Southern Pinwheel

M83, NGC 5236 · Galaxy in Hydra

Magnitude
7.6
Size
13′ × 12′
Effective surface brightness
21.7 mag/arcsec²
Best months
Mar, Apr, May
Declination
-30°
Filter
None (broadband target)

A bright barred spiral, superb from the southern hemisphere and a low-altitude struggle from northern Europe.

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 Southern Pinwheel, 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 subs30%19 min117 subs30 min182 subs1 h 18 min469 subs
ZWO Seestar S50 Pro10 s subs16%21 min129 subs33 min200 subs1 h 25 min511 subs
ZWO Seestar S3010 s subs18%22 min130 subs33 min196 subs1 h 20 min483 subs
ZWO Seestar S30 Pro10 s subs10%23 min138 subs35 min213 subs1 h 30 min540 subs
DwarfLab DWARF 315 s subs13%26 min104 subs43 min171 subs1 h 57 min467 subs
DwarfLab DWARF mini15 s subs18%19 min77 subs30 min121 subs1 h 18 min312 subs
DwarfLab Draco30 s subs17%16 min32 subs25 min50 subs1 h 05 min130 subs
DwarfLab DWARF II15 s subs12%1 h 23 min331 subs1 h 53 min452 subs4 h 06 min984 subs
Vaonis Vespera II10 s subs15%19 min117 subs30 min182 subs1 h 18 min469 subs
Vaonis Vespera Pro10 s subs13%47 min281 subs1 h 10 min419 subs2 h 50 min1,022 subs
Vaonis Vespera 310 s subs15%18 min111 subs29 min174 subs1 h 15 min449 subs
Vaonis Vespera Pro 210 s subs13%44 min266 subs1 h 06 min398 subs2 h 43 min978 subs
Unistellar eQuinox 24 s subs38%25 min372 subs32 min474 subs1 h 01 min921 subs
Unistellar Odyssey4 s subs39%2 h 10 min1,952 subs2 h 35 min2,324 subs4 h 23 min3,951 subs
Celestron Origin10 s subs25%5 min30 subs8 min47 subs21 min128 subs
Celestron Origin Mark II10 s subs29%6 min36 subs10 min63 subs30 min180 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