{"title":"Orion Optics UK CT Carbon Newtonian Telescopes","description":"\u003cp\u003eOrion Optics UK CT carbon Newtonian telescopes are optical tube assemblies built around a carbon fibre tube, which is lighter than steel and changes length very little as the temperature drops, so focus holds better through the night. The line includes the CT8, CT10, CT12, CT14 and CT16, plus the CT10L and CT12L with longer focal lengths.\u003c\/p\u003e\u003cp\u003eThe standard versions suit deep-sky imaging and wide views, while the L models favour higher magnification on planets and the Moon.\u003c\/p\u003e","products":[{"product_id":"orion-optics-uk-ct8-optical-tube-assembly","title":"Orion Optics UK CT8 Optical Tube Assembly","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e200mm (8\") Aperture\u003c\/li\u003e\n\u003cli\u003e900mm Focal Length (f\/4.5)\u003c\/li\u003e\n\u003cli\u003e1\/10 PV Wavefront Certified Optics\u003c\/li\u003e\n\u003cli\u003eCarbon Fiber Sandwich Tube Construction\u003c\/li\u003e\n\u003cli\u003e7kg Optical Tube Weight\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section-center\"\u003e\n      \u003ch2\u003eOrion Optics UK CT8 Optical Tube Assembly\u003c\/h2\u003e\n      \u003cp\u003eThe 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.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eUltra-Grade Optics: A Certified 1\/10 PV Wavefront System\u003c\/h3\u003e\n      \u003cp\u003eThe 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.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n    \n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eCarbon Fiber Construction: A 7kg Tube with Zero Thermal Expansion\u003c\/h3\u003e\n      \u003cp\u003eThe 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.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eImaging-Ready Mechanics: 9-Point Cell and Precision 2\" Focuser\u003c\/h3\u003e\n      \u003cp\u003eEvery 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.\u003c\/p\u003e\n      \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003eCNC Tube Rings:\u003c\/strong\u003e A pair of anodised black, CNC machined rings weighing 1kg provides a secure mounting platform for the OTA.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eIncluded Finder:\u003c\/strong\u003e An 8x50 achromatic finderscope helps in locating and centering targets before imaging.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eExtension Tube:\u003c\/strong\u003e A 40mm screw-threaded extension tube is included to help achieve focus with a variety of cameras and accessories.\u003c\/li\u003e\n      \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eThe 1\/10 PV Advantage: What You See vs. Standard 1\/4 PV Optics\u003c\/h3\u003e\n      \u003cp\u003eWhile 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.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n\u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the 1\/10 PV wavefront of the CT8 mean for planetary viewing?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eA \u003cstrong\u003e1\/10 PV wavefront\u003c\/strong\u003e 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.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the f\/4.5 focal ratio of the CT8 benefit deep-sky imaging of the Orion Nebula (M42)?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe fast \u003cstrong\u003ef\/4.5 focal ratio\u003c\/strong\u003e 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.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eIs the CT8's carbon fiber tube worth it over an aluminum tube?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eYes, particularly for astrophotography. Carbon fiber has virtually \u003cstrong\u003ezero thermal expansion\u003c\/strong\u003e. 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.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of mount is needed for the 7kg CT8 optical tube?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe CT8 optical tube weighs \u003cstrong\u003e7kg\u003c\/strong\u003e, and the rings add another \u003cstrong\u003e1kg\u003c\/strong\u003e. 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.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the CT8 come with eyepieces or a diagonal?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eNo. 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.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the purpose of the 9-point mirror cell on the CT8?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe \u003cstrong\u003e9-point suspension mirror cell\u003c\/strong\u003e 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.\u003c\/p\u003e\n  \u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003ctable class=\"DAV-specifications\"\u003e\n    \u003ctbody\u003e\n      \u003ctr\u003e\n\u003ctd\u003eAperture\u003c\/td\u003e\n\u003ctd\u003e200mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocal Length\u003c\/td\u003e\n\u003ctd\u003e900mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd\u003ef\/4.5\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eOptical Grade\u003c\/td\u003e\n\u003ctd\u003e1\/10 PV wavefront\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003ePrimary Mirror Glass\u003c\/td\u003e\n\u003ctd\u003eSuprax\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eOptical Coatings\u003c\/td\u003e\n\u003ctd\u003eEnhanced Hilux\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSecondary Mirror Size\u003c\/td\u003e\n\u003ctd\u003e63mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Material\u003c\/td\u003e\n\u003ctd\u003eCarbon fibre sandwich\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Diameter\u003c\/td\u003e\n\u003ctd\u003e255mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Length\u003c\/td\u003e\n\u003ctd\u003e860mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eOptical Tube Weight\u003c\/td\u003e\n\u003ctd\u003e7kg\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocuser\u003c\/td\u003e\n\u003ctd\u003e2\" focuser with reduction gearing\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMirror Cell\u003c\/td\u003e\n\u003ctd\u003eCNC machined aluminium, 9 point suspension\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSpider\u003c\/td\u003e\n\u003ctd\u003eAdjustable 4-vane, stainless steel\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSecondary Holder\u003c\/td\u003e\n\u003ctd\u003eMachined aluminium, rotatable\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFinderscope\u003c\/td\u003e\n\u003ctd\u003e8x50\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eExtension Tubes\u003c\/td\u003e\n\u003ctd\u003e40mm long, screw threaded\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Rings\u003c\/td\u003e\n\u003ctd\u003eCNC machined, anodised black\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eWeight of Rings\u003c\/td\u003e\n\u003ctd\u003e1kg\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBoxed Dimensions\u003c\/td\u003e\n\u003ctd\u003e87x48x48mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBoxed Weight\u003c\/td\u003e\n\u003ctd\u003e10.7kg\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003c\/tbody\u003e\n  \u003c\/table\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cul class=\"DAV-grid\"\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003eCT8 Carbon Tube OTA\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003eCNC Tube Rings\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 2\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003e8x50 Finderscope with Bracket\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003e40mm Extension Tube\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003eZygo Interferometry Test Report\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n  \u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/orion-optics-uk-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eOrion Optics UK 1-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Orion Optics UK","offers":[{"title":"Default Title","offer_id":52942379417885,"sku":"OOUK-CT8-OPTICAL-TUBE-ASSEMBLY","price":3132.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Logo_3d62404a-c67e-4a94-b599-38773701bfec.jpg?v=1789607180"},{"product_id":"orion-optics-uk-ct10-optical-tube-assembly","title":"Orion Optics UK CT10 Optical Tube Assembly","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e250mm (10\") Aperture Newtonian Reflector\u003c\/li\u003e\n\u003cli\u003e1200mm Focal Length\u003c\/li\u003e\n\u003cli\u003ef\/4.8 Focal Ratio\u003c\/li\u003e\n\u003cli\u003eGuaranteed 1\/10 PV Wavefront Optics\u003c\/li\u003e\n\u003cli\u003eCarbon Fibre Sandwich Construction Tube\u003c\/li\u003e\n\u003cli\u003e9-Point CNC Machined Mirror Cell\u003c\/li\u003e\n\u003cli\u003e2\" Focuser with Reduction Gearing\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eOrion Optics UK CT10 Optical Tube Assembly\u003c\/h2\u003e\n\u003cp\u003eThe Orion Optics UK CT10 sets an uncompromising standard for high-resolution imaging, built around a hand-figured 250mm Suprax primary mirror guaranteed to a 1\/10 PV wavefront accuracy. Its fast f\/4.8 focal ratio and 1200mm focal length provide the image scale needed for detailed views of planets and deep-sky targets. Housed in a 1050mm carbon fibre sandwich tube and supported by a 9-point CNC-machined cell, the CT10 delivers optical perfection with the mechanical stability required to achieve it.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUltra-Grade 1\/10 PV Optics: The Apex of Newtonian Performance\u003c\/h3\u003e\n\u003cp\u003eThe heart of the CT10 is its 250mm primary mirror, figured to Orion Optics UK's highest \"Ultra\" grade of 1\/10 Peak-to-Valley (PV) wavefront. This level of precision, verified by an included Zygo interferometer report, ensures that the maximum amount of light is focused into a single point, producing images with exceptional contrast and sharpness. Paired with enhanced Hilux coatings, the optical system delivers maximum light transmission for brighter views of faint objects.