Astronomy:NGC 2301

From HandWiki
NGC 2301
File:300px
NGC 2301 imaged by Chandra X-ray Observatory
Observation data (J2000 epoch)
ConstellationMonoceros[1]
Right ascension 06h 51m 45s[2]
Declination+00° 27′ 36″[2]
Distance2,840 ly (872 pc)[3]
Apparent magnitude (V)6.0[1]
Apparent dimensions (V)12′[1]
Physical characteristics
Estimated age165 million years old
Other designationsCr 119
See also: Open cluster, List of open clusters

NGC 2301 is an open cluster of stars in the constellation of Monoceros.[1] It was discovered by German-English astronomer William Herschel in 1786. This formation is visible through 7x50 binoculars and it is considered the best open cluster for small telescopes in the constellation.[4] It is located 5° WNW of Delta Monocerotis and 2° SSE of 18 Monocerotis. The brightest star of the cluster is an orange G8 subgiant star of 8.0 magnitude, but it is possible that it is a foreground star. The cluster contains also blue giants. The brightest main sequence star is a B9 star with magnitude 9.1.[5]

References

  1. ↑ 1.0 1.1 1.2 1.3 Finlay, Warren H. (2014). Concise Catalogue of Deep-Sky Objects. The Patrick Moore Practical Astronomy Series (2nd ed.). Springer Cham. p. 200. doi:10.1007/978-3-319-03170-5. ISBN 978-3-319-03169-9. 
  2. ↑ 2.0 2.1 "SIMBAD Astronomical Database". Results for NGC 2301. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+2301&submit=SIMBAD+search. 
  3. ↑ WEBDA: NGC 2301
  4. ↑ Steve O'Meara's Herschel 400 Observing Guide p. 55
  5. ↑ Craig Crossen; Gerald Rhemann (2012). Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes. Springer Science & Business Media. p. 110. ISBN 9783709106266. https://books.google.com/books?id=3vELBwAAQBAJ&pg=PA110. Retrieved 30 October 2015. 

Template:NGC objects:2000-2499