Constellation Cassiopeia Declination +60° 13′ 06″ Apparent magnitude (V) 6.5 | Right ascension 00 30 00 Distance 5,450 ly (1,670 pc) Apparent dimensions (V) 21' | |
NGC 129 is an open cluster in the constellation Cassiopeia. It was discovered by William Herschel in 1788. It is located almost exactly halfway between the bright stars Caph (β Cassiopeiae) and γ Cassiopeiae. It is large but not dense and can be observed by binoculars, where the most obvious is a small triangle of stars of magnitude 8 and 9, located in the center of the cluster.
NGC 129 contains several giant stars. The brightest member of the cluster in DL Cassiopeiae, a binary system which contains a Cepheid variable with 8,00 days period. Using the fluctuations of the brightness of DL Cassiopeia from 8,7 to 9,28, Gieren and al in 1994 determined the distance of NGC 129 at 2034 ±110 kpc (6.630 ±360 ly), quite larger than the distance obtained by Turner et al. (1992), who obtained distance of 1,670 ±13 pc, from ZAMS fitting of the cluster. A possible cause of this difference is the different level of obstruction of light and star reddening of the stars of the cluster. One more cepheid variable, V379 Cas, is also a possible member of NGC 129.