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NGC 2808

Globular cluster in the constellation Carina

NGC 2808
AHubble Space Telescope (HST) image of NGC 2808
Observation data (J2000 epoch)
Class	I[1]
Constellation	Carina
Right ascension	09h12m 03.10s[2]
Declination	–64° 51′ 48.6″[2]
Distance	31.3 kly (9.6 kpc)[3]
Apparent magnitude (V)	6.2[4]
Apparent dimensions (V)	13.8′[4]
Physical characteristics
Mass	1.42×106[3] M☉
Metallicity	${\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}$ = –1.14[3] dex
Estimated age	10.2 Gyr[5]
Other designations	GCl 13, Melotte95[6]
See also: Globular cluster, List of globular clusters

NGC 2808 is a globular cluster^[6] in the constellation Carina. The cluster currently belongs to the Milky Way, although it was likely stolen from a dwarf galaxy that collided with the Milky Way. NGC 2808 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.

The cluster is being disrupted by the galactic tide, trailing a long tidal tail.^[7]

Star generations[edit]

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.^[8]

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 core of a dwarf galaxy that collided with the Milky Way, the Sausage Galaxy.^[9]

See also[edit]

• Messier 54 and Messier 79, two other possibly extragalactic globular clusters
• Omega Centauri

References[edit]

External links[edit]

• Media related to NGC 2808 at Wikimedia Commons