Skip to content

Language

Country

Vaonis Dual Band Filter for Vespera

by Vaonis
SKU VAO-AC022
Original price CA$559.00 - Original price CA$559.00
Original price
CA$559.00
CA$559.00 - CA$559.00
Current price CA$559.00
Price Match Policy!
  • Dual-band filter isolates Hydrogen-alpha (656.3nm) and Oxygen-III (500.7nm) wavelengths
  • Narrow 12nm bandpass dramatically increases contrast on emission nebulae
  • Integrated electronic chip enables automatic detection by the Vespera telescope
  • Weighs only 17 g (0.6 oz) for seamless integration
Backordered
Availability Info
FREE Shipping in Canada
  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • Vaonis Dual Band Filter for Vespera

    The Vaonis Dual Band Filter for Vespera is a dual-narrowband interference filter engineered to isolate the two most prominent nebula emission lines at a 12nm bandpass. By selectively passing light from Hydrogen-alpha at 656.3nm and Oxygen-III at 500.7nm, this 17 g filter dramatically increases image contrast, even from light-polluted urban skies. An integrated electronic micro-card allows your Vespera to automatically detect the filter and optimize its imaging parameters for breathtaking results on emission targets.

    Isolate H-alpha & O-III with a 12nm Bandpass

    This filter is your Vespera's key to unlocking the faint, colorful structures hidden within nebulae. The tight 12nm bandpass at both the 656.3nm (H-alpha) and 500.7nm (O-III) wavelengths aggressively rejects skyglow from city lights and natural sources, darkening the background and making faint details pop.

    This targeted approach is exceptionally effective for emission targets where these gases are dominant. You'll see significantly improved detail and color separation on the Orion Nebula (M42), planetary nebulae like the Dumbbell Nebula (M27), and vast supernova remnants such as the Veil Nebula.

    Smart Integration: Automatic Vespera Detection and Calibration

    Unlike generic filters, the Vaonis Dual Band Filter is designed to work intelligently with your Vespera. The filter's housing contains an electronic micro-card that communicates directly with the telescope, enabling instant, automatic detection the moment you install it.

    Once detected, Vespera adapts its observation and image processing algorithms specifically for the filter's transmission properties. This seamless integration ensures you get the best possible data without manual adjustments, preserving the simple, automated workflow that defines the Vespera experience. The optical design was engineered to work at full aperture, ensuring no negative impact on your instrument's light-gathering power.

  • What is the main benefit of the Vaonis Dual Band Filter for Vespera?

    The primary benefit is a dramatic increase in contrast when imaging nebulae. By isolating the key Hydrogen-alpha (656.3nm) and Oxygen-III (500.7nm) wavelengths with a narrow 12nm bandpass, the filter darkens the sky background, blocks light pollution, and reveals finer details and richer colors in emission, planetary, and dark nebulae.

    How does the Vaonis Dual Band Filter work with the Vespera telescope?

    It integrates seamlessly. The filter contains an electronic micro-card that allows the Vespera to automatically detect its presence. Once detected, the Vespera's software intelligently adjusts its exposure settings and image processing parameters to optimize the final image for the filter's specific characteristics.

    Will the Vaonis Dual Band Filter improve images of galaxies like Andromeda (M31)?

    No, this filter is not recommended for galaxies. Galaxies are broadband targets, meaning they emit light across the entire visible spectrum. A narrowband filter like this one will block most of that light, resulting in a dim, color-poor image. For galaxies and star clusters, it is best to observe without a filter to capture their full, natural light.

    Is the Vaonis Dual Band Filter effective for imaging the Orion Nebula (M42) from a city?

    Absolutely. The Orion Nebula (M42) is a prime example of an emission nebula rich in both Hydrogen-alpha and Oxygen-III. The 12nm bandpass of this filter is specifically designed to cut through city light pollution and isolate the nebula's light, revealing faint outer structures that would otherwise be washed out.

    What does the 12nm bandpass on the Vaonis Dual Band Filter mean?

    The 12nm bandpass refers to the width of the "window" of light the filter allows to pass through around its target wavelengths. A narrower bandpass is more effective at blocking unwanted light, such as streetlights and natural skyglow. This selectivity is what creates the high-contrast views of nebulae.

    Should I use the Vaonis Dual Band Filter for star clusters like the Hercules Cluster (M13)?

    While primarily for nebulae, the filter can help produce sharper stars in globular clusters like the Hercules Cluster (M13). By cutting out bloated, scattered light from the sky background, stars can appear as tighter points. However, it will also reduce the overall brightness and alter the natural star colors.

  • Net Weight 17 g (0.6 oz)
    Package Weight 60 g (2.12 oz)
    Gross Weight 0.1 kg
    Dimensions Width: 7.80 cm (3.07 in), Thickness: 0.6 cm (0.24 in)
    Materials Glass, Plastic
    Color Black (exterior)
    • Dual Band Filter

      × 1

  • Vaonis 2-Year Warranty