NGC 1647 explained

NGC 1647
Type:Open Cluster
Epoch:J2000
Constellation:Taurus
Ra:[1]
Dist Ly:1,800 ly (on average)
Dist Pc:550 ps[2]
Appmag V:6.4
Size V:45'
Names:Cr 54

NGC 1647 is an open cluster in the constellation Taurus. It contains nearly 90 stars and it lies at a distance of 550 parsec.[2] It is visible even with binoculars close to Aldebaran. It was discovered by William Herschel in 1784.[3] It is located behind the Taurus dark nebula complex, approximately 160 parsec away. The brightest main sequence stars are of spectral type B7. Its age is estimated to be 150 million years.[4]

Notes and References

  1. NGC 1647. 2015-06-19.
  2. C. A. Guerrero . J. H. Peña . J. P. Sareyan . uvby-B Photoelectric Photometry of the Open Clusters NGC 1647 and NGC 1778. Revista Mexicana de Astronomía y Astrofísica. 2011. 47. 1. 185–192. 19 June 2015. 2011RMxAA..47..185G .
  3. http://www.ngcicproject.org/ngcicdb.asp NGC/IC online - result for NGC 1647
  4. 6. Zdanavičius, J.. Straižys, V.. Chen, C. W.. Chen, W. P.. Zdanavičius, K.. Kazlauskas, A.. Černis, K.. Philip, A. G. D.. Boyle, R. P.. Tautvaišienė, G.. Seven-Color Photometry of the Open Cluster NGC 1647 Area. Baltic Astronomy. 2005. 14. 179–203. 2005BaltA..14..179Z .