Orion Optics UK CT8 Optical Tube Assembly
- 200mm (8") Aperture
- 900mm Focal Length (f/4.5)
- 1/10 PV Wavefront Certified Optics
- Carbon Fiber Sandwich Tube Construction
- 7kg Optical Tube Weight
Simulate the exact field of view of the Orion Optics UK CT8 Optical Tube Assembly with your specific telescope.
Launch Visual Assistant
Simulate the exact field of view of the Orion Optics UK CT8 Optical Tube Assembly with your specific telescope.
Launch Imaging AssistantThe Orion Optics UK CT8 combines a fast f/4.5 focal ratio with a 200mm aperture, built around a hand-figured Suprax primary mirror certified to a 1/10 PV wavefront accuracy. This instrument is engineered for high-resolution imaging, weighing only 7kg thanks to its carbon fiber sandwich tube construction which measures 860mm in length. Every optical surface features Enhanced Hilux coatings for maximum light transmission, delivering views where contrast is limited only by atmospheric seeing, not the telescope's optical precision.
The heart of the CT8 is its 200mm primary mirror, figured to Orion Optics UK's highest "Ultra" grade of 1/10 PV wavefront. This is not a theoretical standard; each CT8 is delivered with its own Zygo laser interferometry report, verifying that its optical surface deviates from a perfect parabola by a fraction of a wavelength of light. The Suprax primary mirror, with its low thermal expansion, is finished with Enhanced Hilux coatings to ensure maximum reflectivity for capturing faint deep-sky detail.
The optical tube is a sandwich-construction carbon fiber design, providing extreme rigidity and near-zero thermal expansion. This physical stability is critical for a fast f/4.5 system, as it maintains a constant focal plane even as ambient temperatures change during an imaging session. At a mere 7kg, the 860mm long tube is easily managed by mid-range equatorial mounts, making it an accessible choice for imagers who demand optical perfection without requiring a massive support system.
Every mechanical component is designed to support the optical system's potential. The primary mirror rests on a 9-point flotation CNC machined cell that prevents flexure and is supported by a fan cooling system for rapid thermal stabilization. Upfront, a 2" focuser with reduction gearing allows for fine, repeatable focus adjustments, while the 63mm secondary mirror is held by a fully adjustable 4-vane spider and rotatable holder, ensuring precise collimation.
While many telescopes are described as "diffraction-limited" (equivalent to 1/4 PV wavefront), a 1/10 PV system delivers a fundamentally higher level of image fidelity. This difference is most apparent on high-contrast planetary and lunar targets. With 1/10 PV optics, you resolve finer, more stable detail within Jupiter's cloud bands, see the Cassini Division in Saturn's rings as a sharp black gap, and discern subtle rilles on the Moon that would be blurred or invisible in a lesser instrument.
A 1/10 PV wavefront means the mirror surface is exceptionally close to a perfect parabola. For planetary observers, this translates to higher contrast and sharper detail. You will see more subtle features in Jupiter's atmosphere, crisper definition in Saturn's rings, and finer details in lunar craters compared to standard 1/4 PV optics, especially during moments of good atmospheric seeing.
The fast f/4.5 focal ratio allows the 200mm aperture to gather light very quickly. When imaging a bright, extended object like the Orion Nebula (M42), this means you can capture significant detail in shorter sub-exposures. This reduces the demands on your mount's tracking accuracy and allows you to build up a deep, high-signal image in less total time.
Yes, particularly for astrophotography. Carbon fiber has virtually zero thermal expansion. As temperatures drop overnight, a metal tube will shrink, causing the focal point to shift and requiring refocusing. The CT8's carbon fiber tube holds focus stable throughout the night, which is a critical advantage for long imaging sessions.
The CT8 optical tube weighs 7kg, and the rings add another 1kg. A total payload of 8kg plus your camera and guide scope (likely 10-11kg total) requires a stable equatorial mount. Mounts in the EQ6/CEM40 class or larger are recommended for astrophotography to ensure tracking accuracy and stability.
No. The CT8 is supplied as an optical tube assembly optimized for astrophotography. It does not include eyepieces, a diagonal, or a barlow lens. You will need to supply your own 1.25" or 2" eyepieces for visual use. A quality coma corrector is also highly recommended for imaging with its fast f/4.5 optics.
The 9-point suspension mirror cell provides uniform support to the back of the 200mm primary mirror. This prevents the mirror from sagging or deforming under its own weight as the telescope points to different parts of the sky, which would degrade the image. This precise mechanical support is essential to maintaining the certified 1/10 PV optical quality in practice.
| Aperture | 200mm |
| Focal Length | 900mm |
| Focal Ratio | f/4.5 |
| Optical Grade | 1/10 PV wavefront |
| Primary Mirror Glass | Suprax |
| Optical Coatings | Enhanced Hilux |
| Secondary Mirror Size | 63mm |
| Tube Material | Carbon fibre sandwich |
| Tube Diameter | 255mm |
| Tube Length | 860mm |
| Optical Tube Weight | 7kg |
| Focuser | 2" focuser with reduction gearing |
| Mirror Cell | CNC machined aluminium, 9 point suspension |
| Spider | Adjustable 4-vane, stainless steel |
| Secondary Holder | Machined aluminium, rotatable |
| Finderscope | 8x50 |
| Extension Tubes | 40mm long, screw threaded |
| Tube Rings | CNC machined, anodised black |
| Weight of Rings | 1kg |
| Boxed Dimensions | 87x48x48mm |
| Boxed Weight | 10.7kg |
CT8 Carbon Tube OTA
× 1
CNC Tube Rings
× 2
8x50 Finderscope with Bracket
× 1
40mm Extension Tube
× 1
Zygo Interferometry Test Report
× 1