NGC 2509

Last updated
NGC 2509
NGC 2509 DSS.jpg
DSS image of NGC 2509
Observation data (J2000 epoch)
Right ascension 08h 00m 48s [1]
Declination −19° 03 06 [1]
Distance 9,500 ly (2,900 pc [1] )
Apparent magnitude  (V)9.3 [2]
Apparent dimensions (V)2.5 ± 0.5
Physical characteristics
Estimated age1,200 Myr [1]
Other designations NGC 2509, Cr 171, Mel 81, OCl 630 [2]
Associations
Constellation Puppis
See also: Open cluster, List of open clusters

NGC 2509 is an open cluster in the constellation of Puppis. It was discovered on 3 December 1783 by William Herschel. [3] It was described as "bright, pretty rich, slightly compressed" by John Louis Emil Dreyer, the compiler of the New General Catalogue. [3]

The cluster is about 14 light-years (4.2 parsecs) wide, [1] but the cluster's other parameters remain poorly known. Some studies have estimated a distance of about 9,500 light-years (2,900 parsecs) away from the Solar System, [1] while older estimates put it at only 2980 light-years (912 parsecs) away. [4] Estimates of the cluster's age have also varied significantly, from 1.2 billion years old [1] to 8 billion years old. [4] The latest analysis based on the parallaxes measured by the Gaia spacecraft confirms that it is a relatively distant object, with a distance between 2500 and 3000 parsecs. [5]

References

  1. 1 2 3 4 5 6 7 Carraro, G.; Costa, E. (2007). "Photometry of the five marginally studied open clusters Collinder 74, Berkeley 27, Haffner 8, NGC 2509, and VdB-Hagen 4". Astronomy & Astrophysics. 464 (2): 573. arXiv: astro-ph/0611705 . Bibcode:2007A&A...464..573C. doi:10.1051/0004-6361:20066350. S2CID   1419651.
  2. 1 2 "NGC 2509". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 9 August 2017.
  3. 1 2 "New General Catalog Objects: NGC 2500 - 2549". cseligman.com. Retrieved 9 August 2017.
  4. 1 2 Sujatha, S.; Babu, G. S. D. (2003). "Study of open cluster NGC 2509". Bulletin of the Astronomical Society of India. 31: 9–18. Bibcode:2003BASI...31....9S.
  5. Cantat-Gaudin, T.; Jordi, C.; Vallenari, A.; et al. (2018). "A Gaia DR2 view of the open cluster population in the Milky Way". Astronomy & Astrophysics. 618: A93. arXiv: 1805.08726 . Bibcode:2018A&A...618A..93C. doi:10.1051/0004-6361/201833476. S2CID   56245426.