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Askar 103APO with ZWO ASI585MC Pro

0.85″ per pixel across a 0.91° × 0.51° field, at 700.4 mm and f/6.8. 20 of the catalogue's 29 equatorial mounts carry the 8.05 kg train within the imaging derate.

Every figure is computed from catalogue rows that link their maker's page. Rows marked provisional have not yet had a second, human check.

Optics

At 700.4 mm, with the Askar 1.0x Full-frame Flattener for 103APO. The other 2 configurations are in the table below.

Focal length700.4mmnative; the corrector is 1.0x
Focal ratiof/6.8103 mm aperture
Image scale0.85″/px2.9 µm pixels
Field of view0.91 × 0.51°55′ × 31′
Sensor11.136 × 6.264mm12.78 mm diagonal; 44 mm circle stated
Each configuration of the Askar 103APO with the ZWO ASI585MC Pro
ConfigurationFocal lengthRatioScaleField
Askar 1.0x Full-frame Flattener for 103APO700.4mmf/6.80.85″/px0.91° × 0.51°
Askar 0.8x Full-frame Reducer for 103APO560.3mmf/5.41.07″/px1.14° × 0.64°
Askar 0.6x Full-frame Reducer for 103APO420.2mmf/4.11.42″/px1.52° × 0.85°

Image circle: 44 mm, the corrector's stated figure (Askar 1.0x Full-frame Flattener for 103APO). Source

Sampling

Seeing divided by image scale: how many pixels a star's core spans. Each band is a tradeoff, and wide-field work is undersampled on purpose.

At 2.5″ seeing a star’s core spans 2.93 pixels on this sensor. Practical band for typical seeing.

Star FWHM in pixels at three seeing conditions, for each configuration
Seeing1.0x · 700.4 mm0.8x · 560.3 mm0.6x · 420.2 mm
1.5″1.76pxpractical1.41pxpractical1.05pxundersampled
2.5″2.93pxpractical2.34pxpractical1.76pxpractical
3.5″4.10pxoversampled3.28pxoversampled2.46pxpractical
  • Practical band for typical seeing.
  • Oversampled: lower per-pixel signal and tighter guiding; binning recovers most of it.
  • Undersampled; the standard, deliberate wide-field trade.

Framing

The 13 catalogue targets against this field, by the fraction of the frame each fills along its tighter axis.

M45 Pleiades fills 488 % of the frame and M27 Dumbbell Nebula 22 %. Of the 13, 5 fill the frame, 7 need a mosaic, 1 is small in the frame.

0.91° × 0.51°325 % · needs a mosaic
Target drawn at true angular size against this rig’s sensor, at native focal length. The glow and stars are synthetic, not survey imagery; the size is OpenNGC’s.

Open in the framing tool, at any camera angle

The 13 targets against the Askar 103APO with the ZWO ASI585MC Pro: size, frame filled and fit
TargetSize1.0x · 700.4 mm0.8x · 560.3 mm0.6x · 420.2 mm
M31 Andromeda Galaxy178′ × 70′325%needs a mosaic260%needs a mosaic195%needs a mosaic
M45 Pleiades150′ × 150′488%needs a mosaic390%needs a mosaic293%needs a mosaic
NGC 7000 North America Nebula120′ × 30′220%needs a mosaic176%needs a mosaic132%tight crop
NGC 1499 California Nebula160′ × 40′293%needs a mosaic234%needs a mosaic176%needs a mosaic
IC 1805 Heart Nebula60′ × 60′195%needs a mosaic156%needs a mosaic117%tight crop
M42 Orion Nebula90′ × 60′195%needs a mosaic156%needs a mosaic117%tight crop
NGC 2237 Rosette Nebula80′ × 50′163%needs a mosaic130%tight crop98%tight crop
M101 Pinwheel Galaxy24′ × 23′75%fills the frame60%fills the frame45%fills the frame
M27 Dumbbell Nebula6.7′ × 6.7′22%small in the frame17%small in the frame13%small in the frame
M51 Whirlpool Galaxy13.7′ × 11.7′38%fills the frame30%fills the frame23%small in the frame
M81 Bode's Galaxy22′ × 11.3′40%fills the frame32%fills the frame24%small in the frame
M13 Hercules Globular Cluster16.5′ × 16.5′54%fills the frame43%fills the frame32%fills the frame
NGC 4565 Needle Galaxy16.8′ × 2.9′31%fills the frame25%small in the frame18%small in the frame

Target sizes: OpenNGC by Mattia Verga (tag v20260501), CC BY-SA 4.0. This table is shared under the same license. Source and license

Spacing

The corrector rows this telescope links in the Backfocus Solver's catalogue, with the face each figure is measured from.

