Little Dumbbell

M76, NGC 650 · Planetary nebula in Perseus

Magnitude
10.1
Size
2.7′ × 1.8′
Effective surface brightness
21.3 mag/arcsec²
Best months
Sep, Oct, Nov
Declination
+52°
Filter
Dual-band recommended

A small, bright-per-pixel planetary in Perseus. Dual-band makes the two lobes and the faint wings much easier.

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 Little Dumbbell, 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 subs, dual-band6%25 min150 subs28 min168 subs41 min248 subs
ZWO Seestar S50 Pro10 s subs, dual-band3%28 min168 subs31 min188 subs46 min275 subs
ZWO Seestar S3010 s subs, dual-band41 px29 min175 subs32 min193 subs46 min274 subs
ZWO Seestar S30 Pro10 s subs, dual-band43 px30 min181 subs34 min202 subs49 min293 subs
DwarfLab DWARF 315 s subs, dual-band59 px31 min123 subs35 min142 subs56 min225 subs
DwarfLab DWARF mini15 s subs, dual-band41 px24 min98 subs28 min111 subs41 min164 subs
DwarfLab Draco30 s subs, dual-band4%20 min40 subs22 min45 subs33 min67 subs
DwarfLab DWARF II15 s subs54 px1 h 22 min330 subs1 h 50 min441 subs3 h 52 min927 subs
Vaonis Vespera II10 s subs3%20 min122 subs30 min182 subs1 h 14 min444 subs
Vaonis Vespera Pro10 s subs3%48 min289 subs1 h 09 min415 subs2 h 41 min966 subs
Vaonis Vespera 310 s subs3%19 min116 subs29 min173 subs1 h 11 min425 subs
Vaonis Vespera Pro 210 s subs3%45 min273 subs1 h 06 min394 subs2 h 34 min924 subs
Unistellar eQuinox 24 s subs8%24 min363 subs30 min457 subs58 min866 subs
Unistellar Odyssey4 s subs8%2 h 05 min1,870 subs2 h 27 min2,210 subs4 h 06 min3,697 subs
Celestron Origin10 s subs5%5 min30 subs8 min47 subs20 min122 subs
Celestron Origin Mark II10 s subs6%6 min39 subs10 min63 subs28 min171 subs

Open in the calculator

Imaging the planetary nebula

Planetary nebulae are small but intensely bright per pixel in OIII and H-alpha, so they respond very well to a dual-band filter and do not need much time for the main shell. The faint outer halos most of them have are a different proposition and need hours. Keep subs short if the central region saturates.

Per-telescope pages