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NGC 1624

NGC 1624, also known as Sh2-212[3] in the Sharpless catalog, is a very young open cluster in the constellation Perseus inside an emission nebula. It was discovered by German-British astronomer William Herschel in 1790.[4] NGC 1624 is about 20,000 ly (6,000 pc) from Earth, and latest estimates give it an age of less than 4 million years.[2] Its apparent magnitude is 11.8,[1] and apparent diameter is about 3.0 arc minutes.[4] Its celestial location is right ascension (α) 04h 40m 36.0s and declination (δ) +50° 27′ 42″.[1] It is potentially an area of massive star formation.[5]

NGC 1624
Image of NGC 1624 with the Isaac Newton Telescope
Credit: IGAPS
Observation data (J2000 epoch)
Right ascension04h 40m 36.0s[1]
Declination+50° 27′ 42″[1]
Distance20000 ± 2000 ly (6000 ± 600 pc[2])
Apparent magnitude (V)11.8[1]
Physical characteristics
Estimated age<4 Myr[2]
Other designationsCr 53, C 0436+503, OCl 403, Tribble Nebula
Associations
ConstellationPerseus
See also: Open cluster, List of open clusters

According to Robert Trumpler's classification of open clusters, this cluster contains fewer than 50 stars (letter p) with a high concentration (I) and whose magnitudes are distributed over an average interval (number 2). The letter n at the end (I2pn) means that the cluster is inside a nebula.

Along with nearby emission nebula Sh2-211[6] it makes up what has become known as the Tribble Nebulae,[7] so called because they look like the furry creatures first introduced in the Star Trek episode "The Trouble with Tribbles".

Gallery edit

References edit

  1. ^ a b c d e "NGC 1624". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 9 November 2017.
  2. ^ a b c "Sejong Open Cluster Survey (SOS) - IV. The Young Open Clusters NGC 1624 and NGC 1931". SIMBAD. Centre de données astronomiques de Strasbourg.
  3. ^ "Sh2-212". Galaxy Map. Retrieved 16 November 2021.
  4. ^ a b Seligman, Courtney. "New General Catalogue objects: NGC 1600 - 1649". cseligman.com. Retrieved 9 November 2017.
  5. ^ Deharveng, L.; Lefloch, B.; Kurtz, S.; Nadeau, D.; Pomarès, M.; Caplan, J.; Zavagno, A. (2008). "Triggered massive-star formation on the borders of Galactic H II regions". Astronomy & Astrophysics. 482 (2): 585–596. arXiv:0803.4152. doi:10.1051/0004-6361:20079233. S2CID 16100087.
  6. ^ "Sh2-211". Galaxy Map. Retrieved 16 November 2021.
  7. ^ "Tribble Nebulae". Flickr. 15 November 2021. Retrieved 16 November 2021.

External links edit

  •   Media related to NGC 1624 at Wikimedia Commons
  • NGC 1624 spider.seds.org
  • NGC 1624
  • Sh2-211
  • Sh2-212



1624, this, article, includes, list, general, references, lacks, sufficient, corresponding, inline, citations, please, help, improve, this, article, introducing, more, precise, citations, november, 2017, learn, when, remove, this, template, message, also, know. This article includes a list of general references but it lacks sufficient corresponding inline citations Please help to improve this article by introducing more precise citations November 2017 Learn how and when to remove this template message NGC 1624 also known as Sh2 212 3 in the Sharpless catalog is a very young open cluster in the constellation Perseus inside an emission nebula It was discovered by German British astronomer William Herschel in 1790 4 NGC 1624 is about 20 000 ly 6 000 pc from Earth and latest estimates give it an age of less than 4 million years 2 Its apparent magnitude is 11 8 1 and apparent diameter is about 3 0 arc minutes 4 Its celestial location is right ascension a 04h 40m 36 0s and declination d 50 27 42 1 It is potentially an area of massive star formation 5 NGC 1624Image of NGC 1624 with the Isaac Newton Telescope Credit IGAPSObservation data J2000 epoch Right ascension04h 40m 36 0s 1 Declination 50 27 42 1 Distance20000 2000 ly 6000 600 pc 2 Apparent magnitude V 11 8 1 Physical characteristicsEstimated age lt 4 Myr 2 Other designationsCr 53 C 0436 503 OCl 403 Tribble NebulaAssociationsConstellationPerseusSee also Open cluster List of open clustersAccording to Robert Trumpler s classification of open clusters this cluster contains fewer than 50 stars letter p with a high concentration I and whose magnitudes are distributed over an average interval number 2 The letter n at the end I2pn means that the cluster is inside a nebula Along with nearby emission nebula Sh2 211 6 it makes up what has become known as the Tribble Nebulae 7 so called because they look like the furry creatures first introduced in the Star Trek episode The Trouble with Tribbles Gallery edit nbsp The Tribble Nebula in Perseus Sh2 211 and Sh2 212 nbsp NGC 1624 in mid infrared with unWISEReferences edit a b c d e NGC 1624 SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 9 November 2017 a b c Sejong Open Cluster Survey SOS IV The Young Open Clusters NGC 1624 and NGC 1931 SIMBAD Centre de donnees astronomiques de Strasbourg Sh2 212 Galaxy Map Retrieved 16 November 2021 a b Seligman Courtney New General Catalogue objects NGC 1600 1649 cseligman com Retrieved 9 November 2017 Deharveng L Lefloch B Kurtz S Nadeau D Pomares M Caplan J Zavagno A 2008 Triggered massive star formation on the borders of Galactic H II regions Astronomy amp Astrophysics 482 2 585 596 arXiv 0803 4152 doi 10 1051 0004 6361 20079233 S2CID 16100087 Sh2 211 Galaxy Map Retrieved 16 November 2021 Tribble Nebulae Flickr 15 November 2021 Retrieved 16 November 2021 External links edit nbsp Media related to NGC 1624 at Wikimedia Commons NGC 1624 spider seds org NGC 1624 Sh2 211 Sh2 212 nbsp This star cluster related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title NGC 1624 amp oldid 1169575142, wikipedia, wiki, book, books, library,

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