Abell 39

PN A66 39 · Planetary nebula in Hercules

Magnitude
13.7
Size
2.9′
Effective surface brightness
23.5 mag/arcsec²
Best months
May, Jun, Jul
Declination
+28°
Filter
Dual-band recommended

A near-perfect faint sphere in Hercules. Very low surface brightness, an OIII target for dark skies and long dual-band stacks.

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 Abell 39, 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-band7%14 h5,179 subs17 h6,236 subs30 h10,857 subs
ZWO Seestar S50 Pro10 s subs, dual-band4%17 h5,951 subs20 h7,095 subs34 h12,092 subs
ZWO Seestar S3010 s subs, dual-band44 px18 h6,632 subs21 h7,689 subs34 h12,310 subs
ZWO Seestar S30 Pro10 s subs, dual-band47 px18 h6,514 subs21 h7,716 subs36 h12,974 subs
DwarfLab DWARF 315 s subs, dual-band3%15 h3,564 subs19 h4,653 subs39 h9,411 subs
DwarfLab DWARF mini15 s subs, dual-band44 px14 h3,365 subs17 h4,070 subs30 h7,150 subs
DwarfLab Draco30 s subs, dual-band4%11 h1,317 subs13 h1,611 subs24 h2,895 subs
DwarfLab DWARF II15 s subs58 px61 h14,555 subs87 h20,950 subs200+ h48,902 subs
Vaonis Vespera II10 s subs3%13 h4,588 subs22 h8,041 subs64 h23,135 subs
Vaonis Vespera Pro10 s subs3%32 h11,572 subs52 h18,832 subs140+ h50,567 subs
Vaonis Vespera 310 s subs3%12 h4,333 subs21 h7,649 subs62 h22,145 subs
Vaonis Vespera Pro 210 s subs3%30 h10,885 subs50 h17,858 subs130+ h48,336 subs
Unistellar eQuinox 24 s subs8%19 h17,165 subs25 h22,546 subs51 h46,065 subs
Unistellar Odyssey4 s subs9%100+ h94,040 subs130+ h113,618 subs220+ h199,189 subs
Celestron Origin10 s subs6%2 h 52 min1,032 subs5 h 35 min2,012 subs17 h6,294 subs
Celestron Origin Mark II10 s subs6%3 h 25 min1,233 subs7 h 20 min2,643 subs24 h8,809 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