M32
NGC 221 · Galaxy in Andromeda
- Magnitude
- 8.1
- Size
- 8′ × 6′
- Effective surface brightness
- 20.9 mag/arcsec²
- Best months
- Sep, Oct, Nov
- Declination
- +41°
- Filter
- None (broadband target)
The compact elliptical companion of Andromeda, sitting on its disc. Appears in every M31 frame.
Reachable from mid-northern latitudes (UK, northern US, central Europe) and from the south.
How long with each smart telescope
| Telescope | In frame | Bortle 3 (rural) | Bortle 5 (suburban) | Bortle 7 (urban edge) |
|---|---|---|---|---|
| ZWO Seestar S5010 s subs | 19% | 10 min60 subs | 14 min85 subs | 33 min196 subs |
| ZWO Seestar S50 Pro10 s subs | 10% | 11 min66 subs | 15 min93 subs | 35 min213 subs |
| ZWO Seestar S3010 s subs | 11% | 11 min65 subs | 15 min90 subs | 33 min201 subs |
| ZWO Seestar S30 Pro10 s subs | 6% | 12 min70 subs | 16 min99 subs | 37 min225 subs |
| DwarfLab DWARF 315 s subs | 8% | 14 min55 subs | 20 min81 subs | 49 min196 subs |
| DwarfLab DWARF mini15 s subs | 11% | 10 min40 subs | 14 min57 subs | 33 min131 subs |
| DwarfLab Draco30 s subs | 11% | 15 min30 subs | 15 min30 subs | 27 min54 subs |
| DwarfLab DWARF II15 s subs | 7% | 39 min155 subs | 50 min202 subs | 1 h 42 min407 subs |
| Vaonis Vespera II10 s subs | 9% | 10 min60 subs | 14 min85 subs | 33 min196 subs |
| Vaonis Vespera Pro10 s subs | 8% | 23 min139 subs | 32 min193 subs | 1 h 11 min426 subs |
| Vaonis Vespera 310 s subs | 9% | 9 min57 subs | 13 min81 subs | 31 min188 subs |
| Vaonis Vespera Pro 210 s subs | 8% | 22 min132 subs | 31 min184 subs | 1 h 08 min407 subs |
| Unistellar eQuinox 24 s subs | 23% | 11 min167 subs | 14 min206 subs | 25 min379 subs |
| Unistellar Odyssey4 s subs | 24% | 56 min837 subs | 1 h 05 min981 subs | 1 h 47 min1,609 subs |
| Celestron Origin10 s subs | 16% | 5 min30 subs | 5 min30 subs | 9 min54 subs |
| Celestron Origin Mark II10 s subs | 18% | 5 min30 subs | 5 min30 subs | 13 min76 subs |
Imaging the galaxy
Galaxies are broadband targets: their light is mostly starlight spread across the spectrum, so a dual-band filter throws most of it away and makes things slower, not faster. Shoot without a filter (or with a plain UV/IR cut) and rely on total time and a dark sky. The core of a galaxy is usually many times brighter than its outer disc, so a short stack shows the nucleus long before the arms; the figures here are for the arms and disc, not the core.
Field rotation in Alt-Az mode crops the edges of the stack over a long session, so on a big galaxy re-centre now and then or use EQ mode where your scope supports it.
Per-telescope pages
- How long to image the M32 with the ZWO Seestar S50
- How long to image the M32 with the ZWO Seestar S50 Pro
- How long to image the M32 with the ZWO Seestar S30
- How long to image the M32 with the ZWO Seestar S30 Pro
- How long to image the M32 with the DwarfLab DWARF 3
- How long to image the M32 with the DwarfLab DWARF mini
- How long to image the M32 with the DwarfLab Draco
- How long to image the M32 with the DwarfLab DWARF II
- How long to image the M32 with the Vaonis Vespera II
- How long to image the M32 with the Vaonis Vespera Pro
- How long to image the M32 with the Vaonis Vespera 3
- How long to image the M32 with the Vaonis Vespera Pro 2
- How long to image the M32 with the Unistellar eQuinox 2
- How long to image the M32 with the Unistellar Odyssey
- How long to image the M32 with the Celestron Origin
- How long to image the M32 with the Celestron Origin Mark II