Baader UFC S70 / RASA 36 adapter plate (63667)
234.02 $
Tax included
The Baader UFC S70 adapter plate is designed to connect the Baader Universal Filter Changer (UFC) system to RASA 36 telescopes. This adapter ensures a secure and precise fit, allowing for efficient and convenient filter changes during astrophotography or observation sessions. Built with high-quality materials, it is engineered to maintain optical alignment and performance while integrating seamlessly with your telescope setup.
Baader UFC-Tilter (75225)
255.29 $
Tax included
This tilter is designed to provide an optimally flattened field of view by allowing a shift of up to 1° to compensate for misalignments in the image field. It is an essential tool for astrophotographers and observers seeking precise alignment and improved image quality. The tilter integrates seamlessly with compatible systems, ensuring reliable performance and ease of use.
Baader Filters U-Venus 2" (10862)
308.94 $
Tax included
The Baader U-Venus 2" filter is specifically designed for capturing ultraviolet (UV) light, making it an excellent tool for observing and photographing Venus. This filter isolates UV wavelengths, allowing for detailed imaging of Venusian cloud structures that are otherwise invisible in visible light. It is optimized for astrophotography and is not suitable for visual observation due to its focus on UV transmission.
Baader Filters U-Venus 1.25" (15281)
221.07 $
Tax included
The Baader U-Venus 1.25" filter is a specialized tool designed for capturing ultraviolet (UV) light, making it ideal for imaging Venus. By isolating UV wavelengths, this filter enables detailed observation of the planet's cloud structures, which are not visible in standard visible light. It is specifically suited for astrophotography and is not intended for visual use due to its UV focus.
Baader Filters 1.25" methane filter (20197)
221.07 $
Tax included
The Baader methane band filter is designed for imaging astronomical objects, particularly planets, using webcams and CCD cameras. It is not suitable for visual observation because the human eye is not sensitive to the spectral range covered by this filter. This filter is ideal for capturing methane absorption features in planetary atmospheres, such as those of Jupiter, Saturn, and Uranus.