How long to image the Rosette Nebula with the Vaonis Vespera 3

From a Bortle 6 suburban sky, the Vaonis Vespera 3 needs about 2 h 09 min (777 subs of 10 s) for a solid image of the Rosette Nebula. A quick look takes 32 min; a showpiece 8 h 37 min. Under a Bortle 3 rural sky the solid figure drops to 48 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 only just fits, at 91% of the short side.

Rosette Nebula with the Vaonis Vespera 3: 10 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site10 min61 subs40 min243 subs2 h 41 min969 subs
Bortle 2Typical dark site11 min65 subs43 min259 subs2 h 52 min1,035 subs
Bortle 3Rural12 min73 subs48 min290 subs3 h 13 min1,159 subs
Bortle 4Rural / suburban transition15 min92 subs1 h 01 min365 subs4 h 03 min1,459 subs
Bortle 5Suburban20 min121 subs1 h 21 min484 subs5 h 23 min1,936 subs
Bortle 6Bright suburban32 min195 subs2 h 09 min777 subs8 h 37 min3,105 subs
Bortle 7Suburban / urban transition56 min334 subs3 h 42 min1,334 subs15 h5,333 subs
Bortle 8City1 h 32 min550 subs6 h 06 min2,199 subs24 h8,793 subs
Bortle 9Inner city2 h 48 min1,011 subs11 h4,043 subs45 h16,170 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 2 h 48 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, and 30% off the battery for a January night.)

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How it frames

The Rosette Nebula is 80′ × 60′ across. The Vespera 3 frames 2.60° × 1.46° at 2.44″ per pixel, so it only just fits, at 91% of the short side. Centre it carefully: there is no room to crop back afterwards.

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 s48 min290 subs1 h 21 min484 subs3 h 42 min1,334 subs
20 s41 min123 subs1 h 13 min221 subs3 h 35 min645 subs
30 s39 min78 subs1 h 11 min142 subs3 h 32 min425 subs

With and without the dual-band filter

Solid quality, default sub length.
FilterBortle 3Bortle 5Bortle 7
No filter48 min290 subs1 h 21 min484 subs3 h 42 min1,334 subs
dual-band (Dual Band filter), clip-on56 min334 subs1 h 06 min394 subs1 h 49 min654 subs

The Vespera 3 has no built-in dual-band filter. Optional clip-on Vaonis filters: dual-band, light-pollution (CLS) and solar. The new optical baffle is not a substitute for a CLS filter. On an emission target like this it is the single biggest upgrade you can make.

About the Rosette Nebula

A ring of hydrogen more than a degree across around the cluster NGC 2244. One of the best dual-band targets of winter and forgiving of light pollution.

NGC 2237, NGC 2244, Caldwell 49 · Emission nebula in Monoceros · magnitude 9.0 · 80′ × 60′ · best in Dec, Jan, Feb. Reachable from mid-northern latitudes (UK, northern US, central Europe) and from the south.

Emission nebulae glow in a few narrow lines, mostly hydrogen-alpha (deep red) and doubly ionised oxygen (teal). A dual-band filter passes those lines and blocks most skyglow, which is why it cuts the time needed from a suburban sky so dramatically. Use it. From a genuinely dark site the gain is smaller because there is less skyglow to block, and read noise becomes the limit, which is where longer subs (EQ mode, or Expert Mode on a Vespera) earn their keep.

Stars lose colour through a dual-band filter; a short broadband stack blended in fixes that if you care.

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

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Same target, other telescopes

All telescopes for the Rosette Nebula · All targets for the Vespera 3