FirstRig
firstrig.com

Takahashi FC-76DCU with Player One Ares-C Pro

1.36″ per pixel across a 1.14° × 1.14° field, at 570 mm and f/7.5. 25 of the catalogue's 29 equatorial mounts carry the 4.57 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 the native focal length.

Focal length570mmnative
Focal ratiof/7.576 mm aperture
Image scale1.36″/px3.76 µm pixels
Field of view1.14 × 1.14°68′ × 68′
Sensor11.31 × 11.31mm15.99 mm diagonal; no image circle published

No corrector for this telescope is in the catalogue, so these figures are at the native focal length.

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 1.84 pixels on this sensor. Practical band for typical seeing.

Star FWHM in pixels at three seeing conditions
SeeingFWHMBand
1.5″1.10pxundersampled
2.5″1.84pxpractical
3.5″2.57pxpractical
  • Undersampled; the standard, deliberate wide-field trade.
  • Practical band for typical seeing.

Framing

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

M31 Andromeda Galaxy fills 261 % of the frame and M27 Dumbbell Nebula 10 %. Of the 13, 3 fill the frame, 2 are a tight crop, 4 need a mosaic, 4 are small in the frame.

1.14° × 1.14°261 % · 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 Takahashi FC-76DCU with the Player One Ares-C Pro: size, frame filled and fit
TargetSizeFrame filled
M31 Andromeda Galaxy178′ × 70′261%needs a mosaic
M45 Pleiades150′ × 150′220%needs a mosaic
NGC 7000 North America Nebula120′ × 30′176%needs a mosaic
NGC 1499 California Nebula160′ × 40′235%needs a mosaic
IC 1805 Heart Nebula60′ × 60′88%fills the frame
M42 Orion Nebula90′ × 60′132%tight crop
NGC 2237 Rosette Nebula80′ × 50′117%tight crop
M101 Pinwheel Galaxy24′ × 23′35%fills the frame
M27 Dumbbell Nebula6.7′ × 6.7′10%small in the frame
M51 Whirlpool Galaxy13.7′ × 11.7′20%small in the frame
M81 Bode's Galaxy22′ × 11.3′32%fills the frame
M13 Hercules Globular Cluster16.5′ × 16.5′24%small in the frame
NGC 4565 Needle Galaxy16.8′ × 2.9′25%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, and none for it is in the catalogue yet. The maker: “76Dレデューサーを取り付けると417mm(F/5.5)に、FC/FSマルチフラットナー1.04×を取り付けると590mm(F/7.8)になり、それぞれで35mmフルサイズの イメージサークルまでフラットフィールドで青ハローのほとんどない星像が撮影できます。” Source

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 4.57 kg, 2.25 kg of it assumed. 25 of the 29 equatorial mounts in the catalogue carry it within the derate; the smallest rated is the ZWO AM3N, at 57 %. 4 more would run it over 60 %.

Mounts that carry the Takahashi FC-76DCU with the Player One Ares-C Pro, smallest rated payload first
MountRatedUsedBand
ZWO AM3N8kg57%Workable; more sensitive to wind, little room to grow
iOptron HEM158.2kg56%Workable; more sensitive to wind, little room to grow
Sky-Watcher Wave 100i10kg46%Comfortable
iOptron CEM26 (AccuAlign, 1.5" tripod)12kg38%Headroom for a future upgrade
iOptron GEM28 (AccuAlign, 1.5" tripod)12.7kg36%Headroom for a future upgrade
iOptron HEM2713.5kg34%Headroom for a future upgrade
The other 19 mounts that carry it
The remaining mounts that carry this train, by rated payload
MountRatedUsedBand
Rainbow Astro RST-135E13.5kg34%Headroom for a future upgrade
WarpAstron WD-1713.5kg34%Headroom for a future upgrade
Celestron Advanced VX (AVX)13.6kg34%Headroom for a future upgrade
Pegasus Astro NYX-8814kg33%Headroom for a future upgrade
Sky-Watcher HEQ5-R Pro15kg30%Headroom for a future upgrade
Sky-Watcher Wave 150i15kg30%Headroom for a future upgrade
ZWO AM5N15kg30%Headroom for a future upgrade
Celestron CGEM II18kg25%Headroom for a future upgrade
iOptron CEM40 (with tripod)18kg25%Headroom for a future upgrade
iOptron HEM4420kg23%Headroom for a future upgrade
Pegasus Astro NYX-10120kg23%Headroom for a future upgrade
Sky-Watcher EQ6-R Pro20kg23%Headroom for a future upgrade
WarpAstron WD-2020kg23%Headroom for a future upgrade
ZWO AM720kg23%Headroom for a future upgrade
Losmandy GM811G (LW tripod)22.7kg20%Headroom for a future upgrade
Celestron CGX25kg18%Headroom for a future upgrade
iOptron CEM70 (iPolar)31.8kg14%Headroom for a future upgrade
Sky-Watcher CQ350 Pro (with tripod)35kg13%Headroom for a future upgrade
Sky-Watcher EQ8-R (head with counterweights)50kg9%Headroom for a future upgrade
What the 4.57 kg is made of
The imaging payload, component by component
ComponentMassBasis
OTA: Takahashi FC-76DCU1.90kgmaker’s figure
Rings and dovetail0.90kgassumption
Camera: Player One Ares-C Pro0.42kgmaker’s figure
Filter drawer and filter0.20kgassumption
Guide scope and guide camera0.80kgassumption
Cables, dew strap, focuser motor0.35kgassumption
Total4.57kg

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 Player One Ares-C 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 125 (high conversion gain on, 1.376 e⁻ read noise), 76 mm at 570 mm. Under a Bortle 6 sky it is 12 s with no filter and 226 s through a 7 nm dual-band filter.

Shortest sub for the Player One Ares-C Pro on the Takahashi FC-76DCU, by sky and filter
SkyNo filter7 nm dual-band
Bortle 421.00 mag/arcsec²79 s24 min
Bortle 619.00 mag/arcsec²12 sbelow the 30 s floor226 s
Bortle 817.90 mag/arcsec²4.5 sbelow the 30 s floor82 s
  • 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 Takahashi FC-76DCU and the Player One Ares-C Pro
PartPriceRead
Telescope: Takahashi FC-76DCUProvisional$1,300retailer, 2026-09-27FC-76DCU OTA only (SKU TFK07640); in stock 2026-09-27. OPT lists the same SKU at $1,600 but unavailable (https://optcorp.com/products/takahashi-fc-76dcu-refractor-telescope).
Camera: Player One Ares-C ProProvisional$799manufacturer, 2026-09-27camera only (the page's 'Camera' option); import tax may be extra

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 Takahashi FC-76DCU