Globular cluster
NGC 6752
Globular cluster
A globular cluster of hundreds of thousands of old stars orbiting in the Galaxy’s halo: among the oldest objects of the Milky Way, about 12 billion years old. Its metal abundance is 2.9 % of the Sun’s. Distance, brightness and structure come from the Harris catalogue.
| Type | Globular cluster |
|---|---|
| Constellation | Pavo |
| Distance | 4,000 pc (13.0 thousand ly) |
| Metallicity [Fe/H] | -1.54 |
| Half-light radius | 2.2 pc |
| Central concentration (c) | 2.50 · core-collapsed |
| Radial velocity | -26.7 km/s |
| Source | Harris 1996 (2010) |
| Right ascension (J2000) | 19h 10m 52.1s |
| Declination (J2000) | −59° 59′ 05″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 30° N. South of latitude 30° S it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 13 thousand years ago. At that time Homo sapiens was spreading out of Africa; there was no farming yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 231 million years.