Pinwheel Galaxy

M101, NGC 5457 · Galaxy in Ursa Major

Magnitude
7.9
Size
29′ × 27′
Effective surface brightness
22.8 mag/arcsec²
Best months
Apr, May, Jun
Declination
+54°
Filter
None (broadband target)

Big, face-on and faint. Its total magnitude is flattering; spread over half a degree the arms are dim and demand hours, especially from suburban skies.

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 Pinwheel Galaxy, 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 subs67%1 h 40 min602 subs2 h 51 min1,025 subs7 h 59 min2,873 subs
ZWO Seestar S50 Pro10 s subs35%1 h 52 min672 subs3 h 08 min1,129 subs8 h 41 min3,128 subs
ZWO Seestar S3010 s subs40%1 h 55 min689 subs3 h 05 min1,112 subs8 h 13 min2,960 subs
ZWO Seestar S30 Pro10 s subs22%2 h722 subs3 h 20 min1,203 subs9 h 11 min3,306 subs
DwarfLab DWARF 315 s subs29%2 h 08 min514 subs3 h 57 min949 subs12 h2,852 subs
DwarfLab DWARF mini15 s subs40%1 h 39 min396 subs2 h 49 min678 subs7 h 57 min1,910 subs
DwarfLab Draco30 s subs39%1 h 20 min160 subs2 h 19 min278 subs6 h 35 min791 subs
DwarfLab DWARF II15 s subs27%7 h 44 min1,856 subs11 h2,639 subs25 h6,061 subs
Vaonis Vespera II10 s subs34%1 h 40 min602 subs2 h 51 min1,025 subs7 h 59 min2,873 subs
Vaonis Vespera Pro10 s subs30%4 h 10 min1,501 subs6 h 38 min2,390 subs17 h6,275 subs
Vaonis Vespera 310 s subs33%1 h 35 min569 subs2 h 42 min975 subs7 h 38 min2,750 subs
Vaonis Vespera Pro 210 s subs29%3 h 56 min1,414 subs6 h 18 min2,267 subs17 h5,998 subs
Unistellar eQuinox 24 s subs85%2 h 24 min2,164 subs3 h 08 min2,823 subs6 h 20 min5,702 subs
Unistellar Odyssey4 s subs86%13 h11,739 subs16 h14,136 subs27 h24,611 subs
Celestron Origin10 s subs57%23 min138 subs43 min258 subs2 h 10 min782 subs
Celestron Origin Mark II10 s subs65%28 min168 subs57 min340 subs3 h 02 min1,095 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