Andromeda Galaxy

M31, NGC 224 · Galaxy in Andromeda

Magnitude
3.4
Size
178′ × 63′
Effective surface brightness
22.2 mag/arcsec²
Best months
Sep, Oct, Nov
Declination
+41°
Filter
None (broadband target)

The nearest big spiral and the most imaged galaxy in the sky. The core arrives in minutes, the dust lanes in an hour, the faint outer disc needs a whole night. Too big for most smart-scope fields without mosaic.

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 Andromeda Galaxy, default sub length, recommended filter. Click a cell for the full Bortle 1 to 9 table.
TelescopeBortle 3 (rural)Bortle 5 (suburban)Bortle 7 (urban edge)
ZWO Seestar S5010 s subs46 min279 subs1 h 08 min408 subs2 h 41 min969 subs
ZWO Seestar S50 Pro10 s subs38 min227 subs1 h 01 min366 subs2 h 42 min973 subs
ZWO Seestar S3010 s subs34 min204 subs55 min332 subs2 h 29 min893 subs
ZWO Seestar S30 Pro10 s subs40 min243 subs1 h 05 min389 subs2 h 51 min1,028 subs
DwarfLab Dwarf 315 s subs55 min219 subs1 h 28 min351 subs3 h 52 min929 subs
DwarfLab Dwarf Mini15 s subs31 min123 subs52 min208 subs2 h 25 min582 subs
DwarfLab Dwarf II15 s subs2 h 31 min603 subs3 h 30 min840 subs7 h 50 min1,879 subs
Vaonis Vespera II10 s subs34 min204 subs55 min332 subs2 h 29 min893 subs
Vaonis Vespera Pro10 s subs1 h 39 min596 subs2 h 24 min866 subs5 h 41 min2,045 subs
Unistellar eQuinox 24 s subs46 min690 subs59 min890 subs1 h 58 min1,764 subs
Unistellar Odyssey4 s subs4 h 05 min3,683 subs4 h 54 min4,410 subs8 h 26 min7,591 subs
Celestron Origin10 s subs8 min48 subs14 min85 subs41 min244 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