Baader C2 Swan-Band Comet Filter (15nm)
- Targets C2 Swan Bands in comet gas tails
- 15nm bandpass for high-contrast views
- O-III parallel transmission for nebula observation
- Available in 1.25" and 2" mounted formats
The Baader C2 Swan-Band Comet Filter isolates faint cometary emissions within a narrow 15nm bandpass, dramatically increasing the contrast of gas tails against the skyglow. This specialized design targets the unique C2 Swan Bands, revealing delicate streamers and structures that are lost when using general-purpose nebula filters, and is available in both 1.25" and 2" mounted formats to fit any standard eyepiece or accessory.
While a comet's bright dust tail is simply reflected sunlight, its ion or gas tail glows with its own distinct light. The Baader C2 Swan-Band filter is engineered with a 15nm bandpass to isolate this specific emission from diatomic carbon (C2), which is ejected from the comet's nucleus. By blocking out interfering skyglow and light from the dust tail, the filter makes the faint, ethereal structure of the gas tail visible.
Unlike single-purpose comet filters, the Baader C2 Swan-Band filter is designed to be "O-III parallel." This means its transmission window also passes the critical 501nm line from doubly-ionized oxygen (O-III), the same light emitted by planetary and other emission nebulae. This clever design allows the filter to serve a dual role in your accessory case, enhancing views of objects like the Dumbbell Nebula (M27) or the Orion Nebula (M42).
While a dedicated, narrower O-III filter will provide the absolute highest contrast on nebulae, the C2 filter offers a significant boost over unfiltered views, making it a more useful tool than a filter you might only use once every few years for a bright comet.
An observer's first instinct might be to use a standard UHC or O-III nebula filter on a comet, but this is often counterproductive. Those filters are designed to block the very wavelengths the comet's gas tail emits.
The Baader C2 Swan-Band filter is the correct tool for the job. It selectively passes the light from the gas tail while rejecting the light that obscures it, delivering a view that general-purpose filters cannot match.
The Baader C2 Swan-Band filter is a narrow-band filter designed to increase the contrast of a comet's gas (ion) tail. It has a 15nm bandpass that selectively transmits light from diatomic carbon (C2), which is the primary emission from the gas tail, while blocking out light pollution and excessive glare from the comet's dust tail.
Yes. The filter is designed with "O-III parallel" transmission, meaning it also passes light from doubly-ionized oxygen. This makes it effective for enhancing contrast on many emission nebulae, particularly planetary nebulae like the Ring Nebula (M57) and larger structures like the Veil Nebula (NGC 6960).
A dedicated O-III filter will typically have a narrower bandpass (e.g., 7-12nm) and will provide higher contrast on O-III-rich objects. The Baader C2 filter's 15nm bandpass is wider to accommodate the Swan Bands, so while it provides a significant enhancement on nebulae, a specialized O-III filter will yield a darker sky background and more pronounced detail on those specific targets.
No, the opposite is true. The dust tail shines by reflecting sunlight, which is broadband white light. This filter is designed to block most of that light to make the faint, self-luminous gas tail stand out. It will dim the dust tail and coma significantly to improve the visibility of the ion tail.
Absolutely. In a 10" telescope, a bright comet's coma and dust tail can be overwhelmingly bright, washing out the fainter gas tail. The Baader C2 filter will dim the coma and dust tail, darkening the background sky and allowing the delicate streamers, knots, and structure within the gas tail to become clearly visible. It often reveals a tail that was completely invisible without filtration.
Yes, the filter can be used for imaging. Because it passes O-III, it can be effective for capturing detail in planetary nebulae. For serious tri-color imaging, dedicated narrowband filters (O-III, H-alpha, S-II) are superior, but for one-shot color or monochrome imaging, the C2 filter can help isolate nebular structure from a light-polluted sky.
| Bandpass | 15nm |
| Primary Transmission | C2 Swan Bands |
| Secondary Transmission | O-III Parallel |
| Available Sizes | 1.25" Mounted, 2" Mounted |
| Net weight (kg) | 0.01 |
| Filter shape | round |
| Single or Set? | Single Filter |
| Filter mounted | Mounted (LPFC 6mm) |
| Filter Usage | Gas evolution of comets, O-III-paralel Imaging, Contrast Enhancement |
| Filter Thickness (without cell) | 2 mm |
| CWL (Central Wavelength) | 513 nm (for the C2 lines at 511 and 514nm) |
| Transmission Range | ≤ 505 – 520 nm |
| AR-Coating | dielectrically coated, planeoptically polished |
| Filter size | 2 inch |
| Type of Filter | Bandpass |
| HBW (Halfbandwidth) | ≤ 15nm |
Baader C2 Swan-Band Comet Filter (Selected Size)
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Protective Storage Case
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