Pellucid Glasshaven light pollution filter 1.25 in, observatory grade
Light pollution · 1.25 in · 190 nm bandpass
$139
Catalog preview. Not available for purchase.
- Grade
- Observatory grade
- Coating
- Standard coating
- Case
- Plastic case
- Edition
- 2026 edition
Specifications
| Filter type | Light pollution suppression filter |
|---|---|
| Cell | 1.25 in aluminum cell, M28.5 x 0.6 thread |
| Bandpass (FWHM) | 190 nm |
| Peak transmission | 88% |
| Substrate | Optical glass |
| Glass thickness | 2.0 mm |
| Grade | Observatory grade |
| Coating | Standard coating |
| Case | Plastic case |
| Edition | 2026 edition |
Description
The Glasshaven light pollution filter is a broadband filter in a 1.25 in threaded cell. It transmits most of the visible spectrum while blocking part of the light emitted by sodium and mercury vapor street lamps, which contribute much of the glow over towns and cities. Its peak transmission of about 88 percent keeps the view bright enough for stars, planets, and the Moon, so you can leave it in place for general observing rather than switching to a different filter for each target. The filter is intended for use under suburban and urban skies, where the sky background is brightest.
Light pollution adds a diffuse glow that spreads across the sky background and lowers contrast for faint objects. By reducing the wavelengths that make up that glow, the filter darkens the background more than it dims extended objects that emit across a wide range of colors. Galaxies, globular clusters, and open clusters often show more structure under suburban skies with this filter in place. Emission nebulae respond differently, because a UHC or OIII filter usually gives more contrast on those targets than a broadband filter does, and you may find it useful to carry both.
Stars and planets keep their natural colors, although the filter reduces the total light reaching your eye, so faint stars and dim detail will appear slightly fainter than in an unfiltered view. Use it with a telescope of 100 mm aperture or larger when you are looking for faint outer structure in galaxies. Allow your eyes about 15 minutes of dark adaptation after you change the filter, and keep the glass clean, since dust and fingerprints can reduce contrast more than the filter itself does.
The filter threads into any 1.25 in eyepiece or the nosepiece of a 1.25 in diagonal. Both faces of the glass carry an anti-reflection coating, which limits the light lost at each surface and reduces internal reflections.
About this configuration
This listing covers one configuration of the Pellucid Glasshaven light pollution filter 1.25 in, defined by its grade, coating, case, and edition year. The observatory grade comes with a measured transmission curve for the individual filter in the box. Observatory grade glass has the tightest flatness tolerance in the Glasshaven line, which suits imaging with long focal lengths. The standard coating is applied to the filter side of the glass, with a single anti-reflection layer on the back.
A plastic case is light and stacks with other filter cases in an accessory box. This is the 2026 edition, the most recent version of the Glasshaven line in the catalog. The transmission figures in the specifications apply to every configuration of the Glasshaven line.
What's in the box
- Light pollution filter in 1.25 in threaded cell
- Padded storage pouch
- Test report with measured transmission curve
- Plastic storage case
Compatibility notes
- Threads into 1.25 in eyepieces, diagonals, and filter wheels (M28.5 x 0.6).
- Suited to telescopes of any aperture, with the greatest effect under suburban and urban skies.