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Baader FlipMirror II Star Diagonal

SKU BAA-2458055
Original price CA$332.00 - Original price CA$332.00
Original price
CA$332.00
CA$332.00 - CA$332.00
Current price CA$332.00
Price Match Policy!
  • Instantly switch between three different instrument ports
  • Straight-through port for primary camera or spectrograph
  • 90° mirrored port for visual observation or secondary camera
  • Auxiliary bottom port for guiders or calibration lamps
  • Precision-coated mirror ensures high-quality images
  • Compact design minimizes back-focus consumption
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • Baader FlipMirror II Star Diagonal

    The Baader FlipMirror II Star Diagonal transforms your telescope's single focuser port into a versatile three-port imaging hub, eliminating the need to constantly swap accessories in the dark. It provides a straight-through path for a primary camera, a 90-degree mirrored path with a 32mm illuminated field for an eyepiece or guider, and a unique bottom port for calibration lamps or an off-axis guider prism. This system is the definitive solution for streamlining complex imaging, visual, and spectroscopy workflows.

    A Three-Port Hub to Eliminate Instrument Swapping

    A single telescope port is a major bottleneck for serious astronomers. The FlipMirror II solves this by providing three configurable ports, allowing you to have an imager, an eyepiece, and a guider or spectrograph calibration source connected simultaneously. A simple turn of the rotary knob switches the light path between the straight-through rear port and the 90-degree top port, saving time and preventing wear on your equipment.

    High-Fidelity Optics for Visual and Imaging

    At the core of the BFM II is a precise, surface-mirrored flip mirror featuring a multi-layer aluminum coating. This ensures that the angled light path delivers the same image brightness and resolution as a high-end standalone star diagonal. Whether you are conducting visual observations or capturing high-resolution images with small-pixel cameras, the FlipMirror II maintains the integrity of your optical train without compromise.

    Total System Integration with the Baader Adapter Universe

    Designed for maximum compatibility, the FlipMirror II seamlessly integrates with the comprehensive Baader Astro T-2, M48, and M68 adapter systems. This modularity allows you to connect virtually any camera, eyepiece, or accessory while achieving precise optical alignment. Its thoughtful, compact design conserves precious back-focus, though any new component in the optical train requires consideration of the total path length. The system also enables precise adjustment of all light paths to achieve parfocality between your different instruments.

    Unlocking Advanced Workflows in Spectroscopy and Guiding

    The BFM II is purpose-built for advanced applications. The bottom auxiliary port can be used to mount a calibration lamp, allowing you to calibrate spectra without removing your spectrograph from the main port. The back of the flip mirror is also coated and masked to direct this calibration light onto the spectrograph slit. Alternatively, this port can house an off-axis-guider pickoff prism that remains independent of the main mirror's position, ensuring consistent guiding no matter which primary port is active.

  • What are the three ports on the Baader FlipMirror II for?

    The Baader FlipMirror II provides three connection points to manage your equipment efficiently:

    • Rear Port (Straight-Through): This is the primary position for your main imaging camera or a spectrograph, offering a direct, unobstructed light path.
    • Top Port (90° Angled): This port uses the internal mirror and functions like a star diagonal. It's ideal for a visual eyepiece for centering objects, or for a secondary camera.
    • Bottom Port (Auxiliary): This port is designed for specialized tools like a spectrograph calibration lamp or an off-axis guider pick-off prism.

    Will the Baader FlipMirror II degrade my planetary images?

    No. The Baader FlipMirror II uses a precise, surface-mirrored diagonal with a high-reflectivity multi-layer aluminum coating. Its optical quality is engineered to be on par with high-end star diagonals, ensuring that it does not introduce aberrations or reduce sharpness, even when used for high-resolution imaging with cameras that have small pixels.

    How does the Baader FlipMirror II help with spectroscopy?

    The FlipMirror II is a powerful tool for spectroscopy. You can keep your spectrograph attached to the main straight-through port while attaching a calibration lamp to the bottom auxiliary port. The back of the flip mirror is specially coated to redirect the lamp's light into the spectrograph's slit by simply flipping the mirror, allowing for quick and easy calibration frames without disassembling your setup.

    Can I motorize the Baader FlipMirror II for remote operation?

    Yes, the Baader FlipMirror II is designed for future motorization. It can be operated with an optional toothed belt and motor, which can be controlled by systems like the Baader SteelDrive II controller. This allows you to switch between the imaging and visual ports remotely from your computer, which is essential for automated observatories.

    How would I set up the Baader FlipMirror II with my Celestron SCT and a ZWO camera?

    For a common SCT setup, you would attach the Baader FlipMirror II to your telescope's visual back. Your primary ZWO imaging camera would be connected to the straight-through rear port. An eyepiece for finding and centering objects would go in the 90-degree top port. If you use an off-axis guider, the OAG's pick-off prism could be attached to the bottom port, providing a permanent guiding solution regardless of which main port you are using.

    Does the Baader FlipMirror II consume a lot of back-focus?

    The Baader FlipMirror II has a compact and efficient design to minimize back-focus consumption. However, like any accessory added to an optical train (e.g., filter wheels, OAGs), it does have a specific light path length that must be accounted for. It's crucial to check the back-focus requirements of your telescope and any reducers or correctors to ensure you can reach focus with your camera.

  • Net weight (kg) 0.24
    Optical length (mm) 55 mm with S52, 59 mm with M48/T-2
    Inner Connection (eyepiece/-camera-sided) M48, S52
    Outer Connection (eyepiece/-camera-sided) M48
    Inner Connection (lens sided) M42 x 0.75 (T-2), M48, S52
    Optical Design Mirror Diagonal
  • Baader Planetarium Warranty