This telescope needs a corrector. The maker: “1x flattener (optional) ... The flattener corrects field curvature and coma, resulting in flatter field edges and finer star points.” Source

  • Askar 1.0x Full-frame Flattener for 103APO

    Backfocus
    55mm
    Measured from
    base of the M48x0.75 male thread on the flattener's M54-M48 adapter
    Focal length
    1.0x, 700.4 mm
    Image circle
    44 mm; this sensor is 12.78 mm

    Solve the spacer stack with this cameraSource

  • Askar 0.8x Full-frame Reducer for 103APO

    Backfocus
    55mm
    Measured from
    base of the M48x0.75 male thread on the reducer's M54-M48 adapter
    Focal length
    0.8x, 560.3 mm
    Image circle
    44 mm; this sensor is 12.78 mm

    Solve the spacer stack with this cameraSource

  • Askar 0.6x Full-frame Reducer for 103APO

    Backfocus
    55mm
    Measured from
    base of the M48x0.75 male thread on the reducer's M54-M48 adapter
    Focal length
    0.6x, 420.2 mm
    Image circle
    44 mm; this sensor is 12.78 mm

    Solve the spacer stack with this cameraSource

Mounts

The catalogue's equatorial mounts that carry this train within 60 % of their rated payload, the imaging derate. The sum is the Rig Reality Check's.

On the saddle this train weighs 8.05 kg, 2.25 kg of it assumed. 20 of the 29 equatorial mounts in the catalogue carry it within the derate; the smallest rated is the iOptron HEM27, at 60 %. 9 more would run it over 60 %.

Mounts that carry the Askar 103APO with the ZWO ASI585MC Pro, smallest rated payload first
MountRatedUsedBand
iOptron HEM2713.5kg60%Workable; more sensitive to wind, little room to grow
Rainbow Astro RST-135E13.5kg60%Workable; more sensitive to wind, little room to grow
WarpAstron WD-1713.5kg60%Workable; more sensitive to wind, little room to grow
Celestron Advanced VX (AVX)13.6kg59%Workable; more sensitive to wind, little room to grow
Pegasus Astro NYX-8814kg58%Workable; more sensitive to wind, little room to grow
Sky-Watcher HEQ5-R Pro15kg54%Workable; more sensitive to wind, little room to grow
The other 14 mounts that carry it
The remaining mounts that carry this train, by rated payload
MountRatedUsedBand
Sky-Watcher Wave 150i15kg54%Workable; more sensitive to wind, little room to grow
ZWO AM5N15kg54%Workable; more sensitive to wind, little room to grow
Celestron CGEM II18kg45%Comfortable
iOptron CEM40 (with tripod)18kg45%Comfortable
iOptron HEM4420kg40%Comfortable
Pegasus Astro NYX-10120kg40%Comfortable
Sky-Watcher EQ6-R Pro20kg40%Comfortable
WarpAstron WD-2020kg40%Comfortable
ZWO AM720kg40%Comfortable
Losmandy GM811G (LW tripod)22.7kg35%Headroom for a future upgrade
Celestron CGX25kg32%Headroom for a future upgrade
iOptron CEM70 (iPolar)31.8kg25%Headroom for a future upgrade
Sky-Watcher CQ350 Pro (with tripod)35kg23%Headroom for a future upgrade
Sky-Watcher EQ8-R (head with counterweights)50kg16%Headroom for a future upgrade
What the 8.05 kg is made of
The imaging payload, component by component
ComponentMassBasis
OTA: Askar 103APO4.75kgmaker’s figure
Rings and dovetail0.90kgassumption
Corrector: Askar 1.0x Full-frame Flattener for 103APO0.58kgmaker’s figure
Camera: ZWO ASI585MC Pro0.47kgmaker’s figure
Filter drawer and filter0.20kgassumption
Guide scope and guide camera0.80kgassumption
Cables, dew strap, focuser motor0.35kgassumption
Total8.05kg

Assumptions are the Rig Reality Check’s round placeholders, not measurements; replace them with your own figures there.

