NGC 2808

NGC 2808
A Hubble Space Telescope (HST) image of NGC 2808. Credit: HST/NASA/ESA.
Observation data (J2000 epoch)
Constellation	Carina
Right ascension	9h 12m 2.6s[1]
Declination	-64° 51′ 46.2″[1]
Apparent magnitude (V)	7.8[1]
Physical characteristics
See also: Globular cluster, List of globular clusters

NGC 2808 is a globular cluster^[1] in the constellation Carina. The cluster belongs to the Milky Way, and is one of our home galaxy's most massive clusters, containing more than a million stars. It is estimated to be 12.5-billion years old.

Star Generations

It had been thought that NGC 2808, like typical globular clusters, contains only one generation of stars formed simultaneously from the same material. In 2007, a team of astronomers led by Giampaolo Piotto of the University of Padua in Italy investigated Hubble Space Telescope images of NGC 2808 taken in 2005 and 2006 with Hubble's Advanced Camera for Surveys. Unexpectedly, they found that this cluster is composed of three generations of stars, all born within 200 million years of the formation of the cluster.^[2]

Astronomers have argued that globular clusters can produce only one generation of stars, because the radiation from first generation stars would drive the residual gas not consumed in the first star generation phase out of the cluster. However, the great mass of a cluster such as NGC 2808 may suffice to gravitationally counteract the loss of gaseous matter. Thus, a second and a third generation of stars may form.

An alternative explanation for the three star generations of NGC 2808 is that it may actually be the remnant of a dwarf galaxy that collided with the Milky Way.

Sources

Generations of stars in a globular

References

1. ^ ^{a b c d} "SIMBAD Astronomical Database". Results for NGC 2808. http://simbad.u-strasbg.fr/Simbad. Retrieved 2007-05-07. 
2. ^ Piotto, G.; et al. (May 2007). "A Triple Main Sequence in the Globular Cluster NGC 2808". The Astrophysical Journal 661 (1): L53-L56. arXiv:astro-ph/0703767. Bibcode 2007ApJ...661L..53P. doi:10.1086/518503.