NGC 7790

NGC 7790
NGC 7790
	NGC 7790 (taken from Stellarium) ; Credit: Roberto Mura
Observation data (J2000.0 epoch)
Right ascension	23h 58m 24.2s
Declination	+61° 12′ 30″
Distance	10.76 ± 0.75 kly (3.30 ± 0.23 kpc)
Apparent magnitude (V)	8.5
Apparent dimensions (V)	7′.4 diameter
Physical characteristics
Estimated age	60–80 Myr
Other designations	Cr 461
Associations
Constellation	Cassiopeia
	See also: Open cluster, List of open clusters

NGC 7790 is a young open cluster^[1] of stars located some 10,800^[2] light years away from Earth in the northern constellation of Cassiopeia. At this distance, the light from the cluster has undergone extinction from interstellar gas and dust equal to E(B – V ) = 0.51 magnitude in the UBV photometric system. NGC 7790 has a Trumpler class rating of II2m^[2] and the estimated age is 60–80 million years.^[3] It contains three cepheid variables: CEa Cas, CEb Cas, and CF Cas.^[2]

This cluster is on an orbit through the Milky Way galaxy that has an eccentricity of 0.22 ± 0.07 and a period of (225.0 ± 27.1) million years. It will come as close as 20.2 ± 3.9 kly (6.2 ± 1.2 kpc) to, and as distant as 31.6 ± 2.9 kly (9.7 ± 0.9 kpc) from, the Galactic Center. The maximum distance reached above (or below) the galactic plane is 0.78 ± 1.30 kly (0.24 ± 0.40 kpc). On average, it will cross the galactic plane every (35.7 ± 13.0) million years.^[4]

References

^ ^a ^b ^c Revised New General Catalogue and Index Catalogue, Wolfgang Steinicke, February 2009, retrieved 2013-07-01. {{citation}}: External link in |publisher= (help)^{[permanent dead link‍]}
^ ^a ^b ^c ^d ^e Gupta, A. C.; et al. (September 2000), "A complete photometric study of the open cluster NGC 7790 containing Cepheid variables", Astronomy and Astrophysics Supplement, 145 (3): 365–375, Bibcode:2000A&AS..145..365G, doi:10.1051/aas:2000247.
^ ^a ^b Davidge, T. J. (December 2012), "The Young Open Clusters King 12, NGC 7788, and NGC 7790: Pre-main-sequence Stars and Extended Stellar Halos", The Astrophysical Journal, 761 (2): 155, arXiv:1211.6398, Bibcode:2012ApJ...761..155D, doi:10.1088/0004-637X/761/2/155, S2CID 119205384.
^ Wu, Zhen-Yu; et al. (November 2009), "The orbits of open clusters in the Galaxy", Monthly Notices of the Royal Astronomical Society, 399 (4): 2146–2164, arXiv:0909.3737, Bibcode:2009MNRAS.399.2146W, doi:10.1111/j.1365-2966.2009.15416.x, S2CID 6066790.

External links

Media related to NGC 7790 at Wikimedia Commons
NGC 7790 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

This star cluster–related article is a stub. You can help Wikipedia by expanding it.

[revngcic2009-1] Revised New General Catalogue and Index Catalogue, Wolfgang Steinicke, February 2009, retrieved 2013-07-01. {{citation}}: External link in |publisher= (help)^{[permanent dead link‍]}

[AAS145_365-2] Gupta, A. C.; et al. (September 2000), "A complete photometric study of the open cluster NGC 7790 containing Cepheid variables", Astronomy and Astrophysics Supplement, 145 (3): 365–375, Bibcode:2000A&AS..145..365G, doi:10.1051/aas:2000247.

[ApJ761_2_155-3] Davidge, T. J. (December 2012), "The Young Open Clusters King 12, NGC 7788, and NGC 7790: Pre-main-sequence Stars and Extended Stellar Halos", The Astrophysical Journal, 761 (2): 155, arXiv:1211.6398, Bibcode:2012ApJ...761..155D, doi:10.1088/0004-637X/761/2/155, S2CID 119205384.

[MNRAS399_4_2146-4] Wu, Zhen-Yu; et al. (November 2009), "The orbits of open clusters in the Galaxy", Monthly Notices of the Royal Astronomical Society, 399 (4): 2146–2164, arXiv:0909.3737, Bibcode:2009MNRAS.399.2146W, doi:10.1111/j.1365-2966.2009.15416.x, S2CID 6066790.

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