How long to image the M62 with the Vaonis Vespera II

From a Bortle 6 suburban sky, the Vaonis Vespera II needs about 8 min (50 subs of 10 s) for a solid image of the M62. A quick look takes 2 min; a showpiece 33 min. Under a Bortle 3 rural sky the solid figure drops to 5 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 17% of the frame’s short side.

M62 with the Vaonis Vespera II: 10 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site2 min10 subs5 min30 subs15 min91 subs
Bortle 2Typical dark site2 min10 subs5 min30 subs16 min94 subs
Bortle 3Rural2 min10 subs5 min30 subs17 min100 subs
Bortle 4Rural / suburban transition2 min10 subs5 min30 subs19 min115 subs
Bortle 5Suburban2 min10 subs6 min35 subs23 min140 subs
Bortle 6Bright suburban2 min13 subs8 min50 subs33 min199 subs
Bortle 7Suburban / urban transition3 min20 subs13 min78 subs52 min312 subs
Bortle 8City5 min31 subs20 min122 subs1 h 21 min487 subs
Bortle 9Inner city9 min54 subs36 min216 subs2 h 23 min861 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 11 min of run time. The Vespera II’s battery (rated about 4 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 M62 is 15′ across. The Vespera II frames 2.55° × 1.44° at 2.39″ per pixel, so it fills 17% 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, no EQ mode. Time for a solid image by sub length:

Sub lengthBortle 3Bortle 5Bortle 7
10 s5 min30 subs6 min35 subs13 min78 subs
20 s10 min30 subs10 min30 subs13 min38 subs
30 s15 min30 subs15 min30 subs15 min30 subs

About the M62

A bright but lopsided globular near the galactic centre, low from northern latitudes.

NGC 6266 · Globular cluster in Ophiuchus · magnitude 6.5 · 15′ · 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 II

A 50 mm quadruplet on an 8 MP sensor with Vaonis’s mosaic mode for wide fields. Same optics class as the Seestar S50, four times the pixels.

10 s subs by default; Expert Mode manual targets allow 1 to 30 s. Alt-azimuth only, no EQ mode. Optional clip-on Vaonis filters: dual-band, light-pollution (CLS) and solar; the app detects which is fitted.

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 M62 with your Vespera II? Did the solid figure match?Anonymous, one tap. It is how the model gets calibrated.

Have an image of the M62 from a Vespera II? Email it with your total time and sky to [email protected] and it goes here, credited.

Same target, other telescopes

All telescopes for the M62 · All targets for the Vespera II