NGC 654 is an open cluster in the constellation Cassiopeia. It was discovered by William Herschel in 1787. With apparent magnitude 6.5, it can be observed by binoculars.[4] It is located 2,5° northeast of the star Delta Cassiopeiae. In the same low power field can also be seen the open clusters NGC 663 and NGC 659. It surrounds a 7th magnitude yellowish star, an F5Ia supergiant, which is a possible member of the group.[5]
It is 2,400 parsec away. It is a very young cluster, aged approximately 15 million years, but it could be as old as 40 million years, with a time spread of star formation of at least ~20 Myr. The central region of the cluster shows less reddening than the rest of the cluster.[6] One explanation is that between the Solar System and the cluster lie two dust layers, one at 200pc and one more at 1Kpc.[7] Behind the cluster is one more dust layer. The cluster has approx. 80 members, including three Be stars and a few luminous stars like HD 10494 and F5Ia. The earliest spectral type is around B0.[8]
↑A. K. Pandey; K. Upadhyay; K. Ogura; Ram Sagar; V. Mohan; H. Mito; H. C. Bhatt; B. C. Bhatt (April 2005). "Stellar contents of two young open clusters: NGC 663 and 654". MNRAS358 (4): 1290–1308. doi:10.1111/j.1365-2966.2005.08784.x. Bibcode: 2005MNRAS.358.1290P.
↑Biman J. Medhi; Maheswar G.; J. C. Pandey; T. S. Kumar; Ram Sagar (2008). "Optical polarimetric study of open clusters: distribution of interstellar matter towards NGC 654". MNRAS388 (1): 105–116. doi:10.1111/j.1365-2966.2008.13405.x. Bibcode: 2008MNRAS.388..105M.
↑Negueruela, I.; González-Fernández, C.; Marco, A.; Clark, J. S. (2011). "A massive association around the obscured open cluster RSGC3". Astronomy & Astrophysics528: A59. doi:10.1051/0004-6361/201016102. Bibcode: 2011A&A...528A..59N.
↑Humphreys, R. M. (1978). "Studies of luminous stars in nearby galaxies. I. Supergiants and O stars in the Milky Way.". Astrophysical Journal Supplement Series38: 309–350. doi:10.1086/190559. Bibcode: 1978ApJS...38..309H.