Planetary nebula
K 3-67
Planetary nebula
A shell of gas thrown off by a dying Sun-like star, glowing in the ultraviolet light of the hot core at its centre. Within a few tens of thousands of years it will disperse and fade from view. The distance is a statistical estimate, uncertain by 30–50 %.
| Type | Planetary nebula |
|---|---|
| Constellation | Perseus |
| Distance | 4,170 pc (13.6 thousand ly) · estimated |
| Diameter | 0.0 ly |
| Central star | O(C) |
| Expansion speed | 21 km/s |
| PN G name | PN G165.5-06.5 |
| Source | Strasbourg–ESO PN Catalogue |
| Right ascension (J2000) | 4h 39m 47.9s |
| Declination (J2000) | +36° 45′ 43″ |
In the sky
Visible from the whole Northern Hemisphere and south to latitude 53° S. North of latitude 53° 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 14 thousand years ago. At that time Homo sapiens was spreading out of Africa; there was no farming yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 241 million years.