How long to image the M19 with the Vaonis Vespera 3

From a Bortle 6 suburban sky, the Vaonis Vespera 3 needs about 20 min (122 subs of 10 s) for a solid image of the M19. A quick look takes 5 min; a showpiece 1 h 21 min. Under a Bortle 3 rural sky the solid figure drops to 9 min. At Bortle 6 the limit is skyglow, so a darker site or a filter helps more than longer subs. In this scope's field it fills 19% of the frame’s short side.

M19 with the Vaonis Vespera 3: 10 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site2 min12 subs8 min47 subs31 min188 subs
Bortle 2Typical dark site2 min13 subs8 min50 subs33 min197 subs
Bortle 3Rural2 min14 subs9 min54 subs36 min215 subs
Bortle 4Rural / suburban transition3 min17 subs11 min65 subs43 min257 subs
Bortle 5Suburban3 min21 subs13 min81 subs54 min323 subs
Bortle 6Bright suburban5 min31 subs20 min122 subs1 h 21 min486 subs
Bortle 7Suburban / urban transition8 min50 subs33 min200 subs2 h 13 min797 subs
Bortle 8City13 min80 subs53 min320 subs3 h 33 min1,280 subs
Bortle 9Inner city24 min145 subs1 h 36 min578 subs6 h 25 min2,309 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 26 min of run time. The Vespera 3’s battery (rated about 11 h) should cover it; a power bank still keeps the phone running the app alive. (Bortle 6, solid image; we allow 30% over the integration time.)

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How it frames

The M19 is 17′ across. The Vespera 3 frames 2.60° × 1.46° at 2.44″ per pixel, so it fills 19% of the frame’s short side.

Longer subs

10 s subs by default; Expert Mode manual targets allow 1 to 30 s. Alt-azimuth only; CovalENS mosaic widens the field to 4.3° × 2.4°. Time for a solid image by sub length:

Sub lengthBortle 3Bortle 5Bortle 7
10 s9 min54 subs13 min81 subs33 min200 subs
20 s10 min30 subs12 min38 subs32 min97 subs
30 s15 min30 subs15 min30 subs32 min64 subs

About the M19

The most oblate of the globulars, visibly elongated. Low in the south from mid-northern latitudes.

NGC 6273 · Globular cluster in Ophiuchus · magnitude 6.8 · 17′ · best in May, Jun, Jul. Reachable from mid-northern latitudes (UK, northern US, central Europe) and from the south.

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.

About the Vaonis Vespera 3

The 2026 Vespera: same 50 mm quadruplet class as the II on an 8 MP IMX585, with a 24 MP mosaic mode and 11 hours of battery. Per pixel it behaves like a Seestar S50 Pro without the built-in dual-band filter.

10 s subs by default; Expert Mode manual targets allow 1 to 30 s. Alt-azimuth only; CovalENS mosaic widens the field to 4.3° × 2.4°. Optional clip-on Vaonis filters: dual-band, light-pollution (CLS) and solar. The new optical baffle is not a substitute for a CLS filter.

Longer subs matter most under dark skies, where read noise rather than skyglow sets the floor. From a city the difference between 10 s and 30 s subs is small; from a rural site it can halve the total time, especially with a dual-band filter in place.

Stack across nights. Every smart scope app can continue a stack or you can combine the saved frames on a computer; the figures here are totals, not single-session limits.

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Imaged the M19 with your Vespera 3? Did the solid figure match?Anonymous, one tap. It is how the model gets calibrated.

Have an image of the M19 from a Vespera 3? Email it with your total time and sky to [email protected] and it goes here, credited.

Same target, other telescopes

All telescopes for the M19 · All targets for the Vespera 3