Star cluster
NGC 2477
Open star cluster · 813 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 | 1,450 pc (4.7 thousand ly) |
| Age | 813 million years |
| Member stars (MWSC) | 1,209 |
| Reddening E(B−V) | 0.29 |
| Metallicity [Fe/H] | -0.19 |
| Source | MWSC (Kharchenko et al. 2013) |
| Right ascension (J2000) | 7h 52m 08.4s |
| Declination (J2000) | −38° 31′ 48″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 51° N. South of latitude 51° 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 4,729 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 84 million years.