ZWO Narrowband SII Filter - 7nm
- Isolates the 672nm Sulfur-II emission line
- 7nm bandpass for high-contrast imaging
- Standard 1.25" threaded metal cell
- 1/4 wave polished substrate with multi-layer coatings
The ZWO SII 7nm 1.25" Filter isolates the deep-red Sulfur-II emission line centered at 672nm, a critical wavelength for mapping ionized structure in emission nebulae. Its tight 7nm bandpass dramatically increases contrast by rejecting light pollution and moonlight, while the 1/4 wave polished substrate ensures that the finest details are not lost to optical imperfections.
By restricting transmission to a narrow 7nm window around the 672nm SII line, this filter renders the sky background nearly black, causing faint nebulosity to stand out with striking clarity. This high signal-to-noise ratio is essential for revealing the delicate, wispy structures in supernova remnants like the Veil Nebula (NGC 6960) or the intricate star-forming regions within the Eagle Nebula (M16).
Each ZWO narrowband filter is ground and polished to a 1/4 wave surface accuracy, a specification that prevents distortion and maintains image sharpness across the field. Multiple layers of anti-reflection coatings are then applied to eliminate halos around bright stars and maximize light transmission within the 7nm bandpass, preserving the critical signal from your target.
This filter is the essential "S" component in the SHO color palette, made famous by images from the Hubble Space Telescope. When you combine data captured through this SII filter with separate exposures using Hydrogen-alpha and Oxygen-III filters, you can create stunning, scientifically valuable images that map the chemical composition of nebulae in vibrant gold, cyan, and blue hues. The standard 1.25" threaded cell ensures compatibility with most filter wheels and camera nosepieces.
The ZWO 7nm SII filter is a narrowband filter designed for astrophotography with monochrome cameras. It isolates the 672nm wavelength of light emitted by ionized sulfur, which is crucial for capturing specific structural details in emission nebulae and creating "Hubble Palette" (SHO) images.
While technically possible, it is not recommended. Color cameras have a Bayer matrix (RGB filters) over their sensors, and only the red pixels will receive signal from the 672nm SII line. This results in a significant loss of signal and resolution, making a monochrome camera the superior choice for narrowband imaging.
On a target like the Rosette Nebula, the ZWO 7nm SII filter excels at revealing the shock fronts and ionization structures that are less prominent in Hydrogen-alpha. It isolates the outer shell and filamentary details, providing the essential "S" channel data that adds depth and a golden hue to a final SHO composite image.
With a fast f/4 system, you can typically start with exposures of 300 to 600 seconds per sub-frame from a moderately light-polluted (Bortle 4-5) site. Sulfur-II is often the faintest of the three main narrowband channels (Ha, OIII, SII), so you may need to expose 1.5x to 2x longer for SII than you do for Hydrogen-alpha to achieve a comparable signal level.
A narrower bandpass is more effective at rejecting unwanted light, such as from city glow, moonlight, and natural skyglow. The 7nm bandpass provides a very high-contrast view by darkening the sky background significantly, making it superior to wider 12nm or 15nm filters, especially from suburban locations.
Yes. The ZWO 7nm SII filter is mounted in a standard 1.25" metal cell with M28.5x0.6 threads. It is fully compatible with any 1.25" filter wheel, filter drawer, or accessory that accepts standard 1.25" threaded filters.
| SKU | ZWO-SII7NM1.25 |
| Filter Type | Sulfur-II (SII) Narrowband |
| Bandwidth | 7 nm |
| Size | 31.75mm (1.25") |
| Mount Style | Threaded Cell |
| Shape | Round |
| Category | Single Filter |
1.25" Mounted Sulfur II 7nm Filter
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Protective Plastic Case
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