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NGC 2362 information


NGC 2362
NGC 2362 in Canis Major
Observation data (J2000 epoch)
Right ascension07h 18m 41.0s[1]
Declination−24° 57′ 18″[1]
Distance4.83 ± 0.97 kly (1.480 ± 0.296 kpc)[1]
Apparent magnitude (V)3.8[2]
Apparent dimensions (V)6′[2]
Physical characteristics
Mass≥500[3] M
Radius~3 pc[4]
Estimated age5.0 Myr[1]
Other designationsCaldwell 64, Cr 136[5]
Associations
ConstellationCanis Major
See also: Open cluster, List of open clusters

NGC 2362, also known as Caldwell 64, is an open cluster of stars in the southern constellation of Canis Major. It was discovered by the Italian court astronomer Giovanni Batista Hodierna, who published his finding in 1654.[4] William Herschel called it a "beautiful cluster", while William Henry Smyth said it "has a beautiful appearance, the bright white star being surrounded by a rich gathering of minute companions, in a slightly elongated form, and nearly vertical position". In the past it has also been listed as a nebula, but in 1930 Robert J. Trumpler found no evidence of nebulosity.[6] The brightest member star system is Tau Canis Majoris, and therefore it is sometimes called the Tau Canis Majoris Cluster.

The cluster is located at a distance of approximately 1.48 kpc from the Sun,[1] and appears associated with the giant nebula Sh2-310 that lies at the same distance,[7] about one degree to the east. This giant H II region is being ionized by the brighter members of the NGC 2362 cluster.[4]

NGC 2362 is a relatively young 4–5 million years in age[3] but is devoid of star-forming gas and dust, indicating that the star formation process has come to a halt.[4] It is a massive open cluster, with more than 500 solar masses,[3] an estimated 100-150 member stars, and an additional 500 forming a halo around the cluster. Of these cluster members, only around 35 show evidence of a debris disk.[3] There is one slightly evolved O-type star, Tau Canis Majoris, and around 40 B-type stars still on the main sequence. Only one candidate classical Be star has been found, as of 2005.[4]

  1. ^ a b c d e Cite error: The named reference Wu2009 was invoked but never defined (see the help page).
  2. ^ a b Cite error: The named reference Finlay2006 was invoked but never defined (see the help page).
  3. ^ a b c d Cite error: The named reference Currie2009 was invoked but never defined (see the help page).
  4. ^ a b c d e Cite error: The named reference Dahm2008 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference OMeara2002 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference VY was invoked but never defined (see the help page).

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NGC 2362

Last Update:

NGC 2362, also known as Caldwell 64, is an open cluster of stars in the southern constellation of Canis Major. It was discovered by the Italian court astronomer...

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Tau Canis Majoris

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brightest member of the open cluster NGC 2362. τ Canis Majoris lies at the center of the very young open cluster NGC 2362 which contains several hundred stars...

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VY Canis Majoris

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that of the stars, which are members of the open cluster NGC 2362, that ionize the rim. NGC 2362 could be anywhere in the ranges of 1.5±0.5 kiloparsecs...

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Canis Major

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stars are only a few million years old. Lying 2 degrees southwest of NGC 2362 is NGC 2354 a fainter open cluster of magnitude 6.5, with around 15 member...

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NGC 2354

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NGC 2354 is an open cluster in the constellation Canis Major. It lies 2 degrees southwest from NGC 2362 and northeast of Delta Canis Majoris. About 15...

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NGC 7609

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NGC 7609 or known as Arp 150 and HCG 95A, is a large elliptical galaxy located in Pegasus. Its speed relative to the cosmic microwave background is 11...

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UW Canis Majoris

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distance of around 3,800 light years. It is thought to be a distant member of NGC 2362 which would place it about 5,000 light years and more closely match its...

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Open cluster

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he identified the objects now designated Messier 41, Messier 47, NGC 2362 and NGC 2451. It was realized as early as 1767 that the stars in a cluster...

