How long to image the M77 with the Vaonis Vespera II

From a Bortle 6 suburban sky, the Vaonis Vespera II needs about 30 min (182 subs of 10 s) for a solid image of the M77. A quick look takes 8 min; a showpiece 2 h 01 min. Under a Bortle 3 rural sky the solid figure drops to 14 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 8% of the frame’s short side.

M77 with the Vaonis Vespera II: 10 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site3 min19 subs13 min76 subs50 min301 subs
Bortle 2Typical dark site3 min20 subs13 min79 subs52 min314 subs
Bortle 3Rural4 min22 subs14 min85 subs56 min339 subs
Bortle 4Rural / suburban transition4 min25 subs17 min100 subs1 h 06 min398 subs
Bortle 5Suburban5 min31 subs21 min124 subs1 h 22 min493 subs
Bortle 6Bright suburban8 min46 subs30 min182 subs2 h 01 min725 subs
Bortle 7Suburban / urban transition12 min73 subs49 min292 subs3 h 14 min1,167 subs
Bortle 8City19 min116 subs1 h 17 min464 subs5 h 09 min1,854 subs
Bortle 9Inner city35 min208 subs2 h 18 min830 subs9 h 13 min3,319 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 39 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, and 30% off the battery for a November night.)

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How it frames

The M77 is 7′ × 6′ across. The Vespera II frames 2.55° × 1.44° at 2.39″ per pixel, so it fills 8% 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 s14 min85 subs21 min124 subs49 min292 subs
20 s13 min38 subs19 min58 subs47 min142 subs
30 s15 min30 subs19 min38 subs47 min94 subs

About the M77

A Seyfert galaxy with a blazing core and faint outer arms. The nucleus is easy; the arms are not.

NGC 1068 · Galaxy in Cetus · magnitude 8.9 · 7′ × 6′ · best in Oct, Nov, Dec. 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 M77 with your Vespera II? Did the solid figure match?Anonymous, one tap. It is how the model gets calibrated.

Have an image of the M77 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 M77 · All targets for the Vespera II