Star cluster
NGC 4349
Open star cluster · 257 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 | Crux |
| Distance | 2,155 pc (7.0 thousand ly) |
| Age | 257 million years |
| Member stars (MWSC) | 390 |
| Reddening E(B−V) | 0.45 |
| Metallicity [Fe/H] | 0.11 |
| Source | MWSC (Kharchenko et al. 2013) |
| Right ascension (J2000) | 12h 24m 14.4s |
| Declination (J2000) | −61° 52′ 12″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 28° N. South of latitude 28° S it never sets. It stands highest at midnight in March, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 7,029 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 125 million years.