Globular cluster
M 3 (NGC 5272)
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 3.2 % of the Sun’s. Distance, brightness and structure come from the Harris catalogue.
| Type | Globular cluster |
|---|---|
| Constellation | Canes Venatici |
| Distance | 10,200 pc (33.3 thousand ly) |
| Metallicity [Fe/H] | -1.50 |
| Half-light radius | 6.9 pc |
| Central concentration (c) | 1.89 |
| Radial velocity | -147.6 km/s |
| Source | Harris 1996 (2010) |
| Right ascension (J2000) | 13h 42m 11.6s |
| Declination (J2000) | +28° 22′ 38″ |
In the sky
Visible from the whole Northern Hemisphere and south to latitude 62° S. North of latitude 62° N it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 33 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 590 million years.