M71

NGC 6838 · Globular cluster in Sagitta

Magnitude
8.2
Size
7′
Effective surface brightness
20.8 mag/arcsec²
Best months
Jun, Jul, Aug
Declination
+19°
Filter
None (broadband target)

A loose globular in Sagitta that was long mistaken for an open cluster. Rich Milky Way background.

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 M71, 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 subs16%9 min57 subs13 min80 subs30 min180 subs
ZWO Seestar S50 Pro10 s subs8%10 min63 subs15 min88 subs33 min196 subs
ZWO Seestar S3010 s subs10%10 min62 subs14 min85 subs31 min185 subs
ZWO Seestar S30 Pro10 s subs5%11 min67 subs15 min93 subs34 min207 subs
DwarfLab DWARF 315 s subs7%13 min53 subs19 min77 subs45 min180 subs
DwarfLab DWARF mini15 s subs10%9 min38 subs13 min53 subs30 min120 subs
DwarfLab Draco30 s subs9%15 min30 subs15 min30 subs25 min50 subs
DwarfLab DWARF II15 s subs7%36 min146 subs47 min188 subs1 h 33 min374 subs
Vaonis Vespera II10 s subs8%9 min57 subs13 min80 subs30 min180 subs
Vaonis Vespera Pro10 s subs7%22 min133 subs30 min181 subs1 h 05 min392 subs
Vaonis Vespera 310 s subs8%9 min55 subs13 min77 subs29 min173 subs
Vaonis Vespera Pro 210 s subs7%21 min126 subs29 min172 subs1 h 02 min375 subs
Unistellar eQuinox 24 s subs20%10 min156 subs13 min191 subs23 min347 subs
Unistellar Odyssey4 s subs21%52 min774 subs1 h904 subs1 h 38 min1,472 subs
Celestron Origin10 s subs14%5 min30 subs5 min30 subs8 min50 subs
Celestron Origin Mark II10 s subs16%5 min30 subs5 min30 subs12 min70 subs

Open in the calculator

Imaging the globular cluster

Globular clusters are point sources packed tight, so they come quickly: the core resolves into stars within a handful of minutes on any smart scope. More time deepens the halo and pulls in the faint outer members. Use short subs so the core does not saturate into a white blob, and no filter.

Per-telescope pages