Blinking Planetary

NGC 6826, Caldwell 15 · Planetary nebula in Cygnus

Magnitude
8.8
Size
0.5′ × 0.4′
Effective surface brightness
20.5 mag/arcsec²
Best months
Jun, Jul, Aug
Declination
+51°
Filter
Dual-band recommended

Named for a visual trick, it is a small bright disc around a bright central star. Quick.

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 Blinking Planetary, 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-band13 px9 min52 subs9 min56 subs12 min74 subs
ZWO Seestar S50 Pro10 s subs, dual-band13 px9 min57 subs10 min62 subs14 min82 subs
ZWO Seestar S3010 s subs, dual-band8 px9 min57 subs10 min62 subs13 min80 subs
ZWO Seestar S30 Pro10 s subs, dual-band8 px10 min61 subs11 min66 subs14 min87 subs
DwarfLab DWARF 315 s subs, dual-band11 px11 min46 subs13 min51 subs17 min69 subs
DwarfLab DWARF mini15 s subs, dual-band8 px8 min34 subs9 min37 subs12 min49 subs
DwarfLab Draco30 s subs, dual-band21 px15 min30 subs15 min30 subs15 min30 subs
DwarfLab DWARF II15 s subs10 px24 min98 subs31 min124 subs59 min235 subs
Vaonis Vespera II10 s subs13 px7 min40 subs9 min54 subs19 min114 subs
Vaonis Vespera Pro10 s subs18 px15 min92 subs20 min120 subs41 min247 subs
Vaonis Vespera 310 s subs12 px6 min38 subs9 min52 subs18 min109 subs
Vaonis Vespera Pro 210 s subs18 px14 min87 subs19 min115 subs39 min236 subs
Unistellar eQuinox 24 s subs23 px7 min102 subs8 min124 subs14 min217 subs
Unistellar Odyssey4 s subs32 px33 min496 subs38 min574 subs1 h 01 min915 subs
Celestron Origin10 s subs20 px5 min30 subs5 min30 subs5 min32 subs
Celestron Origin Mark II10 s subs24 px5 min30 subs5 min30 subs7 min44 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