2" BBHS® Mirror – Adjustable Star Diagonal

Compared to purely dielectric coatings, BBHS^® provides a much broader spectral range with 98–99% reflection from just above 390 nm to 2000 nm, and it maintains high reflectivity even with varying viewing angles – the silver layer produces no stray light whatsoever. A trained eye will especially see a greater colour range when using short focal length APO refractors. Particularly in planetary observation at the highest magnifications, a noticeable increase in colour intensity can be easily observed compared to all previous coatings. Additionally, a clear increase in contrast is noticeable due to the absence of any stray light. Only glass-ceramic is used as the substrate for the BBHS^® coating, ensuring extremely fast temperature adaptation and image stability in combination with the CNC-milled aluminium housings.

It has been proven that silver, in combination with temperature-resistant glass-ceramic, offers the absolute best viewing experience with a complete absence of stray light. Try it – the difference is impressive. Afterwards, you will want to observe planets only straight-through or with these hard-silver–coated Sitall mirrors. As a guideline, prisms are recommended for telescopes with a focal ratio of about f/6 to f/7 or slower, and for faster optics, the BBHS^® mirros are preferable.

In addition to the sealed BBHS^®rear-surface coating, the prisms feature the proven Phantom Coating^® Group anti-reflection treatment.

The precisely fitting  2" ClickLock^® eyepiece clamp securely holds even heavy accessories with a simple 20° twist. By cleverly using leverage, the clamping force is multiplied many times. The inserted accessory is held on three sides, similar to a quick-release chuck, preventing any tilting movement. Every eyepiece or measuring device is automatically aligned parallel to the optical axis – even in the case of diameter tolerances.

The BBHS^® mirror is mounted in a CNC-machined aluminium housing and rests stress-free on an adjustable cradle. Just like a high-quality refractor objective, the mirror can also be collimated. This allows the realisation of fully adjustable systems, for example for the construction of binocular telescopes. As with a premium refractor, you will not need to change the collimation during normal use: the 3-point alignment is set at our factory so that the image shows no noticeable rotation around its centre when the star diagonal is rotated by 180° in a correctly aligned eyepiece clamp. Optical and mechanical axes are perfectly matched on our optical test benches. Therefore, make sure to rule out all other potential sources of error – such as a tilted focuser – before adjusting the collimation.

When a BBHS^® mirror leaves our factory, the optical and mechanical axes are aligned rotationally symmetrically with each other on the optical bench. Please note that once the collimation is changed, the warranty on the factory collimation of the BBHS^® star diagonal becomes void. All other warranty coverage remains unaffected. Should you notice immediately after purchase that the optical axis is not correct, please contact the dealer from whom you bought the device without delay.