| NGC 7510 | |
|---|---|
 Amateur image of NGC7510 | |
| Observation data (J2000.0 epoch) | |
| Right ascension | 23h 11.1m [1] |
| Declination | +60° 34′ [1] |
| Distance | 11.4 kly (3.48 kpc) [2] |
| Apparent magnitude (V) | 7.9 [1] |
| Apparent dimensions (V) | 7.0′ [1] |
| Physical characteristics | |
| Estimated age | 107 [3] |
| Other designations | Cr 454 |
| Associations | |
| Constellation | Cepheus |
NGC 7510 is an open cluster of stars located around 11,400 [2] light years away in the constellation Cepheus, near the border with Cassiopeia. [3] At this distance, the light from the cluster has undergone extinction from interstellar gas and dust equal to E(B – V) = 0.90 ± 0.02 magnitude in the UBV photometric system. [2] Its brightest member is a giant star with a stellar classification of B1.5 III. This cluster forms part of the Perseus Spiral Arm. [4] It has a Trumpler class rating of II 2 m [2] and is around 10 million years old. [3]
- ^ a b c d James O'Meara, Stephen (2007), Steve O'Meara's Herschel 400 Observing Guide, Cambridge University Press, p. 278, ISBN 978-0521858939.
- ^ a b c d Paunzen, E.; et al. (November 2005), "CCD photometric search for peculiar stars in open clusters. VI. NGC 1502, NGC 3105, Stock 16, NGC 6268, NGC 7235 and NGC 7510", Astronomy and Astrophysics, 443 (1): 157–162, arXiv: astro-ph/0508151, Bibcode: 2005A&A...443..157P, doi: 10.1051/0004-6361:20053287, S2CID 17585037.
- ^ a b c Barbon, R.; Hassan, S. M. (February 1996), "A new study of the young open cluster NGC 7510", Astronomy and Astrophysics Supplement, 115: 325–332, Bibcode: 1996A&AS..115..325B.
- ^ Crossen, Craig; Rhemann, Gerald (2004), Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes, Springer, p. 78, ISBN 978-3211008515.
-
Media related to
NGC 7510 at Wikimedia Commons - "SIMBAD Astronomical Database". Results for NGC 6884. Retrieved 2007-04-10.
- NGC 7510 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |
| NGC 7510 | |
|---|---|
|
Amateur image of NGC7510 | |
| Observation data (J2000.0 epoch) | |
| Right ascension | 23h 11.1m [1] |
| Declination | +60° 34′ [1] |
| Distance | 11.4 kly (3.48 kpc) [2] |
| Apparent magnitude (V) | 7.9 [1] |
| Apparent dimensions (V) | 7.0′ [1] |
| Physical characteristics | |
| Estimated age | 107 [3] |
| Other designations | Cr 454 |
| Associations | |
| Constellation | Cepheus |
NGC 7510 is an open cluster of stars located around 11,400 [2] light years away in the constellation Cepheus, near the border with Cassiopeia. [3] At this distance, the light from the cluster has undergone extinction from interstellar gas and dust equal to E(B – V) = 0.90 ± 0.02 magnitude in the UBV photometric system. [2] Its brightest member is a giant star with a stellar classification of B1.5 III. This cluster forms part of the Perseus Spiral Arm. [4] It has a Trumpler class rating of II 2 m [2] and is around 10 million years old. [3]
- ^ a b c d James O'Meara, Stephen (2007), Steve O'Meara's Herschel 400 Observing Guide, Cambridge University Press, p. 278, ISBN 978-0521858939.
- ^ a b c d Paunzen, E.; et al. (November 2005), "CCD photometric search for peculiar stars in open clusters. VI. NGC 1502, NGC 3105, Stock 16, NGC 6268, NGC 7235 and NGC 7510", Astronomy and Astrophysics, 443 (1): 157–162, arXiv: astro-ph/0508151, Bibcode: 2005A&A...443..157P, doi: 10.1051/0004-6361:20053287, S2CID 17585037.
- ^ a b c Barbon, R.; Hassan, S. M. (February 1996), "A new study of the young open cluster NGC 7510", Astronomy and Astrophysics Supplement, 115: 325–332, Bibcode: 1996A&AS..115..325B.
- ^ Crossen, Craig; Rhemann, Gerald (2004), Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes, Springer, p. 78, ISBN 978-3211008515.
-
Media related to
NGC 7510 at Wikimedia Commons
- "SIMBAD Astronomical Database". Results for NGC 6884. Retrieved 2007-04-10.
- NGC 7510 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
| Stars |
| ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||||
|
Star clusters |
| ||||||||||||
| Nebulae |
| ||||||||||||
| Galaxies |
| ||||||||||||
|
| This star cluster–related article is a stub. You can help Wikipedia by expanding it. |