Globular cluster
AvdB (Pal 14)
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 2.4 % of the Sun’s. Distance, brightness and structure come from the Harris catalogue.
| Type | Globular cluster |
|---|---|
| Constellation | Hercules |
| Distance | 76,500 pc (249.5 thousand ly) |
| Metallicity [Fe/H] | -1.62 |
| Half-light radius | 27.1 pc |
| Central concentration (c) | 0.80 |
| Radial velocity | 72.3 km/s |
| Source | Harris 1996 (2010) |
| Right ascension (J2000) | 16h 11m 00.6s |
| Declination (J2000) | +14° 57′ 28″ |
In the sky
Visible from the whole Northern Hemisphere and south to latitude 75° S. North of latitude 75° N it never sets. It stands highest at midnight in May, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 250 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 4.4 billion years.