\u003c\/p\u003e\n\u003cp\u003eCompared to standard \"diffraction-limited\" 1\/4 PV optics, a 1\/10 PV mirror minimizes scattered light and resolves finer details, a critical advantage for separating tight double stars or discerning subtle cloud bands on Jupiter. This isn't an optional upgrade; it's the standard for the CT series, built for observers who demand the highest possible fidelity from their instrument.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eCarbon Fibre Sandwich Tube: 1050mm of Thermal Stability\u003c\/h3\u003e\n\u003cp\u003eTo maintain the precision of its optics, the CT10 employs a carbon fibre sandwich tube with a 300mm diameter. This advanced material has a near-zero coefficient of thermal expansion, meaning the 1200mm focal length remains constant even as ambient temperatures drop during an observing session. This eliminates the need for constant refocusing, a common issue with aluminum or steel tube telescopes, making it ideal for long-exposure astrophotography.\u003c\/p\u003e\n\u003cp\u003eThe 1050mm tube is finished with a gloss exterior and a matte black interior to absorb stray light and maximize image contrast. At a weight of only 11kg, the CT10 OTA is manageable for a wide range of equatorial mounts capable of supporting its payload and length.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePrecision Mechanics: A 9-Point Cell and 2\" Geared Focuser\u003c\/h3\u003e\n\u003cp\u003eAn exceptional mirror requires an equally capable support system. The CT10 features a CNC-machined 9-point flotation cell that supports the 250mm primary mirror without introducing any print-through or astigmatism. This ensures the mirror's lab-tested accuracy is realized at the eyepiece. The secondary mirror is held in a rigid, rotatable aluminum holder by a fully adjustable 4-vane stainless steel spider, minimizing diffraction effects.\u003c\/p\u003e\n\u003cp\u003eFor critical focusing, the CT10 is equipped with a 2\" focuser with reduction gearing, allowing for smooth, minute adjustments essential for achieving sharp focus at high magnifications or with an imaging camera. The optical train is completed with a pair of CNC-machined tube rings, providing a secure and stable mounting platform for the 11kg tube assembly.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the 1\/10 PV wavefront accuracy of the CT10 mean for visual observing?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA \u003cstrong\u003e1\/10 PV wavefront\u003c\/strong\u003e means the primary mirror's surface is exceptionally close to a perfect parabola. For visual observers, this translates to higher contrast and sharpness, especially on challenging targets. You'll notice crisper detail in planetary cloud bands, tighter star points, and the ability to resolve faint companion stars closer to their brighter primaries. It ensures you are seeing everything the telescope's 250mm aperture is capable of resolving.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the CT10's carbon fibre tube help with astrophotography?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003ecarbon fibre sandwich tube\u003c\/strong\u003e has virtually zero thermal expansion. During a long imaging session, temperature changes can cause metal tubes to shrink, shifting the focal plane and ruining sharp focus. The CT10's tube holds focus rigidly throughout the night, preventing focus drift in your sub-exposures and resulting in consistently sharp images from start to finish.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the f\/4.8 focal ratio of the CT10 good for imaging galaxies like the Andromeda Galaxy (M31)?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, the \u003cstrong\u003ef\/4.8 focal ratio\u003c\/strong\u003e is considered fast and is excellent for deep-sky imaging. It allows you to collect a significant amount of light in shorter exposure times compared to slower f\/8 or f\/10 systems. While a coma corrector (sold separately) is recommended for achieving perfect star shapes across the entire field with large camera sensors, the CT10's combination of aperture and speed makes it a powerful instrument for capturing faint details in galaxies and nebulae.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of mount is required for the Orion Optics UK CT10?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe CT10 optical tube weighs \u003cstrong\u003e11kg\u003c\/strong\u003e and the rings add another \u003cstrong\u003e1.5kg\u003c\/strong\u003e, for a total of 12.5kg (approx. 27.5 lbs) before adding a camera or other accessories. For stable astrophotography, you should choose a German Equatorial Mount with a payload capacity of at least 40-45 lbs (approx. 20kg) to ensure rigidity and accurate tracking.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Orion Optics UK CT10 for high-magnification views of Jupiter's Great Red Spot?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The CT10 is an exceptional planetary instrument. Its guaranteed \u003cstrong\u003e1\/10 PV wavefront\u003c\/strong\u003e optics, combined with the large \u003cstrong\u003e250mm aperture\u003c\/strong\u003e for high resolution, will deliver incredibly detailed and high-contrast views of Jupiter, Saturn, and Mars when seeing conditions permit. The precision 2\" focuser with reduction gearing is crucial for achieving the critical focus needed at the high magnifications required for such observations.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the CT10's 9-point mirror cell for a 250mm mirror?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA \u003cstrong\u003e9-point flotation cell\u003c\/strong\u003e provides optimized support for the 250mm (10-inch) primary mirror. It distributes the mirror's \u003cstrong\u003e11kg\u003c\/strong\u003e weight evenly across nine points, preventing gravitational sag or flexure as the telescope moves. This ensures the mirror retains its precise 1\/10 PV shape, free from any induced astigmatism, regardless of where the telescope is pointed in the sky.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptics Grade\u003c\/td\u003e\n\u003ctd\u003e1\/10 PV Wavefront\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAperture\u003c\/td\u003e\n\u003ctd\u003e250mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocal Length\u003c\/td\u003e\n\u003ctd\u003e1200mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd\u003ef\/4.8\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePrimary Mirror Glass\u003c\/td\u003e\n\u003ctd\u003eSuprax\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eCoatings\u003c\/td\u003e\n\u003ctd\u003eEnhanced Hilux\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSecondary Mirror Size\u003c\/td\u003e\n\u003ctd\u003e63mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Material\u003c\/td\u003e\n\u003ctd\u003eCarbon fibre sandwich\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Diameter\u003c\/td\u003e\n\u003ctd\u003e300mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Length\u003c\/td\u003e\n\u003ctd\u003e1050mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Weight\u003c\/td\u003e\n\u003ctd\u003e11kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocuser\u003c\/td\u003e\n\u003ctd\u003e2\" focuser with reduction gearing\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFinder Scope\u003c\/td\u003e\n\u003ctd\u003e8x50\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMirror Cell\u003c\/td\u003e\n\u003ctd\u003eCNC machined aluminium, 9 point suspension\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSpider\u003c\/td\u003e\n\u003ctd\u003eAdjustable 4 vane, stainless steel\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSecondary Holder\u003c\/td\u003e\n\u003ctd\u003eMachined aluminium, rotatable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMounting Rings\u003c\/td\u003e\n\u003ctd\u003eCNC machined tube rings, anodised black\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRing Weight\u003c\/td\u003e\n\u003ctd\u003e1.5kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExtension Tubes\u003c\/td\u003e\n\u003ctd\u003e40mm long, screw threaded\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBoxed Dimensions\u003c\/td\u003e\n\u003ctd\u003e128x52x52mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBoxed Weight\u003c\/td\u003e\n\u003ctd\u003e17kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/orion-optics-uk-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eOrion Optics UK 1-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Orion Optics UK","offers":[{"title":"Default Title","offer_id":52942379516189,"sku":"OOUK-CT10-OPTICAL-TUBE-ASSEMBLY","price":4356.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Logo_ae8497e7-2f2c-4d11-b94e-f91dc5d21578.jpg?v=1789607188"},{"product_id":"orion-optics-uk-ct10l-optical-tube-assembly","title":"Orion Optics UK CT10L Optical Tube Assembly","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e250mm (10-inch) Aperture\u003c\/li\u003e\n\u003cli\u003e1575mm Focal Length (f\/6.3)\u003c\/li\u003e\n\u003cli\u003eGuaranteed 1\/10 PV Wavefront Optics\u003c\/li\u003e\n\u003cli\u003eCarbon Fibre Sandwich Tube Construction\u003c\/li\u003e\n\u003cli\u003e12.5kg Optical Tube Weight\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section-center\"\u003e\n      \u003ch2\u003eOrion Optics UK CT10L Optical Tube Assembly\u003c\/h2\u003e\n      \u003cp\u003eThe Orion Optics UK CT10L is an instrument of uncompromising optical quality, built around a 250mm f\/6.3 primary mirror hand-figured to a guaranteed 1\/10 PV wavefront accuracy. Its 1575mm focal length provides the magnification needed for detailed planetary observation, while the carbon fibre tube, measuring 1440mm long, ensures focus remains stable as temperatures change. Weighing just 12.5kg, this OTA delivers research-grade optical performance in a package manageable by mid-range equatorial mounts.