How long to image the M110 with the DwarfLab DWARF II

From a Bortle 6 suburban sky, the DwarfLab DWARF II needs about 13 h (3,119 subs of 15 s) for a solid image of the M110. A quick look takes 3 h 15 min; a showpiece 52 h. Under a Bortle 3 rural sky the solid figure drops to 6 h 21 min. At Bortle 6 the limit is a mix of skyglow and read noise. In this scope's field it fills 20% of the frame’s short side.

M110 with the DwarfLab DWARF II: 15 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site1 h 26 min343 subs5 h 42 min1,369 subs23 h5,474 subs
Bortle 2Typical dark site1 h 29 min356 subs5 h 56 min1,423 subs24 h5,689 subs
Bortle 3Rural1 h 35 min381 subs6 h 21 min1,524 subs25 h6,096 subs
Bortle 4Rural / suburban transition1 h 51 min443 subs7 h 23 min1,771 subs30 h7,081 subs
Bortle 5Suburban2 h 15 min541 subs9 h2,161 subs36 h8,643 subs
Bortle 6Bright suburban3 h 15 min780 subs13 h3,119 subs52 h12,476 subs
Bortle 7Suburban / urban transition5 h 09 min1,237 subs21 h4,945 subs82 h19,779 subs
Bortle 8City8 h 06 min1,945 subs32 h7,780 subs130+ h31,117 subs
Bortle 9Inner city14 h3,457 subs58 h13,825 subs230+ h55,299 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 17 h of run time. That is more than one night: over 3 nights, about 5 h 38 min each. The DWARF II’s battery is rated at about 3 h, so each night needs an external power bank. (Bortle 6, solid image; we allow 30% over the integration time.)

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Everything that fits the DWARF II →

How it frames

The M110 is 22′ × 11′ across. The DWARF II frames 3.19° × 1.79° at 2.99″ per pixel, so it fills 20% of the frame’s short side.

About the M110

Andromeda's larger, diffuse elliptical companion. Low surface brightness; it fades into the background in short stacks.

NGC 205 · Galaxy in Andromeda · magnitude 8.1 · 22′ × 11′ · best in Sep, Oct, Nov. 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 DwarfLab DWARF II

The original pocket scope. 24 mm aperture and tiny 1.45 µm pixels mean it is slow per pixel, so bin or downsample and be patient.

15 s is the hard maximum in any mode; DwarfLab recommends EQ mode at 15 s. Two built-in filters, VIS and Astro (IR-pass); no dual-band. The optional UHC filter is no longer sold.

The DWARF II uses fixed 15 s subs, so the only levers you have are the sky you shoot from, the filter, and total time.

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 M110 with your DWARF II? Did the solid figure match?Anonymous, one tap. It is how the model gets calibrated.

Have an image of the M110 from a DWARF 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 M110 · All targets for the DWARF II