How long to image the Centaurus A with the DwarfLab DWARF II

From a Bortle 6 suburban sky, the DwarfLab DWARF II needs about 2 h 19 min (557 subs of 15 s) for a solid image of the Centaurus A. A quick look takes 35 min; a showpiece 9 h 17 min. Under a Bortle 3 rural sky the solid figure drops to 1 h 12 min. At Bortle 6 the limit is a mix of skyglow and read noise. In this scope's field it fills 24% of the frame’s short side.

Centaurus A with the DwarfLab DWARF II: 15 s subs.
SkyQuick lookTarget obvious, still noisySolidClean enough to shareShowpieceSmooth faint detail, print-worthy
Bortle 1Excellent dark site16 min66 subs1 h 06 min264 subs4 h 23 min1,054 subs
Bortle 2Typical dark site17 min69 subs1 h 08 min273 subs4 h 33 min1,091 subs
Bortle 3Rural18 min73 subs1 h 12 min290 subs4 h 50 min1,159 subs
Bortle 4Rural / suburban transition21 min83 subs1 h 23 min331 subs5 h 31 min1,324 subs
Bortle 5Suburban25 min100 subs1 h 39 min397 subs6 h 36 min1,586 subs
Bortle 6Bright suburban35 min140 subs2 h 19 min557 subs9 h 17 min2,228 subs
Bortle 7Suburban / urban transition54 min216 subs3 h 36 min864 subs14 h3,453 subs
Bortle 8City1 h 24 min335 subs5 h 35 min1,339 subs22 h5,353 subs
Bortle 9Inner city2 h 27 min588 subs9 h 48 min2,352 subs39 h9,407 subs

Adjust in the calculator

Power and kit for this session

Allowing for slewing, focusing and rejected subs, that is about 3 h 01 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 Centaurus A is 26′ × 20′ across. The DWARF II frames 3.19° × 1.79° at 2.99″ per pixel, so it fills 24% of the frame’s short side.

About the Centaurus A

A giant elliptical with a thick dust band across it, the brightest radio galaxy in the sky. A southern-hemisphere showpiece.

NGC 5128, Caldwell 77 · Galaxy in Centaurus · magnitude 6.8 · 26′ × 20′ · best in Mar, Apr, May. Low or below the horizon from northern Europe; best from the southern US southwards.

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

Have an image of the Centaurus A 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 Centaurus A · All targets for the DWARF II