How long to image the M108 with the DwarfLab DWARF II

From a Bortle 6 suburban sky, the DwarfLab DWARF II needs about 4 h 54 min (1,175 subs of 15 s) for a solid image of the M108. A quick look takes 1 h 13 min; a showpiece 20 h. Under a Bortle 3 rural sky the solid figure drops to 2 h 31 min. At Bortle 6 the limit is a mix of skyglow and read noise. In this scope's field it fills 8% of the frame’s short side.

M108 with the DwarfLab DWARF II: 15 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site34 min138 subs2 h 17 min549 subs9 h 09 min2,196 subs
Bortle 2Typical dark site36 min143 subs2 h 22 min569 subs9 h 28 min2,273 subs
Bortle 3Rural38 min152 subs2 h 31 min605 subs10 h2,418 subs
Bortle 4Rural / suburban transition43 min174 subs2 h 53 min693 subs12 h2,770 subs
Bortle 5Suburban52 min208 subs3 h 28 min832 subs14 h3,328 subs
Bortle 6Bright suburban1 h 13 min294 subs4 h 54 min1,175 subs20 h4,697 subs
Bortle 7Suburban / urban transition1 h 54 min457 subs7 h 37 min1,827 subs30 h7,305 subs
Bortle 8City2 h 57 min710 subs12 h2,839 subs47 h11,354 subs
Bortle 9Inner city5 h 12 min1,250 subs21 h4,998 subs83 h19,990 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 6 h 22 min of run time. The DWARF II’s battery is rated at about 3 h, so the session needs an external power bank. (Bortle 6, solid image; we allow 30% over the integration time.)

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How it frames

The M108 is 8.7′ × 2.2′ across. The DWARF II frames 3.19° × 1.79° at 2.99″ per pixel, so it fills 8% of the frame’s short side.

About the M108

An edge-on spiral with a mottled, dusty disc, a degree from the Owl Nebula. Frame both together.

NGC 3556 · Galaxy in Ursa Major · magnitude 10.0 · 8.7′ × 2.2′ · 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 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 M108 with your DWARF II? Did the solid figure match?Anonymous, one tap. It is how the model gets calibrated.

Have an image of the M108 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 M108 · All targets for the DWARF II