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

Total integration for a solid image of the M32, default sub length, recommended filter, and how much of each frame it fills. Click a cell for the full Bortle 1 to 9 table.
TelescopeIn frameBortle 3 (rural)Bortle 5 (suburban)Bortle 7 (urban edge)
ZWO Seestar S5010 s subs19%10 min60 subs14 min85 subs33 min196 subs
ZWO Seestar S50 Pro10 s subs10%11 min66 subs15 min93 subs35 min213 subs
ZWO Seestar S3010 s subs11%11 min65 subs15 min90 subs33 min201 subs
ZWO Seestar S30 Pro10 s subs6%12 min70 subs16 min99 subs37 min225 subs
DwarfLab DWARF 315 s subs8%14 min55 subs20 min81 subs49 min196 subs
DwarfLab DWARF mini15 s subs11%10 min40 subs14 min57 subs33 min131 subs
DwarfLab Draco30 s subs11%15 min30 subs15 min30 subs27 min54 subs
DwarfLab DWARF II15 s subs7%39 min155 subs50 min202 subs1 h 42 min407 subs
Vaonis Vespera II10 s subs9%10 min60 subs14 min85 subs33 min196 subs
Vaonis Vespera Pro10 s subs8%23 min139 subs32 min193 subs1 h 11 min426 subs
Vaonis Vespera 310 s subs9%9 min57 subs13 min81 subs31 min188 subs
Vaonis Vespera Pro 210 s subs8%22 min132 subs31 min184 subs1 h 08 min407 subs
Unistellar eQuinox 24 s subs23%11 min167 subs14 min206 subs25 min379 subs
Unistellar Odyssey4 s subs24%56 min837 subs1 h 05 min981 subs1 h 47 min1,609 subs
Celestron Origin10 s subs16%5 min30 subs5 min30 subs9 min54 subs
Celestron Origin Mark II10 s subs18%5 min30 subs5 min30 subs13 min76 subs

Open in the calculator

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