Planetary nebula
He 2-111
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 | Centaurus |
| Distance | 2,040 pc (6.7 thousand ly) · estimated |
| Diameter | 1.0 ly |
| Central star | V 16.7 |
| Expansion speed | 12 km/s |
| PN G name | PN G315.0-00.3 |
| Source | Strasbourg–ESO PN Catalogue |
| Right ascension (J2000) | 14h 33m 18.3s |
| Declination (J2000) | −60° 49′ 45″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 29° N. South of latitude 29° 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 6,654 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 118 million years.