M5

NGC 5904 · Globular cluster in Serpens

Magnitude
5.7
Size
23′
Effective surface brightness
20.9 mag/arcsec²
Best months
Apr, May, Jun
Declination
+2°
Filter
None (broadband target)

A bright, slightly elliptical globular in Serpens that rivals M13 and resolves into stars quickly.

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 M5, 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 subs53%5 min30 subs7 min43 subs16 min97 subs
ZWO Seestar S50 Pro10 s subs28%5 min33 subs8 min47 subs18 min106 subs
ZWO Seestar S3010 s subs32%5 min33 subs7 min45 subs17 min100 subs
ZWO Seestar S30 Pro10 s subs17%6 min35 subs8 min50 subs19 min112 subs
DwarfLab DWARF 315 s subs23%8 min30 subs10 min41 subs24 min97 subs
DwarfLab DWARF mini15 s subs32%8 min30 subs8 min30 subs16 min65 subs
DwarfLab Draco30 s subs31%15 min30 subs15 min30 subs15 min30 subs
DwarfLab DWARF II15 s subs21%19 min77 subs25 min101 subs50 min201 subs
Vaonis Vespera II10 s subs27%5 min30 subs7 min43 subs16 min97 subs
Vaonis Vespera Pro10 s subs24%12 min70 subs16 min96 subs35 min211 subs
Vaonis Vespera 310 s subs26%5 min30 subs7 min41 subs15 min93 subs
Vaonis Vespera Pro 210 s subs23%11 min66 subs15 min92 subs34 min202 subs
Unistellar eQuinox 24 s subs67%6 min83 subs7 min102 subs12 min187 subs
Unistellar Odyssey4 s subs68%28 min415 subs32 min485 subs53 min794 subs
Celestron Origin10 s subs45%5 min30 subs5 min30 subs5 min30 subs
Celestron Origin Mark II10 s subs51%5 min30 subs5 min30 subs6 min38 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