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Caldwell catalogue

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objects, such as the Hyades, the Double Cluster (NGC 869 and NGC 884), and the Sculptor Galaxy (NGC 253). The Messier catalogue was actually compiled...

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Vela Molecular Ridge

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region Sh2-310 can be found in which it was formed the massive open cluster NGC 2362. The Vela Molecular Ridge is a nebulous complex composed of several giant...

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List of most massive stars

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massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region". Astronomy & Astrophysics. 456 (2): 623–638...

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List of open clusters

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of Gas Giant Planet Formation: A Spitzer Study of the 5 Myr Old Cluster NGC 2362". The Astrophysical Journal. 698 (1): 1–27. arXiv:0903.2666. Bibcode:2009ApJ...

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List of most luminous stars

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massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region". Astronomy & Astrophysics. 456 (2): 623–638...

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NGC 2546

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photoelectric investigation of Ap-stars in open clusters. III - NGC 2362, NGC 2546, and NGC 3228". Astronomy and Astrophysics. 115 (2): 275–279. Bibcode:1982A&A...

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Herschel 400 Catalogue

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II Program. The catalogue contains 400 objects. All objects are from the NGC. All objects are visible in mid northern latitudes, since they were all observed...

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NGC 2169

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NGC 2169 is an open cluster in the Orion constellation. It was possibly discovered by Giovanni Batista Hodierna before 1654 and discovered by William...

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New General Catalogue

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of Stars (abbreviated NGC) is an astronomical catalogue of deep-sky objects compiled by John Louis Emil Dreyer in 1888. The NGC contains 7,840 objects...

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Melotte catalogue

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2020-06-26. "ngc 1857". sim-id. Retrieved 2020-06-26. "ngc 2192". sim-id. Retrieved 2020-06-26. "ngc 2215". sim-id. Retrieved 2020-06-26. "ngc 2243". sim-id...

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NGC 2264

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NGC 2264 is the designation number of the New General Catalogue that identifies two astronomical objects as a single object: the Cone Nebula, and the...

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List of stars in Canis Major

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35415 07h 18m 42.49s −24° 57′ 15.8″ 4.37 −5.59 3196 O9Ib member of the NGC 2362 star cluster; β Lyr variable ν3 CMa ν3 8 47442 31700 06h 37m 53.43s −18° 14′ 14...

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List of NGC objects

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galaxies. List of NGC objects (1–1000) List of NGC objects (1001–2000) List of NGC objects (2001–3000) List of NGC objects (3001–4000) List of NGC objects (4001–5000)...

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NGC 2349

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(SIMBAD 2007) harv error: no target: CITEREFSIMBAD2007 (help) NGC 2349 @ SEDS NGC objects pages NGC 2349 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray...

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Rosette Nebula

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confused with NGC 246, which is also nicknamed the "Skull Nebula." The complex has the following New General Catalogue (NGC) designations: NGC 2237 – Part...

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Collinder catalogue

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Embedded within Messier 24. Associated with Messier 17. Associated with NGC 6820. Embedded within the Iris Nebula. There are some errors in Collinder's...

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Messier 78

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Messier 78 or M78, also known as NGC 2068, is a reflection nebula in the constellation Orion. It was discovered by Pierre Méchain in 1780 and included...

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NGC 2003

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NGC 2003 (also known as PGC 3518064, ESO 086-SC006 and SL 526) is a globular cluster located in the Dorado constellation and is part of the Large Magellanic...

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NGC 2175

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Open Cluster NGC 2175 (also known as OCL 476 or Cr 84) is an open cluster in the Orion constellation, embedded in a diffusion nebula. It was discovered...

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NGC 2359

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NGC 2359 (also known as Thor's Helmet) is an emission nebula in the constellation Canis Major. The nebula is approximately 3,670 parsecs (11.96 thousand...

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