Supernova
CTB 37A (SNR G348.5+0.1)
Supernova remnant
The shock wave of a supernova expanding at thousands of kilometres per second: it sweeps up and heats the interstellar gas and shines in radio waves. The distance is estimated from the radio surface-brightness–diameter (Σ–D) relation and may be off by a factor of two.
| Type | Supernova |
|---|---|
| Constellation | Scorpius |
| Distance | 2,930 pc (9.6 thousand ly) · estimated |
| Diameter | 41.7 ly |
| Type | Shell type |
| Radio flux (1 GHz) | 72 Jy |
| Source | Green's SNR Catalogue |
| Right ascension (J2000) | 17h 14m 06.0s |
| Declination (J2000) | −38° 31′ 59″ |
In the sky
Visible from the whole Southern Hemisphere and north to latitude 51° N. South of latitude 51° S it never sets. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 9,556 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 170 million years.