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eGuaranteed 1\/10 PV Wavefront Optics: The Pinnacle of Newtonian Correction\u003c\/h3\u003e\n      \u003cp\u003eThe heart of the CT10L is its 250mm Suprax primary mirror, which is not just diffraction-limited, but corrected to the highest possible standard offered by Orion Optics UK. A 1\/10 PV wavefront figure means the mirror surface deviates from a perfect parabola by an incredibly small margin, resulting in maximum contrast and sharpness. Every CT10L is delivered with its own Zygo laser interferometry report, providing certified proof of its elite optical quality.\u003c\/p\u003e\n      \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003eEnhanced Hilux Coatings:\u003c\/strong\u003e Multi-layer dielectric coatings deliver superior reflectivity for brighter images compared to standard aluminum.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003e50mm Secondary Mirror:\u003c\/strong\u003e A precisely sized secondary provides full illumination for visual use and smaller imaging sensors without excessive obstruction.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eCertified Performance:\u003c\/strong\u003e The included Zygo test report documents the exact wavefront error of your specific mirror, removing all ambiguity about its performance.\u003c\/li\u003e\n      \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eZero-Expansion Carbon Fibre Tube: A 1440mm Stable Optical Platform\u003c\/h3\u003e\n      \u003cp\u003eTo maintain the precision of its optics, the CT10L employs a sandwich-construction carbon fibre tube. This material exhibits virtually zero thermal expansion, preventing the focal point from shifting during long imaging sessions or nights with dropping temperatures. The 300mm diameter tube is finished with a gloss exterior and a matte black interior to absorb stray light and maximize image contrast.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n    \n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eImaging-Ready Mechanics: 9-Point Cell and 2-inch Geared Focuser\u003c\/h3\u003e\n      \u003cp\u003eThe mechanical systems of the CT10L are engineered to support the optical performance. The primary mirror rests on a 9-point flotation cell, CNC machined from aluminum to prevent any print-through or astigmatism from mechanical stress. An integrated fan provides active cooling to help the mirror reach thermal equilibrium quickly.\u003c\/p\u003e\n      \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003e2-inch Geared Focuser:\u003c\/strong\u003e A precision-machined 2-inch focuser with reduction gearing allows for smooth, fine adjustments critical for achieving sharp focus at high magnification.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eCNC Tube Rings:\u003c\/strong\u003e A pair of solid, black-anodised CNC machined rings weighing 1.5kg provide a secure and stable mounting platform for the 12.5kg tube.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eAdjustable Spider:\u003c\/strong\u003e The stainless steel 4-vane spider is fully adjustable, allowing for precise secondary mirror collimation to maintain optical alignment.\u003c\/li\u003e\n      \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eThe 1\/10 PV Difference: Visualizing Research-Grade Optics\u003c\/h3\u003e\n      \u003cp\u003eWhile a standard 1\/4 PV wavefront optic produces good images, the 1\/10 PV wavefront correction of the CT10L elevates views from good to exceptional. This level of accuracy concentrates more light into the central Airy disk of a star, resulting in visibly higher contrast on planetary details, tighter star points, and the ability to resolve fainter, closer double stars. Under steady seeing conditions, a 1\/10 PV optic delivers an image that is fundamentally sharper and more detailed than what a lesser mirror can physically produce.\u003c\/p\u003e\n      \u003cdiv class=\"DAV-comparison-grid\"\u003e\n        \u003cdiv class=\"DAV-comparison-item\"\u003e\n          \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Saturn-1_4-PV.jpg\" alt=\"Saturn viewed through a 1\/4 PV wavefront telescope\"\u003e\n          \u003cp\u003e1\/4 PV (Standard)\u003c\/p\u003e\n        \u003c\/div\u003e\n        \u003cdiv class=\"DAV-comparison-item\"\u003e\n          \u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Saturn-1_10-PV.jpg\" alt=\"Saturn viewed through a 1\/10 PV wavefront telescope\"\u003e\n          \u003cp\u003e1\/10 PV (CT Series)\u003c\/p\u003e\n        \u003c\/div\u003e\n      \u003c\/div\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n\u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the CT10L's 1\/10 PV wavefront accuracy mean for viewing Jupiter?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eFor an object like Jupiter, the \u003cstrong\u003e1\/10 PV wavefront\u003c\/strong\u003e accuracy of the Orion Optics CT10L translates directly to higher contrast and finer detail. You will be able to more clearly resolve subtle cloud bands, festoons, and small ovals, as well as fine detail within the Great Red Spot. The superior correction minimizes light scatter, making the planet's moons appear as sharp, distinct disks rather than fuzzy points of light during moments of excellent atmospheric seeing.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the carbon fibre tube on the CT10L benefit long-exposure astrophotography?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe primary benefit is \u003cstrong\u003efocal stability\u003c\/strong\u003e. Metal tubes expand and contract with temperature changes, causing the focal point to shift and resulting in soft or bloated stars over a long imaging session. The CT10L's carbon fibre sandwich tube has virtually zero thermal expansion, meaning your focus will remain sharp from the beginning of the night to the end without constant adjustments.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eIs the CT10L's f\/6.3 focal ratio suitable for both visual and imaging?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eYes, f\/6.3 is an excellent compromise. For visual observers, it's fast enough to provide bright, wide-field views with low-power eyepieces but slow enough to be very forgiving on eyepiece designs, delivering sharp stars across the field. For imagers, the \u003cstrong\u003e1575mm focal length\u003c\/strong\u003e provides ample image scale for galaxies, planetary nebulae, and planets without requiring extreme seeing conditions.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of mount is required for the Orion Optics CT10L?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe CT10L optical tube weighs \u003cstrong\u003e12.5kg\u003c\/strong\u003e and the rings add another \u003cstrong\u003e1.5kg\u003c\/strong\u003e, for a total of 14kg. For visual use, a mount with a payload capacity of at least 18kg (40 lbs) is recommended. For serious astrophotography, a mount in the 22kg (50 lbs) payload class or higher is essential to handle the tube's 1440mm length and provide the necessary stability for sharp, long exposures.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWith its 250mm aperture, can the CT10L resolve globular clusters like the Hercules Cluster (M13)?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eAbsolutely. A \u003cstrong\u003e250mm\u003c\/strong\u003e aperture has significant light-gathering and resolving power. On a target like M13, the CT10L will resolve the dense core into a field of thousands of individual pin-point stars. The 1\/10 PV optics ensure these stars are as sharp as the seeing will permit, creating a stunning, three-dimensional visual experience.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is a Zygo report included with the CT10L?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe Zygo interferometer report is your \u003cstrong\u003ecertificate of optical quality\u003c\/strong\u003e. It is a printout from a high-precision laser measurement device that shows the exact surface accuracy of your specific primary mirror. Including this report demonstrates that the advertised 1\/10 PV wavefront specification is not just a marketing claim but a measured, verifiable fact for the instrument you receive.\u003c\/p\u003e\n  \u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003ctable class=\"DAV-specifications\"\u003e\n    \u003ctbody\u003e\n      \u003ctr\u003e\n\u003ctd\u003eOptics Grade\u003c\/td\u003e\n\u003ctd\u003e1\/10 PV Wavefront Standard\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eAperture\u003c\/td\u003e\n\u003ctd\u003e250mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocal Length\u003c\/td\u003e\n\u003ctd\u003e1575mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd\u003ef\/6.3\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003ePrimary Mirror Glass\u003c\/td\u003e\n\u003ctd\u003eSuprax\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eCoatings\u003c\/td\u003e\n\u003ctd\u003eEnhanced Hilux\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSecondary Mirror Size\u003c\/td\u003e\n\u003ctd\u003e50mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Material\u003c\/td\u003e\n\u003ctd\u003eCarbon Fibre Sandwich\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Diameter\u003c\/td\u003e\n\u003ctd\u003e300mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Length\u003c\/td\u003e\n\u003ctd\u003e1440mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Weight\u003c\/td\u003e\n\u003ctd\u003e12.5kg\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocuser\u003c\/td\u003e\n\u003ctd\u003e2\" with reduction gearing\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMirror Cell\u003c\/td\u003e\n\u003ctd\u003e9-point suspension, CNC machined aluminum\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSpider\u003c\/td\u003e\n\u003ctd\u003e4-vane, stainless steel, fully adjustable\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFinder Scope\u003c\/td\u003e\n\u003ctd\u003e8x50\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMounting Rings\u003c\/td\u003e\n\u003ctd\u003eCNC machined, anodised black\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eRings Weight\u003c\/td\u003e\n\u003ctd\u003e1.5kg\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eExtension Tubes\u003c\/td\u003e\n\u003ctd\u003e40mm, screw threaded\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBoxed Dimensions\u003c\/td\u003e\n\u003ctd\u003e172 x 48 x 48 cm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBoxed Weight\u003c\/td\u003e\n\u003ctd\u003e20kg\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003c\/tbody\u003e\n  \u003c\/table\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cul class=\"DAV-grid\"\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003eCT10L Optical Tube Assembly\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003e8x50 Finder Scope\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003eCNC Machined Tube Rings\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1 Pair\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003e40mm Extension Tube\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n    \u003cli class=\"DAV-grid-item\"\u003e\n      \u003cdiv\u003e\n        \u003cp class=\"DAV-item-title\"\u003eZygo Interferometry Test Report\u003c\/p\u003e\n        \u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n      \u003c\/div\u003e\n    \u003c\/li\u003e\n  \u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/orion-optics-uk-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eOrion Optics UK 1-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Orion Optics UK","offers":[{"title":"Default Title","offer_id":52942379614493,"sku":"OOUK-CT10L-OPTICAL-TUBE-ASSEMBLY","price":6324.