Star cluster
NGC 2482
Open star cluster · 324 million years
An open cluster of stars born together from the same gas cloud in the Milky Way’s disc; the Galaxy’s tidal forces will disperse it within a few hundred million years. Position, distance, age and member count come from the MWSC catalogue; the total brightness is roughly estimated from the member count.
| Type | Star cluster |
|---|---|
| Constellation | Puppis |
| Distance | 1,344 pc (4.4 thousand ly) |
| Age | 324 million years |
| Member stars (MWSC) | 145 |
| Reddening E(B−V) | 0.09 |
| Metallicity [Fe/H] | -0.08 |
| Source | MWSC (Kharchenko et al. 2013) |
| Right ascension (J2000) | 7h 55m 10.2s |
| Declination (J2000) | −24° 16′ 30″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 66° N. South of latitude 66° S it never sets. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 4,384 years ago. At that time the first farming villages were being founded; there was no writing yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 78 million years.