Run the Rig Reality Check with the ZWO ASI585MC Pro as yours, then give it your budget, sky and targets.

Sub length

The shortest sub at which read noise adds no more than 5 % to the stack's noise, from the Exposure Planner. Each figure opens the planner with the same inputs.

At gain 200 (high conversion gain on, 1.1 e⁻ read noise), 103 mm at 700.4 mm. Under a Bortle 6 sky it is 9.7 s with no filter and 176 s through a 7 nm dual-band filter.

Shortest sub for the ZWO ASI585MC Pro on the Askar 103APO, by sky and filter
SkyNo filter7 nm dual-band
Bortle 421.00 mag/arcsec²61 s50 s to 73 s18 min15 min to 22 min
Bortle 619.00 mag/arcsec²9.7 s8.0 s to 12 sbelow the 30 s floor176 s145 s to 209 s
Bortle 817.90 mag/arcsec²3.5 s2.9 s to 4.2 sbelow the 30 s floor64 s53 s to 76 s
  • The read noise is read off the maker’s chart; the small figures give the range its reading uncertainty allows.
  • Under 30 s, download and dither time dominate, so the planner raises shorter results to 30 s. The dual-band column uses the reference’s approximation: Dual narrowband 7 nm (Ha + OIII).

Prices

Dated readings from the maker's store or a major US retailer, with the page each came from. A first-year total needs a mount and the essentials, which the Rig Reality Check adds.

Dated prices for the Askar 103APO and the ZWO ASI585MC Pro
PartPriceRead
Telescope: Askar 103APOProvisional$1,199retailer, 2026-09-27OTA only (SKU ASK-103APO); flattener/reducers sold separately
Camera: ZWO ASI585MC ProProvisional$599manufacturer, 2026-09-27variant ASI585MC Pro
$599retailer, 2026-09-27
Corrector: Askar 1.0x Full-frame Flattener for 103APOProvisional$219retailer, 2026-09-27SKU ASK-103APO-1FLAT
Corrector: Askar 0.8x Full-frame Reducer for 103APOProvisional$219retailer, 2026-09-27SKU ASK-103APO-08XR
Corrector: Askar 0.6x Full-frame Reducer for 103APOProvisional$329retailer, 2026-09-27SKU ASK-103APO-06XR

Provisional rows have not yet had a second, human check against their source. The Rig Reality Check prices whole builds, essentials included.

How this is computed

scale["/px]    = 206.265 × pixel[µm] / focal length[mm]
field[°]       = 2 × atan(sensor side[mm] / (2 × focal length[mm])) × 180/π
sampling       = seeing FWHM["] / scale["/px]
frame filled   = max(major axis / field width, minor axis / field height)
utilization    = Σ imaging mass[kg] / rated payload[kg]
shortest sub   = R² / (e_sky × ((1 + p)² − 1)),   p = 5 %

Focal length is the telescope’s, times a corrector’s factor only where its maker states one. The image scale and field use the exact forms; the worked example shows the arithmetic. The sampling bands are the physics reference’s presentation choice, and every band is printed so the tradeoff can be read in full.

The payload sums every part on the saddle, the way the Rig Reality Check does, and the bands encode the 50 to 60 % imaging derate, which is forum practice rather than a maker’s figure. Spacing figures are the Backfocus Solver’s rows; sub lengths are the Exposure Planner’s.

Source: docs/03-physics-reference.md §§ 1, 3 and 4. Implemented in packages/physics (optics.ts, payload.ts, exposure.ts, scoring.ts), each with the reference's worked examples as unit tests.

Last updated Computed from the catalogue when the site is builtEvery camera on the Askar 103APO