Astronomy:NGC 1342

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NGC 1342
NGC 1342 imaged in 2026
Observation data (J2000 epoch)
ConstellationPerseus[1]
Right ascension 03h 31m 38s[2]
Declination+37° 22′ 36″[2]
Distance2,170 ly (670 pc)[3]
Apparent magnitude (V)6.7[1]
Apparent dimensions (V)17′[1]
Physical characteristics
Estimated age450 million years
Other designationsCr 40
See also: Open cluster, List of open clusters

NGC 1342 is an open cluster of stars in the northern constellation of Perseus.[1] Alternatively, it is known as the Stingray Cluster,[4] or the Little Scorpion Cluster, due to a visual resemblance to the constellation Scorpius.[5]

NGC 1342 cluster was discovered by William Herschel on 28 December 1799. It is located in the south of the constellation, almost halfway between Algol (β Persei) and ζ Persei, away from the plane of the Milky Way. NGC 1342 has an apparent size of 17' and an apparent magnitude of 6.7, marginally visible by naked eye.[6]

In 1962, Beverly Turner Lynds discovered LDN 1434, located nearby NGC 1342.[5] In 1994, Peña, J. H. and Peniche, R. estimated by the use of photometric data, that the age of the cluster is 400 million years.[7]

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. 174. doi:10.1007/978-3-319-03170-5. ISBN 978-3-319-03169-9. 
  2. ↑ 2.0 2.1 "NGC 1342". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+1342. 
  3. ↑ WEBDA: NGC 1342
  4. ↑ Stoyan, Ronald; Schurig, Stephan (2014). interstellarum Deep Sky Atlas. Erlangen: Cambridge University Press; Oculum-Verlag GmbH. ISBN 978-1-107-50338-0. OCLC 920437579. http://www.deep-sky-atlas.com/. 
  5. ↑ 5.0 5.1 "Little Scorpion Cluster (NGC 1342)". Deep Sky Corner. https://deepskycorner.ch/obj/ngc1342.en.php. 
  6. ↑ Stephen James O'Meara (2011). Deep-Sky Companions: The Secret Deep. 4. Cambridge University Press. pp. 61–62. ISBN 978-1-139-50007-4. https://books.google.com/books?id=v859bKO0A4gC&pg=PA61. 
  7. ↑ Peña, J. H.; Peniche, R.; Bravo, H.; Yam, O. (1994). "uvby-β photometry of open clusters. II. NGC 1342.". Revista Mexicana de Astronomía y Astrofísica 28 (1): 7–16. Bibcode: 1994RMxAA..28....7P.