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Baader Telecentric System TZ-3 - 3x Research Grade

SKU BAA-2459257
Original price CA$648.00 - Original price CA$648.00
Original price
CA$648.00
CA$648.00 - CA$648.00
Current price CA$648.00
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  • 3x Telecentric Focal Extender
  • Engineered for Narrowband H-alpha Solar Filters
  • Produces a Parallel (Collimated) Light Path
  • Maintains Etalon Bandpass Across the Entire Field
  • Research Grade Optical Design
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  • Description
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  • Baader Telecentric System TZ-3 - 3x Research Grade

    The Baader Telecentric System TZ-3 is an essential optical component for high-resolution solar imaging, providing a 3x focal length amplification designed to create a perfectly parallel light path. This research-grade system is not a simple Barlow lens; it is an engineered solution to ensure that expensive, sub-angstrom H-alpha etalons deliver their full theoretical contrast and resolution across the entire imaging sensor.

    A 3x Focal Extender for Optimized Etalon Illumination

    The primary function of the TZ-3 is to convert your telescope's native focal ratio into the slow, collimated beam required by SolarSpectrum and other high-end H-alpha filters. By increasing the effective focal length by a factor of 3x, a telescope operating around f/10 is transformed into the target f/30 system, ensuring every ray of light passes through the delicate etalon perpendicularly. This precise illumination is the only way to prevent bandpass shift and preserve uniform detail from the center of the solar disk to the limb.

    The Telecentric Principle: A Parallel Light Path, Not Just Magnification

    A telecentric system is designed to place its exit pupil at infinity. The result is that principal rays from any point in the field of view strike the image plane parallel to the main optical axis, as if they originated from the center of the field. This is fundamentally different from a Barlow, where off-axis rays are still angled. This parallel light path is the key to the TZ-3's function, guaranteeing that the filter's bandpass remains constant and does not shift toward shorter wavelengths at the edge of the field.

    A Mandatory Component for Sub-Angstrom Solar Etalons

    For any H-alpha observation with a filter narrower than 1 Angstrom, a telecentric system is not optional—it is mandatory. Feeding a non-parallel, or conical, light beam into a sub-angstrom etalon destroys its contrast. An etalon rated for 0.5Å performance might deliver only 0.7Å or worse if used with a standard Barlow at the same focal ratio. The Baader TZ-3 is the prerequisite for unlocking the true, high-contrast potential of your specialized solar filter, revealing fine spicules, plage, and filament details that would otherwise be lost to bandpass artifacts.

    Baader TZ-3 vs. A Standard Barlow Lens: Why It Matters

    While both a Barlow and a Telecentric system increase focal length, their impact on a narrowband filter is radically different. A Barlow lens simply makes the light cone narrower; it does not make the rays parallel.

    • Baader TZ-3: Creates a true, parallel optical path. The etalon sees the same perpendicular light rays across the entire field, preserving the specified bandpass and delivering maximum contrast uniformly.
    • Barlow Lens: Creates a converging light cone. Off-axis rays still enter the etalon at an angle, causing a spectral shift that degrades contrast and resolution, especially away from the center of the field. Using a Barlow in a serious H-alpha system is a fundamental optical mismatch.
  • Why is the Baader TZ-3 essential for my sub-angstrom H-alpha filter?

    Sub-angstrom H-alpha filters, known as etalons, require a perfectly parallel light path (collimated beam) to function correctly. The Baader TZ-3 is specifically designed to create this beam. Using a standard Barlow lens, even if it achieves the same f-ratio, will result in a conical light path that degrades the filter's performance, severely reducing contrast and detail.

    How is the Baader TZ-3 different from a standard 3x Barlow lens?

    A Barlow lens only magnifies the image by making the light cone narrower. A telecentric system, like the Baader TZ-3, fundamentally re-engineers the optical path to make the light rays parallel to the central axis. This is a critical distinction for narrowband filters, as angled rays cause the filter's bandpass to shift, smearing out fine solar details.

    Can I use the Baader TZ-3 for lunar or planetary imaging?

    While the TZ-3 is optimized for the specific requirements of solar etalons, it can be used as a high-quality 3x focal extender for other targets. However, its primary design goal is to produce a telecentric beam, which is not a requirement for standard planetary imaging where a high-quality Barlow may offer a more compact and cost-effective solution.

    What happens if I use a Barlow instead of the Baader TZ-3 with my SolarSpectrum filter on my f/10 SCT?

    Even if you use a 3x Barlow to achieve f/30, the light entering your SolarSpectrum filter will still be in a converging cone. This will cause a bandpass shift across the field of view. The center of the sun might look sharp, but the detail and contrast towards the limb will be significantly reduced, and the filter will not perform to its specified sub-angstrom rating.

    My telescope is f/7. How does the Baader TZ-3 help me for H-alpha?

    An f/7 telescope with the 3x TZ-3 would result in an f/21 system. This is faster than the ideal f/30 target for many etalons. To compensate, you would need to use an aperture mask or iris diaphragm on your telescope's objective to reduce its effective aperture, thereby slowing the system down to the required f/30, ensuring optimal filter performance.

    Why is the Baader TZ-3 recommended over the older TZ-4 for some setups?

    The Baader TZ-3 features a more modern optical calculation and better clear aperture matching for many modern filter systems. It is often better to use the TZ-3 and slightly reduce your telescope's main aperture to reach the target f/30 than to use an older, mismatched 4x system that may introduce vignetting or other optical compromises.

  • Focal Length Multiplier 3x
    Optical System Telecentric
    Primary Application Narrowband H-alpha Solar Filters
    Net weight (kg) 0.21
    Usage for H-alpha observation with SolarSpectrum filters
    Outer Connection (eyepiece/-camera-sided) M42 x 0.75 (T-2), 2"/SCT Thread (50.8mm)
    Inner Connection (lens sided) M42 x 0.75 (T-2)
    Outer Connection (lens sided) 2"/SCT Thread (50.8mm)
  • Baader Planetarium Warranty