California Nebula
NGC 1499 · Emission nebula in Perseus
- Magnitude
- 5.0
- Size
- 160′ × 40′
- Effective surface brightness
- 22.6 mag/arcsec²
- Best months
- Nov, Dec, Jan
- Declination
- +36°
- Filter
- Dual-band recommended
A long, faint hydrogen streak near Menkib, nearly three degrees end to end. Needs a wide field and a dual-band filter; it is almost invisible in broadband.
Reachable from mid-northern latitudes (UK, northern US, central Europe) and from the south.
How long with each smart telescope
| Telescope | Bortle 3 (rural) | Bortle 5 (suburban) | Bortle 7 (urban edge) |
|---|---|---|---|
| ZWO Seestar S5010 s subs, dual-band | 2 h 21 min845 subs | 2 h 36 min935 subs | 3 h 41 min1,326 subs |
| ZWO Seestar S50 Pro10 s subs, dual-band | 1 h 34 min566 subs | 1 h 50 min662 subs | 3 h 01 min1,086 subs |
| ZWO Seestar S3010 s subs, dual-band | 1 h 23 min496 subs | 1 h 37 min585 subs | 2 h 43 min976 subs |
| ZWO Seestar S30 Pro10 s subs, dual-band | 1 h 43 min616 subs | 1 h 60 min718 subs | 3 h 14 min1,163 subs |
| DwarfLab Dwarf 315 s subs, dual-band | 2 h 17 min550 subs | 2 h 40 min642 subs | 4 h 21 min1,045 subs |
| DwarfLab Dwarf Mini15 s subs, dual-band | 1 h 07 min268 subs | 1 h 22 min328 subs | 2 h 27 min589 subs |
| DwarfLab Dwarf II15 s subs | 5 h 26 min1,306 subs | 7 h 42 min1,848 subs | 18 h4,215 subs |
| Vaonis Vespera II10 s subs | 1 h 11 min429 subs | 2 h721 subs | 5 h 33 min1,999 subs |
| Vaonis Vespera Pro10 s subs | 3 h 34 min1,282 subs | 5 h 16 min1,897 subs | 13 h4,584 subs |
| Unistellar eQuinox 24 s subs | 1 h 41 min1,516 subs | 2 h 11 min1,971 subs | 4 h 24 min3,963 subs |
| Unistellar Odyssey4 s subs | 9 h 06 min8,189 subs | 11 h9,847 subs | 19 h17,094 subs |
| Celestron Origin10 s subs | 16 min99 subs | 30 min182 subs | 1 h 31 min545 subs |
Imaging the emission nebula
Emission nebulae glow in a few narrow lines, mostly hydrogen-alpha (deep red) and doubly ionised oxygen (teal). A dual-band filter passes those lines and blocks most skyglow, which is why it cuts the time needed from a suburban sky so dramatically. Use it. From a genuinely dark site the gain is smaller because there is less skyglow to block, and read noise becomes the limit, which is where longer subs (EQ mode) earn their keep.
Stars lose colour through a dual-band filter; a short broadband stack blended in fixes that if you care.
Per-telescope pages
- How long to image the California Nebula with the ZWO Seestar S50
- How long to image the California Nebula with the ZWO Seestar S50 Pro
- How long to image the California Nebula with the ZWO Seestar S30
- How long to image the California Nebula with the ZWO Seestar S30 Pro
- How long to image the California Nebula with the DwarfLab Dwarf 3
- How long to image the California Nebula with the DwarfLab Dwarf Mini
- How long to image the California Nebula with the DwarfLab Dwarf II
- How long to image the California Nebula with the Vaonis Vespera II
- How long to image the California Nebula with the Vaonis Vespera Pro
- How long to image the California Nebula with the Unistellar eQuinox 2
- How long to image the California Nebula with the Unistellar Odyssey
- How long to image the California Nebula with the Celestron Origin