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Logo_ad896c08-c553-4fdd-8058-8eccf68d8f26.jpg?v=1789607197"},{"product_id":"orion-optics-uk-ct12-optical-tube-assembly","title":"Orion Optics UK CT12 Optical Tube Assembly","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e300mm (12\") Aperture f\/4 Newtonian Reflector\u003c\/li\u003e\n\u003cli\u003e1200mm Focal Length\u003c\/li\u003e\n\u003cli\u003eCertified 1\/10 PV Wavefront Primary Mirror\u003c\/li\u003e\n\u003cli\u003eCarbon Fiber Sandwich Tube Construction\u003c\/li\u003e\n\u003cli\u003e9-Point CNC-Machined Flotation Mirror Cell\u003c\/li\u003e\n\u003cli\u003e2\" Dual-Speed Focuser\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eOrion Optics UK CT12 Optical Tube Assembly\u003c\/h2\u003e\n\u003cp\u003eThe Orion Optics UK CT12 combines a fast f\/4 optical system with a massive 300mm aperture, built around a primary mirror hand-figured to a 1\/10 PV wavefront accuracy. Housed in a thermally stable carbon fiber sandwich tube measuring 1100mm long, this OTA is engineered for high-resolution planetary and deep-sky imaging where optical perfection is paramount. The 17kg assembly is supported by a 9-point flotation cell and CNC-machined rings, delivering a rigid and precise platform for capturing the finest details the night sky has to offer.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUltra-Grade 1\/10 PV Wavefront Optics: The CT12's Defining Feature\u003c\/h3\u003e\n\u003cp\u003eThe heart of the CT12 is its 300mm Suprax primary mirror, which comes standard with Orion Optics UK's highest possible optical grade: 1\/10 Peak-to-Valley (PV) wavefront. This isn't an optional upgrade; it's the baseline for the CT series. This level of precision, verified by an included Zygo laser interferometer report, ensures that the telescope delivers the sharpest, highest-contrast images physically possible, limited only by atmospheric seeing.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003e1\/10 PV Wavefront Standard:\u003c\/strong\u003e Represents the pinnacle of mirror figuring, minimizing scattered light and maximizing fine detail on challenging targets like planetary cloud bands and tight double stars.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eEnhanced Hilux Coatings:\u003c\/strong\u003e Provide superior reflectivity for brighter images and increased contrast, crucial for pulling faint deep-sky objects out of the background sky.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eZygo Test Report Included:\u003c\/strong\u003e Every CT12 ships with its own interferometry data, providing absolute proof of the primary mirror's exceptional quality and giving you full confidence in your instrument's capabilities.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eVisualizing the 1\/10 PV Advantage on High-Resolution Targets\u003c\/h3\u003e\n\u003cp\u003eA 1\/10 PV wavefront isn't just a number—it translates directly to superior performance at the eyepiece and sensor. Compared to standard 1\/4 PV or even upgraded 1\/6 PV optics, the near-perfect surface of the CT12's mirror concentrates more light into the central Airy disk of a star's image. This results in visibly higher contrast on low-contrast planetary features, like the subtle banding on Saturn or the Cassini Division in its rings, especially during moments of steady seeing.\u003c\/p\u003e\n\u003cdiv class=\"DAV-image-grid\"\u003e\n  \u003cdiv class=\"DAV-image-grid-item\"\u003e\n\u003cimg alt=\"Saturn view through 1\/4 PV optics\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Saturn-1_4-PV.jpg\"\u003e\n  \u003cp\u003e1\/4 PV (Standard)\u003c\/p\u003e\n\u003c\/div\u003e\n  \u003cdiv class=\"DAV-image-grid-item\"\u003e\n\u003cimg alt=\"Saturn view through 1\/6 PV optics\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Saturn-1_6-PV.jpg\"\u003e\n  \u003cp\u003e1\/6 PV (Professional)\u003c\/p\u003e\n\u003c\/div\u003e\n  \u003cdiv class=\"DAV-image-grid-item\"\u003e\n\u003cimg alt=\"Saturn view through 1\/8 PV optics\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Saturn-1_8-PV.jpg\"\u003e\n  \u003cp\u003e1\/8 PV (Research)\u003c\/p\u003e\n\u003c\/div\u003e\n  \u003cdiv class=\"DAV-image-grid-item\"\u003e\n\u003cimg alt=\"Saturn view through 1\/10 PV optics\" src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Saturn-1_10-PV.jpg\"\u003e\n  \u003cp\u003e1\/10 PV (Ultra)\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eCarbon Fiber Tube \u0026amp; 9-Point Cell: Stability for f\/4 Imaging\u003c\/h3\u003e\n\u003cp\u003eAt a fast f\/4 focal ratio, maintaining precise focus is critical. The CT12's carbon fiber sandwich tube, with a 350mm diameter, offers near-zero thermal expansion. This ensures the 1200mm focal length remains constant as temperatures drop overnight, eliminating the need for constant refocusing during an imaging session. The 300mm primary mirror is supported by a CNC-machined 9-point flotation cell, which prevents gravitational distortion and includes a fan for rapid thermal stabilization.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eZero-Expansion Tube:\u003c\/strong\u003e The carbon fiber construction maintains focus stability, a non-negotiable requirement for serious astrophotography with a fast optical system.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e9-Point Flotation Cell:\u003c\/strong\u003e Distributes the mirror's weight evenly to preserve its precise 1\/10 PV figure, regardless of the telescope's orientation.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eActive Cooling:\u003c\/strong\u003e An integrated fan accelerates the cooling of the primary mirror to match ambient temperature, reducing tube currents and sharpening the image faster.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePrecision 2\" Focuser and 8x50 Finder: Critical Imaging Components\u003c\/h3\u003e\n\u003cp\u003eThe CT12 is equipped with components that match the quality of its optics. The 2\" focuser features reduction gearing for fine focus adjustments, essential for achieving sharp stars with a modern imaging sensor. For visual target acquisition, a high-quality 8x50 finder scope is included, providing a bright, wide field of view to easily locate objects before switching to the main eyepiece or camera.\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003e\n\u003cstrong\u003eDual-Speed Focuser:\u003c\/strong\u003e Allows for rapid coarse focusing and then extremely fine adjustments, critical for locking in perfect focus with the narrow focal zone of an f\/4 system.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003e8x50 Finder:\u003c\/strong\u003e A substantial finder that gathers enough light to show many deep-sky objects directly, making star-hopping intuitive and fast.\u003c\/li\u003e\n\u003cli\u003e\n\u003cstrong\u003eIncluded 40mm Extension Tube:\u003c\/strong\u003e Ensures that a wide range of eyepieces and cameras can reach focus without requiring additional accessories.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is the CT12's 1\/10 PV wavefront specification so important for planetary imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eFor planetary imaging, contrast is everything. A \u003cstrong\u003e1\/10 PV wavefront\u003c\/strong\u003e mirror minimizes light scatter, which directly increases the contrast of fine, low-contrast details like Jupiter's cloud belts, the Great Red Spot, or subtle features on Mars. This higher precision allows you to push magnification further during moments of good seeing and resolve details that would be smeared out by optics with a lower PV rating.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the CT12's f\/4 focal ratio affect imaging of deep-sky objects like the Orion Nebula (M42)?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe fast \u003cstrong\u003ef\/4 focal ratio\u003c\/strong\u003e allows the CT12 to capture photons at a much faster rate than an f\/8 or f\/10 system. When imaging a large, bright target like the Orion Nebula (M42), this means you can collect the same amount of data in significantly shorter sub-exposures. This reduces demands on your mount's tracking accuracy and allows you to build up a deep, high-signal image more efficiently.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of mount is required for the 17kg CT12 OTA?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWith an approximate tube weight of \u003cstrong\u003e17kg\u003c\/strong\u003e (plus 2kg for rings and additional weight for a camera and guide scope), the CT12 requires a substantial equatorial mount with a high payload capacity. For imaging, you should look for a mount rated for at least 25-30kg to ensure stability and precise tracking. Mounts in the EQ6-R Pro, CGX, or higher class are recommended.