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Messier 47
Open cluster Messier 47 in Puppis
Credit: NOIRLab / NSF / AURA
Observation data (J2000.0 epoch)
Right ascension07h 36.6m [1]
Declination−14° 30′[1]
Distance498 pc[1]
Apparent magnitude (V)4.4[2]
Apparent dimensions (V)30′[2]
Physical characteristics
Mass453[1] M☉
Radius10.61 pc[1]
Estimated age78 million years
Other designationsNGC 2422, NGC 2478, Cr 152
Associations
See also: Open cluster, List of open clusters

Messier 47 (M47 or NGC 2422) and also known as NGC 2478[3] is an open cluster in the mildly southern constellation of Puppis. It was discovered by Giovanni Batista Hodierna before 1654 and in his then keynote work re-discovered by Charles Messier on 1771.[a] It was also independently discovered by Caroline Herschel.

There is no cluster in the position indicated by Messier, which he expressed in terms of its right ascension and declination with respect to the star 2 Puppis. However, if the signs (+ and −) he wrote are swapped, the position matches.[4] Until this equivalency was found, M47 was considered a lost Messier Object. This identification as the same thing (ad idem) only came in 1959 with a realization by Canadian astronomer T. F. Morris.[5]

M47 is centered about 1,600 light-years away and is about 78 million years old. The member stars have been measured down to about red dwarfs at apparent magnitude 19. There are around 500 members,[1] the brightest being HD 60855, a magnitude 5.7 Be star. The cluster is dominated by hot class B main sequence and giant stars, but a noticeable colour contrast comes from its brightest red giants.[5]

It about a degree from Messier 46, which is much older and much further away.[5]

  • Image of star cluster Messier 47 taken using the Wide Field Imager camera, installed on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile.
    Image of star cluster Messier 47 taken using the Wide Field Imager camera, installed on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile.

See also

References and footnotes

  1. ^ a b c d e f Prisinzano, L; Micela, G; Sciortino, S; Favata, F (2003). "Luminosity and Mass Function of the Galactic open cluster NGC 2422". Astronomy & Astrophysics. 404 (3): 927–938. arXiv:astro-ph/0304321. Bibcode:2003A&A...404..927P. doi:10.1051/0004-6361:20030524. S2CID 14697851.
  2. ^ a b Stoyan, Ronald (2008). Atlas of the Messier Objects: Highlights of the Deep Sky. Cambridge University Press. p. 195. ISBN 978-0521895545.
  3. ^ "NGC/IC Project Restoration Efforts". ngcicproject.observers.org. Retrieved 2024-08-02.
  4. ^ Houston, Walter Scott (2005). Deep-Sky Wonders. Sky Publishing Corporation. ISBN 978-1-931559-23-2.
  5. ^ a b c "The hot blue stars of messier 47". ScienceDaily. 17 December 2014.
  1. ^ on February 19


source: https://en.wikipedia.org/wiki/Messier_47