Star cluster
Berkeley 68
Open star cluster · 1.3 billion 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 | Perseus |
| Distance | 1,800 pc (5.9 thousand ly) |
| Age | 1.3 billion years |
| Member stars (MWSC) | 160 |
| Reddening E(B−V) | 0.67 |
| Source | MWSC (Kharchenko et al. 2013) |
| Right ascension (J2000) | 4h 44m 27.6s |
| Declination (J2000) | +42° 06′ 00″ |
In the sky
Visible from the whole Northern Hemisphere and south to latitude 48° S. North of latitude 48° N it never sets. It stands highest at midnight in November, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 5,871 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 104 million years.