Star cluster
NGC 2451A
Open star cluster · 58 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 | 188 pc (613.2 ly) |
| Age | 58 million years |
| Member stars (MWSC) | 297 |
| Reddening E(B−V) | 0.00 |
| Metallicity [Fe/H] | -0.53 |
| Source | MWSC (Kharchenko et al. 2013) |
| Right ascension (J2000) | 7h 41m 20.4s |
| Declination (J2000) | −38° 31′ 12″ |
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 around the year 1413. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 11 million years.