| NGC 7790 | |
|---|---|
NGC 7790 (taken from Stellarium) Credit: Roberto Mura | |
| Observation data (J2000.0epoch) | |
| Right ascension | 23h 58m 24.2s[1] |
| Declination | +61° 12′ 30″[1] |
| Distance | 10.76 ± 0.75 kly (3.30 ± 0.23 kpc)[2] |
| Apparent magnitude (V) | 8.5 |
| Apparent dimensions (V) | 7′.4[2] diameter |
| Physical characteristics | |
| Estimated age | 60–80[3] Myr |
| Other designations | Cr 461 |
| Associations | |
| Constellation | Cassiopeia |
| See also:Open cluster,List of open clusters | |
NGC 7790 is a youngopen cluster[1] ofstars located some 10,800[2]light years away from Earth in the northernconstellation ofCassiopeia. At this distance, the light from the cluster has undergoneextinction from interstellar gas and dust equal to E(B – V ) = 0.51magnitude in theUBV photometric system. NGC 7790 has aTrumpler class rating of II2m[2] and the estimated age is 60–80 million years.[3] It contains threecepheid variables: CEa Cas, CEb Cas, and CF Cas.[2]
This cluster is on an orbit through theMilky Way galaxy that has aneccentricity of 0.22 ± 0.07 and aperiod 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, theGalactic Center. The maximum distance reached above (or below) thegalactic 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]

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