Orion Optics UK IDEAL 16 Optical Tube Assembly
- 400mm (16") Primary Mirror
- 1600mm Focal Length
- Fast f/4 Focal Ratio
- Standard 1/6 PV Wavefront Optics with Zygo Report
- CNC-Machined 9-Point Mirror Cell with 12V Fan
- 29kg Nominal Tube Weight
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Lancer l'assistant d'imagerieThe Orion Optics UK IDEAL 16 Optical Tube Assembly combines a massive 400mm aperture with a fast f/4 focal ratio for unparalleled deep-sky imaging and observation. Its 1600mm focal length provides the scale for detailed planetary views, all built upon a hand-figured primary mirror guaranteed to a 1/6 PV wavefront standard. The entire 29kg assembly is supported by a CNC-machined 9-point mirror cell, ensuring the primary optic maintains its precise figure regardless of orientation.
At the heart of the IDEAL 16 is a 400mm primary mirror, hand-figured in the UK to a demanding 1/6 PV wavefront accuracy. This grade exceeds the "diffraction-limited" standard, delivering visibly higher contrast on planetary details and tighter star points. The fast f/4 focal ratio creates an incredibly bright image plane and a wide field of view, allowing you to capture vast nebulae like the North American Nebula (NGC 7000) in a single frame with reduced exposure times. Every optic is supplied with its own Zygo interferometer test report, providing certified proof of its exceptional quality.
A large, fast mirror is only as good as its support system. The IDEAL 16 utilizes a robust 9-point suspension mirror cell, CNC-machined for precision, to distribute the mirror's weight evenly and prevent performance-robbing flexure. The 1580mm aluminium tube keeps the total weight to a manageable 29kg, while an integrated 12-volt fan accelerates mirror cooling to ambient temperature, minimizing tube currents and ensuring sharp views sooner.
To handle modern imaging cameras and heavy eyepiece combinations, the IDEAL 16 is equipped with a robust Eris 2" rack and pinion focuser. This design offers a significant advantage over simpler Crayford focusers by providing a positive, slip-free rack gear, ensuring it can hold heavy equipment without shifting focus. A smooth-locking mechanism secures your eyepiece or camera with perfect centrality to the 82mm secondary mirror, preserving the optical alignment critical for a fast f/4 system.
While the standard 1/6 PV wavefront optic delivers exceptional views, optional upgrades to 1/8 PV or 1/10 PV are available for the most demanding applications. Peak-to-Valley (PV) wavefront error measures how closely the mirror's surface matches a perfect parabola; a smaller fraction indicates a more precise figure. Upgrading from 1/6 to 1/10 PV yields a noticeable increase in fine detail and contrast, especially crucial for high-resolution planetary imaging where every fraction of a wavelength counts.
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.
1/6 PV (Professional)
1/8 PV (Research)
1/10 PV (Ultra)
With a nominal tube weight of 29kg and a length of 1580mm, the IDEAL 16 requires a substantial equatorial mount. You should look for a mount with a payload capacity of at least 45-50kg for visual use, and preferably higher for stable astrophotography to account for cameras, guide scopes, and other accessories.
Yes, for dedicated planetary imagers, the 1/10 PV upgrade is a significant investment. The higher surface accuracy translates directly to higher contrast on low-contrast features, such as subtle swirls in Jupiter's zones or faint festoons. While the 1/6 PV standard is excellent, the 1/10 PV ensures your final image resolution is limited by the atmosphere, not the telescope's mirror.
The IDEAL 16's combination of a 400mm aperture and f/4 focal ratio is perfect for large targets like M31. The massive light-gathering ability will reveal faint outer dust lanes and companion galaxies M32 and M110 with stunning clarity. The fast focal ratio provides a wide field of view, allowing you to frame the entire galaxy with appropriate eyepieces or a full-frame camera.
A large 400mm mirror is heavy and can deform under its own weight if not supported properly. The CNC 9 point suspension cell provides precisely calculated support points across the back of the mirror. This prevents sagging and flexure as the telescope moves across the sky, maintaining the mirror's precise optical figure and ensuring sharp focus.
Yes, like all fast Newtonian telescopes, the IDEAL 16 will exhibit coma, an aberration that makes stars at the edge of the field of view appear elongated. For astrophotography or wide-field visual observation with 2" eyepieces, using a high-quality coma corrector is essential to achieve sharp, point-like stars across the entire frame.
A large 400mm mirror has significant thermal mass and can take hours to cool to the ambient night air temperature. The integrated 12 volt fan actively circulates air behind the mirror, dramatically reducing this cooldown time. This minimizes "tube currents"—thermals rising from the mirror that distort the view—allowing you to start high-magnification observing or imaging much faster.
| Optical Design | Newtonian Reflector |
| Primary Mirror Diameter | 400mm |
| Focal Length | 1600mm |
| Focal Ratio | f/4 |
| Standard Optics Grade | 1/6 PV wavefront |
| Optics Upgrade Options | 1/8 PV, 1/10 PV |
| Secondary Mirror Size | 82mm |
| Focuser | Eris 2" Rack and Pinion with smooth lock |
| Mirror Cell | CNC 9 point suspension |
| Mirror Cooling | 12 volt fan |
| Tube Material | Aluminium |
| Tube Diameter | 434mm |
| Tube Length | 1580mm |
| Tube Weight | 29kg (nominal) |
| Tube Finish | Galaxy Silver |
IDEAL 16 Optical Tube Assembly
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