21 Mar 2023
Although commonly much weaker than Ha, the SII emission often provides significant detail and outline in bright nebula. Seen here is a starless Eta Carina in the light of SII.
NGC 3372
7 credit
Filter | Avg Exp (s) | Total Exposure | Subframes |
|---|---|---|---|
| Luminance | 104 | 45m | 26 |
| Red | 92 | 40m | 26 |
| Green | 92 | 40m | 26 |
| Blue | 92 | 40m | 26 |
| Halpha | 1119 | 8h5m | 26 |