Heart Nebula
IC 1805, Sh2-190 · Emission nebula in Cassiopeia
- Magnitude
- 6.5
- Size
- 60′
- Effective surface brightness
- 22.8 mag/arcsec²
- Best months
- Oct, Nov, Dec
- Declination
- +61°
- Filter
- Dual-band recommended
A degree-wide hydrogen cloud shaped like a heart, with the bright Melotte 15 cluster and pillars at its centre. Dual-band, and a wide field or mosaic.
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 | 3 h 19 min1,197 subs | 3 h 41 min1,326 subs | 5 h 15 min1,892 subs |
| ZWO Seestar S50 Pro10 s subs, dual-band | 2 h 12 min791 subs | 2 h 35 min931 subs | 4 h 17 min1,543 subs |
| ZWO Seestar S3010 s subs, dual-band | 1 h 55 min692 subs | 2 h 17 min821 subs | 3 h 51 min1,387 subs |
| ZWO Seestar S30 Pro10 s subs, dual-band | 2 h 24 min863 subs | 2 h 48 min1,010 subs | 4 h 36 min1,654 subs |
| DwarfLab Dwarf 315 s subs, dual-band | 3 h 12 min770 subs | 3 h 46 min903 subs | 6 h 11 min1,486 subs |
| DwarfLab Dwarf Mini15 s subs, dual-band | 1 h 33 min372 subs | 1 h 54 min458 subs | 3 h 29 min835 subs |
| DwarfLab Dwarf II15 s subs | 7 h 44 min1,856 subs | 11 h2,639 subs | 25 h6,061 subs |
| Vaonis Vespera II10 s subs | 1 h 40 min602 subs | 2 h 51 min1,025 subs | 7 h 59 min2,873 subs |
| Vaonis Vespera Pro10 s subs | 5 h 03 min1,816 subs | 7 h 31 min2,705 subs | 18 h6,590 subs |
| Unistellar eQuinox 24 s subs | 2 h 24 min2,164 subs | 3 h 08 min2,823 subs | 6 h 20 min5,702 subs |
| Unistellar Odyssey4 s subs | 13 h11,739 subs | 16 h14,136 subs | 27 h24,611 subs |
| Celestron Origin10 s subs | 23 min138 subs | 43 min258 subs | 2 h 10 min782 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 Heart Nebula with the ZWO Seestar S50
- How long to image the Heart Nebula with the ZWO Seestar S50 Pro
- How long to image the Heart Nebula with the ZWO Seestar S30
- How long to image the Heart Nebula with the ZWO Seestar S30 Pro
- How long to image the Heart Nebula with the DwarfLab Dwarf 3
- How long to image the Heart Nebula with the DwarfLab Dwarf Mini
- How long to image the Heart Nebula with the DwarfLab Dwarf II
- How long to image the Heart Nebula with the Vaonis Vespera II
- How long to image the Heart Nebula with the Vaonis Vespera Pro
- How long to image the Heart Nebula with the Unistellar eQuinox 2
- How long to image the Heart Nebula with the Unistellar Odyssey
- How long to image the Heart Nebula with the Celestron Origin