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the carbon fiber tube on the CT12 really prevent focus shift during temperature changes?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. Carbon fiber has an extremely low coefficient of thermal expansion, especially compared to aluminum or steel tubes. This means that as the ambient temperature drops throughout the night, the \u003cstrong\u003e1100mm tube\u003c\/strong\u003e will not shrink, keeping the distance between the primary mirror and the focuser constant. This maintains a stable focal plane, which is critical for long imaging sessions at f\/4 where the depth of focus is very shallow.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat do I need to add to the CT12 to start observing or imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe CT12 is an Optical Tube Assembly (OTA) and requires several key components to be operational. You will need:\u003c\/p\u003e\n\u003cul\u003e\n\u003cli\u003eA suitable equatorial mount (see above).\u003c\/li\u003e\n\u003cli\u003eAt least one 2\" or 1.25\" eyepiece for visual observation (none are included).\u003c\/li\u003e\n\u003cli\u003eA collimation tool (essential for a fast Newtonian).\u003c\/li\u003e\n\u003cli\u003eA 12V power supply for the mirror's cooling fan.\u003c\/li\u003e\n\u003cli\u003eAn astronomy camera and any necessary adapters if you plan to do astrophotography.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the CT12 for high-magnification views of Jupiter in my light-polluted backyard?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAbsolutely. The CT12's large \u003cstrong\u003e300mm aperture\u003c\/strong\u003e provides incredible light-gathering power and high potential resolution. Light pollution primarily affects faint deep-sky objects, but bright targets like Jupiter are largely immune. The limiting factor for planetary viewing is atmospheric seeing, not light pollution. On a night with steady air, the 1\/10 PV optics will deliver exceptionally sharp and detailed views of Jupiter's atmospheric bands and its Galilean moons.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Quality\u003c\/td\u003e\n\u003ctd\u003e1\/10 PV wavefront (Standard)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAperture\u003c\/td\u003e\n\u003ctd\u003e300mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocal Length\u003c\/td\u003e\n\u003ctd\u003e1200mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd\u003ef\/4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePrimary Mirror Glass\u003c\/td\u003e\n\u003ctd\u003eSuprax\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMirror Coatings\u003c\/td\u003e\n\u003ctd\u003eEnhanced Hilux\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSecondary Mirror Size\u003c\/td\u003e\n\u003ctd\u003e75mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocuser\u003c\/td\u003e\n\u003ctd\u003e2\" with reduction gearing\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFinder Scope\u003c\/td\u003e\n\u003ctd\u003e8x50\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Material\u003c\/td\u003e\n\u003ctd\u003eCarbon fibre sandwich\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Diameter\u003c\/td\u003e\n\u003ctd\u003e350mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Length\u003c\/td\u003e\n\u003ctd\u003e1100mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Weight\u003c\/td\u003e\n\u003ctd\u003e17kg (approx)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMirror Cell\u003c\/td\u003e\n\u003ctd\u003e9-point suspension, CNC machined aluminum\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSpider\u003c\/td\u003e\n\u003ctd\u003e4-vane stainless steel, fully adjustable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSecondary Holder\u003c\/td\u003e\n\u003ctd\u003eCNC machined aluminum, rotatable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMounting Rings\u003c\/td\u003e\n\u003ctd\u003eCNC machined, anodised black\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRings Weight\u003c\/td\u003e\n\u003ctd\u003e2kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExtension Tube\u003c\/td\u003e\n\u003ctd\u003e40mm, screw threaded\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBoxed Dimensions\u003c\/td\u003e\n\u003ctd\u003eBox 1: 128x52x52mm, Box 2: 58x58x34mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBoxed Weight\u003c\/td\u003e\n\u003ctd\u003eBox 1: 14kg, Box 2: 12kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eCT12 f\/4 Optical Tube Assembly\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eCNC Machined Tube Rings\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 2\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e8x50 Finder Scope\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eZygo Interferometry Test Report\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/orion-optics-uk-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eOrion Optics UK 1-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Orion Optics UK","offers":[{"title":"Default Title","offer_id":52942380237085,"sku":"OOUK-CT12-OPTICAL-TUBE-ASSEMBLY","price":5702.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Logo_96e87270-bbce-4f23-845d-a9a4f25223af.jpg?v=1789607205"},{"product_id":"orion-optics-uk-ct12l-optical-tube-assembly","title":"Orion Optics UK CT12L Optical Tube Assembly","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e300mm (12\") Aperture\u003c\/li\u003e\n\u003cli\u003e1590mm Focal Length, f\/5.3 Focal Ratio\u003c\/li\u003e\n\u003cli\u003eStandard 1\/10 PV Wavefront Optics\u003c\/li\u003e\n\u003cli\u003eCarbon Fibre Sandwich Tube Construction\u003c\/li\u003e\n\u003cli\u003e2\" Focuser with Reduction Gearing\u003c\/li\u003e\n\u003cli\u003e9-Point CNC Machined Mirror Cell\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eOrion Optics UK CT12L Optical Tube Assembly\u003c\/h2\u003e\n\u003cp\u003eThe Orion Optics UK CT12L is an imaging-first Newtonian built around a 300mm primary mirror hand-figured to a 1\/10 PV wavefront standard. Its 1590mm focal length delivers an f\/5.3 ratio, ideal for resolving fine detail on planets and capturing faint structures in deep-sky objects. The entire optical system is housed in a 1450mm carbon fibre sandwich tube weighing approximately 20kg, ensuring thermal stability and maintaining a precise focal plane through long imaging sessions.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eUltra-Grade 1\/10 PV Optics: The Foundation of the 300mm System\u003c\/h3\u003e\n\u003cp\u003eThe heart of the CT12L is its 300mm Suprax primary mirror, which comes standard with Orion Optics UK's highest optical certification: a 1\/10 PV wavefront accuracy. This is not an optional upgrade but the baseline for the CT series, ensuring the highest possible contrast and sharpness. The mirror features Enhanced Hilux coatings for maximum reflectivity, and its performance is documented by an included Zygo interferometry report, providing empirical proof of its quality.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eCarbon Fibre Tube: 1450mm of Thermally Stable Engineering\u003c\/h3\u003e\n\u003cp\u003eTo maintain the performance of its elite optics, the CT12L employs a carbon fibre sandwich tube. This advanced material has a near-zero coefficient of thermal expansion, preventing the 1590mm focal length from shifting as ambient temperature changes. The 350mm diameter tube is finished with a gloss exterior and a matte black interior to suppress stray light, providing a high-contrast backdrop for both visual observation and astrophotography.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003ePrecision Mechanics: A 9-Point Cell and 2-inch Geared Focuser\u003c\/h3\u003e\n\u003cp\u003eThe CT12L's optical performance is supported by a robust mechanical framework. The primary mirror rests on a CNC machined 9-point flotation cell that prevents flexure and is aided by a fan for rapid thermal equalization. Up front, the 63mm secondary mirror is held by a fully adjustable, stainless steel 4-vane spider, while the 2-inch focuser with reduction gearing allows for the precise, repeatable focus adjustments necessary at an f\/5.3 focal ratio.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe 1\/10 PV Difference: Visualizing Optical Accuracy\u003c\/h3\u003e\n\u003cp\u003eOrion Optics UK offers several grades of optical accuracy, but the CT12L includes their finest 1\/10 PV grade as standard. Compared to a common 1\/4 PV \"diffraction-limited\" mirror, a 1\/10 PV surface delivers a wavefront that is significantly closer to a perfect parabola. In practice, this translates to visibly higher contrast on planetary details like Jupiter's cloud bands, tighter star points, and the ability to resolve fainter, more subtle nebulosity that would be lost in the noise of a less accurate system.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the 1\/10 PV wavefront rating on the CT12L mean for observing?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe \u003cstrong\u003e1\/10 Peak-to-Valley (PV) wavefront\u003c\/strong\u003e rating means the surface of the 300mm primary mirror deviates from a perfect parabola by no more than 1\/10th of a wavelength of light. This is an extremely high standard of accuracy that results in superior image contrast and sharpness. For you, the observer, this means seeing finer details on planets, resolving tighter double stars, and capturing more delicate structures in nebulae.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the CT12L's carbon fiber tube benefit astrophotography?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe carbon fiber tube has a near-zero thermal expansion coefficient. During a long imaging session, as temperatures drop overnight, a metal tube will contract and slightly change the focal length, causing images to lose focus. The \u003cstrong\u003eCT12L's 1450mm carbon fiber tube\u003c\/strong\u003e remains dimensionally stable, keeping the focal plane locked and ensuring your images remain sharp from the beginning of the night to the end without constant refocusing.