6356". NASA/IPAC extragalactic database. NASA/IPAC. Retrieved 19 October 2015.
  3. ^ "Revised NGC Data for NGC 6356". Seds. Retrieved 19 October 2015.
  4. ^ "NGC 6356 (= GCL 62)". cseligman. Retrieved 19 October 2015.
  5. ^ "NGC 6356". Seds. Retrieved 19 October 2015.
  6. ^ "The globular cluster NGC 6356". In-the-sky. Retrieved 19 October 2015.
  • Media related to NGC 6356 at Wikimedia Commons