Globular cluster
Djorg 1
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 3.1 % of the Sun’s. Distance, brightness and structure come from the Harris catalogue.
| Type | Globular cluster |
|---|---|
| Constellation | Scorpius |
| Distance | 13,700 pc (44.7 thousand ly) |
| Metallicity [Fe/H] | -1.51 |
| Half-light radius | 6.3 pc |
| Central concentration (c) | 1.50 |
| Radial velocity | -362.4 km/s |
| Source | Harris 1996 (2010) |
| Right ascension (J2000) | 17h 47m 28.3s |
| Declination (J2000) | −33° 03′ 56″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 57° N. South of latitude 57° S it never sets. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 45 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 793 million years.