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the CT12L's 20kg weight manageable for a portable setup?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eAt approximately \u003cstrong\u003e20kg for the tube and 2kg for the rings\u003c\/strong\u003e, the CT12L is a substantial instrument. While it can be transported to a dark sky site, it is not a grab-and-go telescope. It requires a robust equatorial mount and is best suited for a semi-permanent or observatory setup where its weight can be managed safely.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of mount is required for the Orion Optics CT12L OTA?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eWith a combined weight of over 22kg (48.5 lbs) for the OTA and rings, plus the added weight of a camera, guide scope, and other accessories, you will need a heavy-duty equatorial mount. A mount with a rated payload capacity of at least 60-70 lbs is recommended to ensure stability for long-exposure astrophotography with the CT12L's 1590mm focal length.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow will the CT12L's f\/5.3 optics perform on faint galaxies like the Leo Triplet?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe CT12L's combination of a large \u003cstrong\u003e300mm aperture\u003c\/strong\u003e and a fast \u003cstrong\u003ef\/5.3 focal ratio\u003c\/strong\u003e is excellent for galaxy clusters. The large aperture gathers significant light to reveal faint extensions and dust lanes in galaxies like M65 and M66, while the 1\/10 PV optics ensure that the faint signal is rendered with maximum contrast against the sky background, making subtle details more visible.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat level of detail can I expect on Saturn with the CT12L's 300mm, 1\/10 PV mirror?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eUnder steady seeing conditions, the \u003cstrong\u003e300mm aperture and 1\/10 PV optics\u003c\/strong\u003e of the CT12L will provide exceptional planetary views. On Saturn, you can expect to clearly resolve the Cassini Division, subtle cloud banding on the planet's disk, and potentially the Encke Gap with excellent seeing. The high-contrast optics will also make it easier to pick out Saturn's fainter moons against the glare of the rings.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptics Grade\u003c\/td\u003e\n\u003ctd\u003e1\/10 PV wavefront\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAperture\u003c\/td\u003e\n\u003ctd\u003e300mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocal Length\u003c\/td\u003e\n\u003ctd\u003e1590mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd\u003ef\/5.3\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePrimary Mirror\u003c\/td\u003e\n\u003ctd\u003eSuprax with Enhanced Hilux Coatings\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSecondary Mirror Size\u003c\/td\u003e\n\u003ctd\u003e63mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocuser\u003c\/td\u003e\n\u003ctd\u003e2\" with reduction gearing\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFinder Scope\u003c\/td\u003e\n\u003ctd\u003e8x50\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Material\u003c\/td\u003e\n\u003ctd\u003eCarbon fibre sandwich\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Diameter\u003c\/td\u003e\n\u003ctd\u003e350mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Length\u003c\/td\u003e\n\u003ctd\u003e1450mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Weight\u003c\/td\u003e\n\u003ctd\u003e20kg (approx)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMirror Cell\u003c\/td\u003e\n\u003ctd\u003e9-point suspension, CNC machined aluminum\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSpider\u003c\/td\u003e\n\u003ctd\u003e4-vane, stainless steel, fully adjustable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSecondary Holder\u003c\/td\u003e\n\u003ctd\u003eMachined aluminum, rotatable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRings\u003c\/td\u003e\n\u003ctd\u003eCNC machined tube rings, anodised black\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eRings Weight\u003c\/td\u003e\n\u003ctd\u003e2kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eExtension Tubes\u003c\/td\u003e\n\u003ctd\u003e40mm long, screw threaded\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBoxed Dimensions\u003c\/td\u003e\n\u003ctd\u003eBox 1: 172x58x58mm, Box 2: 58x58x34mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBoxed Weight\u003c\/td\u003e\n\u003ctd\u003eBox 1: 18.5kg, Box 2: 12kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eCT12L Optical Tube Assembly\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e8x50 Finder Scope\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eCNC Machined Tube Rings\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1 Pair\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003e40mm Extension Tube\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli class=\"DAV-grid-item\"\u003e\n\u003cdiv\u003e\n\u003cp class=\"DAV-item-title\"\u003eZygo Interferometry Test Report\u003c\/p\u003e\n\u003cp class=\"DAV-item-subtitle\"\u003e× 1\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/orion-optics-uk-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eOrion Optics UK 1-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Orion Optics UK","offers":[{"title":"Default Title","offer_id":52942380335389,"sku":"OOUK-CT12L-OPTICAL-TUBE-ASSEMBLY","price":6427.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Logo_e05da382-d3e9-442f-8edc-fcc9182420bb.jpg?v=1789607213"},{"product_id":"orion-optics-uk-ct14-optical-tube-assembly","title":"Orion Optics UK CT14 Optical Tube Assembly","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e350mm (14\") Aperture\u003c\/li\u003e\n\u003cli\u003e1600mm Focal Length (f\/4.6)\u003c\/li\u003e\n\u003cli\u003eGuaranteed 1\/10 PV Wavefront Optics\u003c\/li\u003e\n\u003cli\u003eCarbon Fibre Sandwich Tube Construction\u003c\/li\u003e\n\u003cli\u003e26kg Optical Tube Weight\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section-center\"\u003e\n      \u003ch2\u003eOrion Optics UK CT14 Optical Tube Assembly\u003c\/h2\u003e\n      \u003cp\u003eThe Orion Optics UK CT14 Optical Tube Assembly combines a massive 350mm aperture with a fast 1600mm (f\/4.6) focal length, all built around a primary mirror hand-figured to a guaranteed 1\/10 PV wavefront accuracy. This instrument is engineered for ultimate imaging stability, featuring a zero-expansion carbon fibre sandwich tube that maintains focus through changing temperatures. Weighing approximately 26kg, the CT14 delivers research-grade optical performance for serious planetary and deep-sky astrophotographers.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003e1\/10 PV Wavefront Optics: The CT14's Hand-Figured 350mm Primary\u003c\/h3\u003e\n      \u003cp\u003eThe heart of the CT14 is its 350mm Suprax primary mirror, which is not just machine-polished but hand-finished to an exceptional 1\/10 PV wavefront standard. This figure represents the peak-to-valley error across the optical surface, and 1\/10th wave is the highest grade Orion Optics UK produces. This level of precision, verified by an included Zygo interferometer report, ensures that the maximum amount of light is concentrated into the smallest possible point, yielding incredibly sharp, high-contrast images of planets and tight stellar fields.\u003c\/p\u003e\n        \u003cul\u003e\n            \u003cli\u003e\n\u003cstrong\u003eEnhanced Hilux Coatings:\u003c\/strong\u003e The primary and secondary mirrors feature high-reflectivity Hilux coatings to maximize light transmission for brighter views of faint deep-sky objects.\u003c\/li\u003e\n            \u003cli\u003e\n\u003cstrong\u003e82mm Secondary Mirror:\u003c\/strong\u003e The optimized secondary mirror provides excellent field illumination for large-sensor cameras without excessive obstruction.\u003c\/li\u003e\n        \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n    \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eZero-Expansion Carbon Fibre Tube and 9-Point Mirror Cell\u003c\/h3\u003e\n      \u003cp\u003eOptical precision requires mechanical stability. The CT14's 400mm diameter tube is a sandwich-construction carbon fibre design with virtually zero thermal expansion, ensuring the 1600mm focal length remains constant as temperatures drop. The primary mirror is supported by a CNC machined, 9-point flotation cell that prevents flexure and astigmatism as the 26kg tube moves across the sky.\u003c\/p\u003e\n      \u003cul\u003e\n        \u003cli\u003e\n\u003cstrong\u003eActive Cooling:\u003c\/strong\u003e The mirror cell includes an integrated fan system that can be run continuously to speed up thermal equalization, minimizing tube currents and ensuring the optics perform at their peak from the start of your session.\u003c\/li\u003e\n        \u003cli\u003e\n\u003cstrong\u003eCNC Tube Rings:\u003c\/strong\u003e A pair of heavy-duty, CNC-machined tube rings weighing 3kg provides a rigid and secure mounting platform for this large-aperture instrument.\u003c\/li\u003e\n      \u003c\/ul\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003ePrecision 2\" Focuser and 8x50 Finder\u003c\/h3\u003e\n      \u003cp\u003eThe CT14 is equipped with a high-quality 2\" rack and pinion focuser with reduction gearing for fine focus control, critical for achieving sharp results at f\/4.6. A 40mm threaded extension tube is included for reaching focus with a variety of cameras and eyepieces. For locating targets, a straight-through 8x50 achromatic finder scope is fitted to the tube, providing bright, wide-field views to complement the main telescope's narrow, high-magnification field.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n  \u003cdiv class=\"DAV-bg-light\"\u003e\n    \u003cdiv class=\"DAV-section\"\u003e\n      \u003ch3\u003eBeyond Diffraction-Limited: Why the CT14's 1\/10 PV Standard Matters\u003c\/h3\u003e\n      \u003cp\u003eMany telescopes are advertised as \"diffraction-limited,\" which corresponds to a 1\/4 PV wavefront accuracy. The CT14's 1\/10 PV standard is significantly more precise, a difference that becomes obvious when observing planets at high magnification. The improved surface accuracy reduces scattered light and sharpens fine details, rendering more subtle cloud bands on Jupiter and cleaner divisions in Saturn's rings. For the CT14, this research-grade figure isn't an expensive upgrade—it's the baseline.