Star cluster
NGC 2451B
Open star cluster · 170 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 | 489 pc (1.6 thousand ly) |
| Age | 170 million years |
| Member stars (MWSC) | 215 |
| Reddening E(B−V) | 0.17 |
| Metallicity [Fe/H] | -0.45 |
| Source | MWSC (Kharchenko et al. 2013) |
| Right ascension (J2000) | 7h 44m 27.6s |
| Declination (J2000) | −37° 40′ 12″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 52° N. South of latitude 52° 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 431. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 28 million years.