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Orion Optics UK IDEAL 8 Optical Tube Assembly

SKU OOUK-IDEAL-8
Original price CA$1,707.00 - Original price CA$1,843.00
Original price
CA$1,707.00
CA$1,707.00 - CA$1,843.00
Current price CA$1,707.00
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  • 200mm (8") Primary Mirror
  • 900mm Focal Length
  • Fast f/4.5 Focal Ratio
  • Guaranteed 1/6 PV Wavefront Standard Optics
  • CNC-Machined 9-Point Mirror Cell
  • 7kg Nominal Tube Weight
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Warranty
  • Orion Optics UK IDEAL 8 Optical Tube Assembly

    The Orion Optics UK IDEAL 8 combines a fast, 200mm f/4.5 optical system with a guaranteed 1/6 PV wavefront primary mirror for exceptional astro-imaging capability. Its 900mm focal length provides a wide field of view, while the entire aluminium tube assembly weighs a manageable 7kg. Every optic is supported by a CNC-machined 9-point suspension cell and includes a Zygo interferometer report certifying its accuracy.

    Guaranteed 1/6 PV Wavefront Optics: The Orion Optics UK Difference

    Unlike mass-produced reflectors that often cite a theoretical "diffraction limited" standard (equivalent to 1/4 PV wavefront), every IDEAL 8 OTA comes with a hand-figured primary mirror guaranteed to achieve 1/6 PV wavefront accuracy. This superior optical quality, verified by an included Zygo interferometer test report, translates directly to higher-contrast planetary views and tighter, more defined stars in deep-sky images. For the most demanding applications, optional upgrades to 1/8 PV and 1/10 PV are available.

    A 200mm f/4.5 System for Wide-Field Imaging

    With a 200mm aperture and a fast f/4.5 focal ratio, the IDEAL 8 is built for capturing large deep-sky objects. This optical speed allows you to gather significant signal in shorter exposure times, reducing demands on your mount's tracking. The 900mm focal length is ideal for framing expansive targets like the Andromeda Galaxy (M31) or the North American Nebula (NGC 7000) with modern astronomy cameras.

    • Focal Ratio (f/4.5): Reduces exposure time compared to slower f/6 or f/8 systems, capturing faint nebulosity more efficiently.
    • Aperture (200mm): Gathers ample light for resolving detail in galaxies and star clusters.
    • Coma Correction Trade-Off: Like all fast Newtonians, the IDEAL 8 will show coma at the edge of the field; pairing it with a high-quality coma corrector is essential for achieving sharp stars across the entire imaging sensor.

    Engineered for Stability: 9-Point Cell, Active Cooling, and Eris Focuser

    The optical quality is matched by a robust mechanical design. A CNC-machined 9-point suspension cell supports the primary mirror without inducing astigmatism or flexure as the telescope moves. A built-in 12-volt fan accelerates mirror cooling to ambient temperature, minimizing tube currents and ensuring sharp images sooner. The in-house designed Eris 2" rack and pinion focuser provides a solid, slip-free platform for heavy imaging trains, with a smooth lock mechanism to hold focus securely.

    Comparing the Optical Grades

    The images below show the same view of Saturn captured through each available optical grade, under identical conditions -- a visual illustration of how each step up in wavefront accuracy sharpens contrast and fine detail.

    Saturn viewed through 1/6 PV Professional grade optics

    1/6 PV (Professional)

    Saturn viewed through 1/8 PV Research grade optics

    1/8 PV (Research)

    Saturn viewed through 1/10 PV Ultra grade optics

    1/10 PV (Ultra)

  • What makes the IDEAL 8's 1/6 PV optics different from standard Newtonians?

    Most standard Newtonians are specified as "diffraction limited," which corresponds to a 1/4 PV wavefront accuracy. The IDEAL 8 guarantees a 1/6 PV wavefront, a significantly higher standard of optical precision. This is achieved through hand-figuring and is verified with an individual Zygo interferometer report for each mirror, resulting in higher image contrast and sharpness.

    How does the f/4.5 focal ratio of the IDEAL 8 benefit deep-sky imaging?

    An f/4.5 system is considered "fast," meaning it collects light more rapidly than a telescope with a higher f-ratio (like f/8 or f/10). For imagers, this means you can achieve the same image brightness in a much shorter exposure time. This reduces the strain on your mount's tracking and allows you to capture more data in a single night.

    Will I see a difference between the 1/6 PV and 1/10 PV upgrade on a target like Jupiter?

    Yes, especially during moments of steady seeing. While the 1/6 PV standard provides excellent views, upgrading to 1/10 PV pushes the mirror's surface accuracy to the limit. On a detailed target like Jupiter, this translates to finer, higher-contrast details in the cloud bands and more subtle features becoming visible. The higher the optical quality, the more resilient the image is to atmospheric turbulence.

    What is the purpose of the 9-point mirror cell in the IDEAL 8?

    The CNC-machined 9-point cell provides optimal support for the 200mm primary mirror. It distributes the weight of the glass evenly across nine specific points, preventing gravity from deforming the mirror's precise shape as the telescope is aimed at different parts of the sky. This ensures the telescope maintains its collimation and optical performance regardless of its orientation.

    Is the 7kg weight of the IDEAL 8 OTA manageable for portable mounts?

    At a nominal weight of 7kg, the IDEAL 8 optical tube is relatively lightweight for its 200mm aperture. This makes it compatible with a wide range of mid-range equatorial mounts (typically those rated for 13-15kg or more for imaging), including many popular portable setups. Always account for the additional weight of your camera, guide scope, and other accessories.

    What is the function of the 12-volt fan on the IDEAL 8?

    The integrated 12-volt fan is a crucial feature for thermal management. It actively draws air over the back of the primary mirror, helping it reach the same temperature as the outside air much faster. This process, called thermal equalization, minimizes "tube currents"—internal air turbulence that can soften the image—leading to sharper, more stable views.

  • Optics Grade 1/6 PV Wavefront Standard (Upgrades to 1/8 PV & 1/10 PV available)
    Primary Mirror Diameter 200mm
    Focal Length 900mm
    Focal Ratio f/4.5
    Secondary Mirror Size 63mm
    Focuser Eris 2" Rack and Pinion with smooth lock
    Mirror Cell CNC 9-point suspension
    Mirror Cooling 12-volt fan
    Tube Material Aluminium
    Tube Weight 7kg (nominal)
    Tube Diameter 225mm
    Tube Length 860mm
    Tube Finish Galaxy Silver
  • Orion Optics UK 1-Year Warranty