How long to image the M96 with the Vaonis Vespera II

From a Bortle 6 suburban sky, the Vaonis Vespera II needs about 1 h 37 min (580 subs of 10 s) for a solid image of the M96. A quick look takes 24 min; a showpiece 6 h 26 min. Under a Bortle 3 rural sky the solid figure drops to 39 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 9% of the frame’s short side.

M96 with the Vaonis Vespera II: 10 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site8 min51 subs34 min203 subs2 h 15 min809 subs
Bortle 2Typical dark site9 min54 subs36 min214 subs2 h 22 min855 subs
Bortle 3Rural10 min59 subs39 min236 subs2 h 37 min943 subs
Bortle 4Rural / suburban transition12 min73 subs48 min289 subs3 h 13 min1,156 subs
Bortle 5Suburban16 min94 subs1 h 02 min373 subs4 h 09 min1,492 subs
Bortle 6Bright suburban24 min145 subs1 h 37 min580 subs6 h 26 min2,319 subs
Bortle 7Suburban / urban transition41 min244 subs2 h 42 min974 subs11 h3,893 subs
Bortle 8City1 h 06 min397 subs4 h 24 min1,585 subs18 h6,338 subs
Bortle 9Inner city2 h722 subs8 h 01 min2,888 subs32 h11,552 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 2 h 06 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 M96 is 7.6′ × 5.2′ across. The Vespera II frames 2.55° × 1.44° at 2.39″ per pixel, so it fills 9% 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 s39 min236 subs1 h 02 min373 subs2 h 42 min974 subs
20 s34 min102 subs57 min171 subs2 h 37 min471 subs
30 s32 min65 subs55 min111 subs2 h 35 min311 subs

About the M96

The brightest of the M95/M96/M105 group, a slightly asymmetric spiral.

NGC 3368 · Galaxy in Leo · magnitude 9.2 · 7.6′ × 5.2′ · 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 M96 with your Vespera II? Did the solid figure match?Anonymous, one tap. It is how the model gets calibrated.

Have an image of the M96 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 M96 · All targets for the Vespera II