Astronomy:NGC 3228
NGC 3228 | |
---|---|
Location of NGC 3228
NGC 3228 DSS.jpg | |
Observation data (J2000 epoch) | |
Constellation | Vela |
Right ascension | 10h 21m 22s[1] |
Declination | −51° 43′ 42″[1] |
Distance | 1,870 ly (573 pc[2]) |
Apparent magnitude (V) | 6.0 [1] |
Apparent dimensions (V) | 11'[2] |
Physical characteristics | |
Estimated age | 260 million years[2] |
Other designations | Collinder 218, vdBH 93 |
NGC 3228 is an open cluster in Vela. It was discovered by Nicolas Louis de Lacaille in 1751–1752, while he was in South Africa and catalogued it as Lac II.7.[3] It is small but bright and can be observed easily with binoculars in sufficiently dark skies.[4]
It is a cluster of Trumpler type I1p or II3p, with few members with large brightness range and a slight concentration toward its center.[3] Klarchenko et al. mention 53 possible members within the angular diameter of the cluster. The tidal radius of the cluster is 1.4 – 5.5 parsecs (4.5 – 18 light years) and represents the average outer limit of NGC 3228, beyond which a star is unlikely to remain gravitationally bound to the cluster core.[2] The brightest member is of mag. 7.9 and the hottest star is of spectral type B9.[3] One member, HD 89856 (mag. 9.04, spectral type B9), is a variable star with period 4.556 days.[5]
References
- ↑ 1.0 1.1 1.2 "NGC 3228". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+3228.
- ↑ 2.0 2.1 2.2 2.3 Kharchenko, N. V.; Piskunov, A. E.; Schilbach, E.; Röser, S.; Scholz, R.-D. (3 October 2013). "Global survey of star clusters in the Milky Way". Astronomy & Astrophysics 558: A53. doi:10.1051/0004-6361/201322302. Bibcode: 2013A&A...558A..53K. ftp://cdsarc.u-strasbg.fr/pub/cats/J/A%2BA/558/A53/catalog.dat.
- ↑ 3.0 3.1 3.2 Kronberg, Christine; Frommert, Hartmut. "NGC 3228". http://messier.seds.org/xtra/ngc/n3228.html.
- ↑ Monks, Neale (2010) (in en). Go-To Telescopes Under Suburban Skies. Springer Science & Business Media. p. 40. ISBN 9781441968517. https://books.google.com/books?id=waO6tUtfblsC&pg=PA40.
- ↑ Paunzen, E.; Hensberge, H.; Maitzen, H. M.; Netopil, M.; Trigilio, C.; Fossati, L.; Heiter, U.; Pranka, M. (26 November 2010). "A photometric long-term study of chemically peculiar stars in open clusters". Astronomy & Astrophysics 525: A16. doi:10.1051/0004-6361/200913789. Bibcode: 2011A&A...525A..16P. ftp://cdsarc.u-strasbg.fr/pub/cats/J/A%2BA/525/A16/stars.v00.
External links
- NGC 3228 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Original source: https://en.wikipedia.org/wiki/NGC 3228.
Read more |