Star cluster
NGC 4852
Open star cluster · 427 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 | Centaurus |
| Distance | 1,106 pc (3.6 thousand ly) |
| Age | 427 million years |
| Member stars (MWSC) | 187 |
| Reddening E(B−V) | 0.25 |
| Source | MWSC (Kharchenko et al. 2013) |
| Right ascension (J2000) | 13h 00m 10.8s |
| Declination (J2000) | −59° 35′ 24″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 30° N. South of latitude 30° S it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around 1582 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 64 million years.