14 May 2020
The Trifid Nebula, Messier 20, is a star-forming region, rich in gas and dust.
The central nebula appears divided into three(ish!) lobes by filaments of foreground dust. The red colour is due to hydrogen-alpha emission, arising from gas ionized by radiation from newly-formed hot stars. At the margins of the nebula, dust reflects the blue light from the same stars.
M20
10 credit
Filtro | Exp. media (s) | Esposizione totale | Sottoframe |
|---|---|---|---|
| Luminance | 67 | 40m | 36 |
| Red | 69 | 40m | 35 |
| Green | 857 | 8h20m | 35 |
| Blue | 65 | 38m | 35 |
| Halpha | 806 | 7h50m | 35 |