NGC 146 is a small open cluster in the constellation Cassiopeia. It was discovered by John Herschel in 1829 using his father's 18.7 inch reflecting telescope.[3]
NGC 146 | |
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![]() Location of NGC 146 | |
Observation data (J2000 epoch) | |
Right ascension | 00h 33m 03.9s[1] |
Declination | +63° 18′ 32″[1] |
Distance | ~10000 (~3000) |
Apparent magnitude (V) | 9.1[2] |
Physical characteristics | |
Estimated age | <10 Myr |
Other designations | Cr 5, OCl 299, C 0030+630[2] |
Associations | |
Constellation | Cassiopeia |
Location
![](http://upload.wikimedia.org/wikipedia/commons/thumb/7/7d/Kappa_Cassiopeiae%2C_NGC146_and_NGC133.jpg/220px-Kappa_Cassiopeiae%2C_NGC146_and_NGC133.jpg)
NGC 146 is fairly easy to locate in the sky, being half a degree away from the bright star Kappa Cassiopeiae. However, spotting the cluster itself is difficult because of its low apparent magnitude of 9.1. Its relatively high declination of about 63° means it is not visible for below 27° S.Its distance is estimated at 3030 parsecs (9880 light years ),[4] but may be around 3500 pc (11000 ly) away.[5]
Characteristics
The cluster is at most 10 million years old, as there are numerous B-type main sequence stars and pre-main-sequence stars but relatively few evolved supergiants. Among its most massive stars are two Herbig Be stars.[5]
References
Further reading
- "The NGC/IC Project". Archived from the original on 2013-01-15. Retrieved 2016-08-02.