\u003c\/p\u003e\n    \u003c\/div\u003e\n  \u003c\/div\u003e\n\n\u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat does the Orion Optics UK CT14's 1\/10 PV wavefront accuracy mean for imaging Jupiter?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eFor a target like Jupiter, the CT14's \u003cstrong\u003e1\/10 PV wavefront optics\u003c\/strong\u003e minimize light scatter, which directly translates to higher contrast. You will resolve finer, more delicate details in the cloud bands, see more intricate structure within the Great Red Spot, and achieve a sharper overall image compared to a standard 1\/4 PV (\"diffraction-limited\") mirror of the same 350mm aperture.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of mount is required for the CT14 Optical Tube?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe CT14 optical tube weighs approximately \u003cstrong\u003e26kg\u003c\/strong\u003e, and the rings add another \u003cstrong\u003e3kg\u003c\/strong\u003e, for a total of 29kg before adding a camera, guide scope, or other accessories. You will need a high-capacity German equatorial mount with a payload rating of at least 45kg (100 lbs) for stable imaging performance.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the f\/4.6 focal ratio of the CT14 require a coma corrector for astrophotography?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eYes. Like all fast Newtonian telescopes, the CT14 will exhibit coma at the edges of the field, especially with larger camera sensors. To achieve sharp, point-like stars across the entire frame, using a high-quality coma corrector designed for f\/4.6 systems is essential for astrophotography.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the CT14's carbon fibre tube benefit long-exposure imaging?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eThe \u003cstrong\u003ecarbon fibre sandwich\u003c\/strong\u003e construction has a near-zero coefficient of thermal expansion. This means as the ambient temperature drops during an imaging session, the \u003cstrong\u003e1430mm\u003c\/strong\u003e tube will not shrink. This keeps the focal plane stable, preventing focus shift and ensuring your images remain sharp throughout the night without constant refocusing.\u003c\/p\u003e\n  \u003c\/div\u003e\n    \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the advantage of the CT14's 9-point mirror cell?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eA large \u003cstrong\u003e350mm\u003c\/strong\u003e primary mirror is heavy and can deform under its own weight if not properly supported. The \u003cstrong\u003e9-point suspension mirror cell\u003c\/strong\u003e distributes the weight of the mirror evenly across nine optimized points. This prevents gravitational sagging and flexure as the telescope points to different parts of the sky, preserving the mirror's precise 1\/10 PV figure and preventing optical aberrations like astigmatism.\u003c\/p\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion\"\u003e\n    \u003ch3 class=\"DAV-accordion-Q\"\u003eCan I use the Orion Optics UK CT14 for visual observation of the Veil Nebula (NGC 6960)?\u003c\/h3\u003e\n  \u003c\/div\u003e\n  \u003cdiv class=\"DAV-accordion-A\"\u003e\n    \u003cp\u003eAbsolutely. The CT14's large \u003cstrong\u003e350mm\u003c\/strong\u003e aperture is exceptional for visual deep-sky observing. When paired with a wide-field 2\" eyepiece and a quality O-III filter, the Veil Nebula will show stunning, intricate filamentary detail. The fast \u003cstrong\u003ef\/4.6\u003c\/strong\u003e focal ratio provides a bright image, making it a powerful instrument for hunting down faint nebulae and galaxies.\u003c\/p\u003e\n  \u003c\/div\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003ctable class=\"DAV-specifications\"\u003e\n    \u003ctbody\u003e\n      \u003ctr\u003e\n\u003ctd\u003eAperture\u003c\/td\u003e\n\u003ctd\u003e350mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocal Length\u003c\/td\u003e\n\u003ctd\u003e1600mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd\u003ef\/4.6\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eStandard Optics Grade\u003c\/td\u003e\n\u003ctd\u003e1\/10 PV wavefront\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003ePrimary Mirror Glass\u003c\/td\u003e\n\u003ctd\u003eSuprax\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMirror Coatings\u003c\/td\u003e\n\u003ctd\u003eEnhanced Hilux\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSecondary Mirror Size\u003c\/td\u003e\n\u003ctd\u003e82mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Material\u003c\/td\u003e\n\u003ctd\u003eCarbon fibre sandwich\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Diameter\u003c\/td\u003e\n\u003ctd\u003e400mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Length\u003c\/td\u003e\n\u003ctd\u003e1430mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eTube Weight\u003c\/td\u003e\n\u003ctd\u003e26kg approx.\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFocuser\u003c\/td\u003e\n\u003ctd\u003e2\" focuser with reduction gearing\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eExtension Tubes\u003c\/td\u003e\n\u003ctd\u003e40mm long, screw threaded\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eFinder Scope\u003c\/td\u003e\n\u003ctd\u003e8x50\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSpider\u003c\/td\u003e\n\u003ctd\u003eAdjustable 4-vane, stainless steel\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMirror Cell\u003c\/td\u003e\n\u003ctd\u003eCNC machined aluminium, 9 point suspension\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eSecondary Holder\u003c\/td\u003e\n\u003ctd\u003eMachined aluminium, rotatable\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eMounting Rings\u003c\/td\u003e\n\u003ctd\u003eCNC machined tube rings, anodised black\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eWeight of Rings\u003c\/td\u003e\n\u003ctd\u003e3kg\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBoxed Dimensions\u003c\/td\u003e\n\u003ctd\u003eBox 1: 172x58x58mm, Box 2: 58x58x34mm\u003c\/td\u003e\n\u003c\/tr\u003e\n      \u003ctr\u003e\n\u003ctd\u003eBoxed Weight\u003c\/td\u003e\n\u003ctd\u003eBox 1: 20kg, Box 2: 14kg\u003c\/td\u003e\n\u003c\/tr\u003e\n    \u003c\/tbody\u003e\n  \u003c\/table\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n  \u003cul class=\"DAV-grid\"\u003e\n  \u003c\/ul\u003e\n\u003c\/li\u003e\n\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/orion-optics-uk-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eOrion Optics UK 1-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Orion Optics UK","offers":[{"title":"Default Title","offer_id":52942380433693,"sku":"OOUK-CT14-OPTICAL-TUBE-ASSEMBLY","price":9373.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Logo_b64200b7-8fb9-4862-8722-a8cb7101fa00.jpg?v=1789607222"},{"product_id":"orion-optics-uk-ct16-optical-tube-assembly","title":"Orion Optics UK CT16 Optical Tube Assembly","description":"\u003cul class=\"DAV-feature-list\"\u003e\n\u003cli\u003e400mm (16\") Aperture\u003c\/li\u003e\n\u003cli\u003e1600mm Focal Length (f\/4)\u003c\/li\u003e\n\u003cli\u003e1\/10 PV Wavefront Standard Optics\u003c\/li\u003e\n\u003cli\u003eCarbon Fiber Sandwich Tube Construction\u003c\/li\u003e\n\u003cli\u003e36kg Optical Tube Weight\u003c\/li\u003e\n\u003cli\u003e9-Point CNC Machined Mirror Cell\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c!-- more --\u003e\n\u003cul class=\"tabs\"\u003e\n\u003cli class=\"active\"\u003eDescription\u003c\/li\u003e\n\u003cli\u003eFAQ\u003c\/li\u003e\n\u003cli\u003eSpecifications\u003c\/li\u003e\n\u003cli\u003eIn the Box\u003c\/li\u003e\n\u003cli\u003eWarranty\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003cul class=\"tabs-content\"\u003e\n\u003cli class=\"active\"\u003e\n\u003cdiv\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section-center\"\u003e\n\u003ch2\u003eOrion Optics UK CT16 Optical Tube Assembly\u003c\/h2\u003e\n\u003cp\u003eThe Orion Optics UK CT16 is an observatory-class imaging instrument built around a hand-figured, 400mm f\/4 primary mirror guaranteed to a 1\/10 PV wavefront accuracy. Paired with a thermally inert carbon fiber sandwich tube and a 9-point flotation cell, its 1600mm focal length is engineered to deliver maximum resolution and contrast on the most demanding deep-sky and planetary targets. Weighing approximately 36kg, the CT16 OTA combines massive light-gathering power with the optical precision required for serious astrophotography.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e1\/10 PV Wavefront Optics: The Foundation of CT16's Imaging Power\u003c\/h3\u003e\n\u003cp\u003eThe heart of the CT16 is its Suprax primary mirror, finished to Orion Optics UK's highest \"Ultra\" grade of 1\/10 PV wavefront. This isn't an optional upgrade; it's the standard for the entire CT line, ensuring that the optical system delivers virtually perfect images. Each mirror's performance is verified by a Zygo laser interferometer, and a report is supplied with the telescope, providing absolute confidence in its quality.\u003c\/p\u003e\n\u003cp\u003eThis level of precision means that the maximum and minimum deviation from a perfect parabolic wavefront is incredibly small. The result is exceptionally high contrast that resolves subtle details in galactic dust lanes and fine banding on gas giants, free from the image degradation caused by lower-quality optics.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eCarbon Fiber Tube \u0026amp; 9-Point Cell: Engineering for Stability\u003c\/h3\u003e\n\u003cp\u003eAt an aggressive f\/4 focal ratio, maintaining precise focus is critical. The CT16's tube is a sandwich-construction carbon fiber design with a 450mm diameter, providing extreme rigidity and near-zero thermal expansion. This ensures the 1600mm focal plane remains locked in place as temperatures change, eliminating a common source of image drift during long imaging sessions.