How long to image the M66 with the Vaonis Vespera II

From a Bortle 6 suburban sky, the Vaonis Vespera II needs about 41 min (246 subs of 10 s) for a solid image of the M66. A quick look takes 10 min; a showpiece 2 h 44 min. Under a Bortle 3 rural sky the solid figure drops to 18 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 10% of the frame’s short side.

M66 with the Vaonis Vespera II: 10 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site4 min24 subs16 min94 subs1 h 02 min375 subs
Bortle 2Typical dark site4 min25 subs16 min99 subs1 h 06 min394 subs
Bortle 3Rural4 min27 subs18 min108 subs1 h 11 min429 subs
Bortle 4Rural / suburban transition5 min33 subs21 min129 subs1 h 26 min515 subs
Bortle 5Suburban7 min41 subs27 min163 subs1 h 48 min651 subs
Bortle 6Bright suburban10 min62 subs41 min246 subs2 h 44 min984 subs
Bortle 7Suburban / urban transition17 min102 subs1 h 07 min405 subs4 h 30 min1,619 subs
Bortle 8City27 min163 subs1 h 49 min652 subs7 h 14 min2,605 subs
Bortle 9Inner city49 min295 subs3 h 16 min1,177 subs13 h4,707 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 53 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 M66 is 9′ × 4′ across. The Vespera II frames 2.55° × 1.44° at 2.39″ per pixel, so it fills 10% 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 s18 min108 subs27 min163 subs1 h 07 min405 subs
20 s16 min48 subs25 min75 subs1 h 05 min196 subs
30 s15 min30 subs24 min49 subs1 h 05 min130 subs

About the M66

The brightest of the Leo Triplet, with asymmetric arms from a past encounter.

NGC 3627 · Galaxy in Leo · magnitude 8.9 · 9′ × 4′ · best in Feb, Mar, Apr. Reachable from mid-northern latitudes (UK, northern US, central Europe) and from the south.

Galaxies are broadband targets: their light is mostly starlight spread across the spectrum, so a dual-band filter throws most of it away and makes things slower, not faster. Shoot without a filter (or with a plain UV/IR cut) and rely on total time and a dark sky. The core of a galaxy is usually many times brighter than its outer disc, so a short stack shows the nucleus long before the arms; the figures here are for the arms and disc, not the core.

Field rotation in Alt-Az mode crops the edges of the stack over a long session, so on a big galaxy re-centre now and then or use EQ mode where your scope supports it.

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 M66 with your Vespera II? Did the solid figure match?Anonymous, one tap. It is how the model gets calibrated.

Have an image of the M66 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 M66 · All targets for the Vespera II