NGC 7331

Caldwell 30 · Galaxy in Pegasus

Magnitude
9.5
Size
10′ × 4′
Effective surface brightness
22.1 mag/arcsec²
Best months
Aug, Sep, Oct
Declination
+34°
Filter
None (broadband target)

A tilted spiral often compared to the Milky Way, with a group of background galaxies alongside. Stephan's Quintet is half a degree away.

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 NGC 7331, 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 subs23%49 min296 subs1 h 20 min482 subs3 h 36 min1,294 subs
ZWO Seestar S50 Pro10 s subs12%55 min330 subs1 h 28 min531 subs3 h 55 min1,409 subs
ZWO Seestar S3010 s subs14%56 min335 subs1 h 27 min521 subs3 h 42 min1,333 subs
ZWO Seestar S30 Pro10 s subs7%59 min354 subs1 h 34 min565 subs4 h 08 min1,489 subs
DwarfLab DWARF 315 s subs10%1 h 05 min259 subs1 h 52 min450 subs5 h 21 min1,286 subs
DwarfLab DWARF mini15 s subs14%49 min195 subs1 h 20 min319 subs3 h 35 min861 subs
DwarfLab Draco30 s subs13%39 min79 subs1 h 05 min131 subs2 h 58 min357 subs
DwarfLab DWARF II15 s subs9%3 h 38 min874 subs5 h 05 min1,219 subs11 h2,722 subs
Vaonis Vespera II10 s subs12%49 min296 subs1 h 20 min482 subs3 h 36 min1,294 subs
Vaonis Vespera Pro10 s subs10%2 h 01 min726 subs3 h 06 min1,117 subs7 h 51 min2,824 subs
Vaonis Vespera 310 s subs11%47 min281 subs1 h 16 min459 subs3 h 26 min1,239 subs
Vaonis Vespera Pro 210 s subs10%1 h 54 min685 subs2 h 57 min1,060 subs7 h 30 min2,700 subs
Unistellar eQuinox 24 s subs29%1 h 07 min1,000 subs1 h 26 min1,290 subs2 h 50 min2,555 subs
Unistellar Odyssey4 s subs30%5 h 56 min5,338 subs7 h 06 min6,392 subs12 h10,996 subs
Celestron Origin10 s subs20%12 min70 subs20 min123 subs59 min353 subs
Celestron Origin Mark II10 s subs22%14 min87 subs27 min163 subs1 h 22 min494 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