\u003c\/p\u003e\n\u003cp\u003eThe 400mm primary mirror is supported by a CNC machined, 9-point suspension cell that prevents gravitational flexure as the telescope tracks across the sky. An integrated fan system provides active cooling, allowing the massive mirror to reach thermal equilibrium quickly for stable, sharp views from the start of your session.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003e400mm Aperture at f\/4: A Deep-Sky Imaging Powerhouse\u003c\/h3\u003e\n\u003cp\u003eWith a 400mm (16\") aperture, the CT16 gathers an immense amount of light, making it ideal for capturing faint nebulae and distant galaxies. The fast f\/4 focal ratio allows you to collect significant signal in shorter sub-exposure times, reducing demands on your mount's tracking and minimizing noise. This combination of light grasp and speed makes the CT16 a formidable tool for advanced deep-sky imaging.\u003c\/p\u003e\n\u003cp\u003eThe optical path includes a 90mm secondary mirror held by a fully adjustable, stainless steel 4-vane spider. This setup is optimized for wide-field imaging, providing even illumination across large camera sensors with the addition of an appropriate coma corrector.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eImaging-Ready Components: 2\" Focuser and 8x50 Finder\u003c\/h3\u003e\n\u003cp\u003eThe CT16 is equipped with a precision 2\" Crayford-style focuser featuring reduction gearing for fine adjustments. This allows for critical focusing accuracy, essential for extracting the maximum detail the 1\/10 PV optics can deliver. The focuser has the back-focus and load-bearing capacity to handle modern imaging trains, including filter wheels and off-axis guiders.\u003c\/p\u003e\n\u003cp\u003eFor initial alignment and target acquisition, a high-quality 8x50 achromatic finder scope is included. The entire optical tube is secured by a pair of CNC machined tube rings, which weigh 3.5kg and provide a rigid, stable connection to your mount.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-bg-light\"\u003e\n\u003cdiv class=\"DAV-section\"\u003e\n\u003ch3\u003eThe 1\/10 PV Advantage: What It Means on Jupiter and M13\u003c\/h3\u003e\n\u003cp\u003eWhile many telescopes use \"diffraction-limited\" optics (typically 1\/4 PV wavefront), the CT16's 1\/10 PV standard offers a tangible leap in image fidelity. On a target like Jupiter, a 1\/4 PV system might show the main equatorial belts clearly, but the 1\/10 PV optic will resolve finer, low-contrast details within those belts, along with delicate festoons and small ovals that would otherwise be smeared out.\u003c\/p\u003e\n\u003cp\u003eFor deep-sky objects, this translates to superior stellar resolution. When viewing the Hercules Cluster (M13), a 1\/10 PV mirror will produce tighter, more point-like stars across the field, allowing you to resolve individual stars deeper into the cluster's dense core. This is the practical benefit of minimizing wavefront error: more light is focused into the central point of a star's image, increasing sharpness and contrast on every object you view.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat kind of mount is required for the Orion Optics UK CT16 OTA?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe CT16 optical tube weighs approximately \u003cstrong\u003e36kg\u003c\/strong\u003e and the rings add another \u003cstrong\u003e3.5kg\u003c\/strong\u003e, for a total weight of nearly 40kg before adding any imaging equipment. A heavy-duty, observatory-class German Equatorial Mount with a payload capacity of at least 50kg (110 lbs) or more is strongly recommended for stable imaging.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eHow does the CT16's 1\/10 PV optics perform on planetary targets like Saturn?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe 1\/10 PV wavefront accuracy provides exceptionally high contrast, which is critical for planetary observing. On Saturn, this means you will see not just the Cassini Division, but also subtler features like the Encke Gap (in good seeing), low-contrast banding on the planet's globe, and the delicate crepe ring. The image will be sharper and more stable than what a standard 1\/4 PV optic can deliver.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eIs the f\/4 focal ratio of the CT16 good for deep-sky imaging?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes, an f\/4 focal ratio is excellent for deep-sky imaging. It is considered a \"fast\" system, allowing you to capture faint details in nebulae and galaxies with shorter exposure times compared to a slower f\/8 or f\/10 system. You will need to pair it with a high-quality coma corrector to ensure sharp stars across the entire field of view.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhat is the benefit of the carbon fiber tube on the CT16?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eThe carbon fiber sandwich tube offers two main advantages. First, it has \u003cstrong\u003evirtually zero thermal expansion\u003c\/strong\u003e, which means the focal point does not shift as the temperature changes during the night. This is crucial for maintaining sharp focus over long imaging runs. Second, it provides a very high stiffness-to-weight ratio, ensuring the optical components remain perfectly aligned.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eDoes the Orion Optics CT16 come with a Zygo test report?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eYes. Every CT-range telescope from Orion Optics UK is supplied with a Zygo interferometry report. This document provides a detailed analysis of the primary mirror's surface accuracy, giving you documented proof that it meets the stringent \u003cstrong\u003e1\/10 PV wavefront\u003c\/strong\u003e specification.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion\"\u003e\n\u003ch3 class=\"DAV-accordion-Q\"\u003eWhy is active cooling important for a 400mm mirror like the one in the CT16?\u003c\/h3\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"DAV-accordion-A\"\u003e\n\u003cp\u003eA large 400mm mirror has significant thermal mass and can take hours to cool to the ambient air temperature. While it's cooling, it creates air currents inside the optical tube (tube seeing) that degrade the image. The integrated fan system on the CT16's 9-point mirror cell actively cools the mirror, drastically reducing this cooldown time so you can achieve sharp, stable images much faster.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ctable class=\"DAV-specifications\"\u003e\n\u003ctbody\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptics Grade\u003c\/td\u003e\n\u003ctd\u003e1\/10 PV wavefront\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eAperture\u003c\/td\u003e\n\u003ctd\u003e400mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocal Length\u003c\/td\u003e\n\u003ctd\u003e1600mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocal Ratio\u003c\/td\u003e\n\u003ctd\u003ef\/4\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003ePrimary Mirror Glass\u003c\/td\u003e\n\u003ctd\u003eSuprax\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMirror Coatings\u003c\/td\u003e\n\u003ctd\u003eEnhanced Hilux\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSecondary Mirror Size\u003c\/td\u003e\n\u003ctd\u003e90mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFocuser\u003c\/td\u003e\n\u003ctd\u003e2\" focuser with reduction gearing\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eFinder Scope\u003c\/td\u003e\n\u003ctd\u003e8x50\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Material\u003c\/td\u003e\n\u003ctd\u003eCarbon fibre sandwich\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Diameter\u003c\/td\u003e\n\u003ctd\u003e450mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Length\u003c\/td\u003e\n\u003ctd\u003e1470mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eOptical Tube Weight\u003c\/td\u003e\n\u003ctd\u003e36kg (approx.)\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Rings\u003c\/td\u003e\n\u003ctd\u003eCNC machined, anodised black\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eTube Rings Weight\u003c\/td\u003e\n\u003ctd\u003e3.5kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eMirror Cell\u003c\/td\u003e\n\u003ctd\u003e9-point suspension, CNC machined aluminium\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSpider\u003c\/td\u003e\n\u003ctd\u003e4-vane, stainless steel, fully adjustable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eSecondary Holder\u003c\/td\u003e\n\u003ctd\u003eMachined aluminium, rotatable\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eIncluded Extension Tubes\u003c\/td\u003e\n\u003ctd\u003e40mm long, screw threaded\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBoxed Dimensions\u003c\/td\u003e\n\u003ctd\u003eBox 1: 172x58x58mm, Box 2: 58x58x34mm\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003ctr\u003e\n\u003ctd\u003eBoxed Weight\u003c\/td\u003e\n\u003ctd\u003eBox 1: 22kg, Box 2: 18kg\u003c\/td\u003e\n\u003c\/tr\u003e\n\u003c\/tbody\u003e\n\u003c\/table\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003cul class=\"DAV-grid\"\u003e\n\u003c\/ul\u003e\n\u003c\/li\u003e\n\u003cli\u003e\n\u003ca href=\"https:\/\/davidastro.com\/pages\/orion-optics-uk-warranty-policy\" rel=\"noopener\" target=\"_blank\"\u003eOrion Optics UK 1-Year Warranty\u003c\/a\u003e\n\u003c\/li\u003e\n\u003c\/ul\u003e","brand":"Orion Optics UK","offers":[{"title":"Default Title","offer_id":52942380794141,"sku":"OOUK-CT16-OPTICAL-TUBE-ASSEMBLY","price":10616.0,"currency_code":"CAD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0753\/5280\/1565\/files\/Orion-Optics-UK-Logo_223e6bb1-751e-40b5-ac62-068e5b4ac278.jpg?v=1789607230"}],"url":"https:\/\/davidastro.com\/collections\/orion-optics-uk-ct-carbon-newtonian-telescopes.oembed","provider":"David Astro","version":"1.0","type":"link"}