Howie Glatter Single 650nm Red Beam Laser Collimator - 1.25"/2"
- 650nm Single Red Laser Beam
- Factory-Aligned to 15 Arc-Seconds
- Fits 1.25" and 2" Eyepiece Holders
- Class IIIa Laser (Maximum 5 mW Output)
- Includes 1mm Aperture Stop for Precision
The Howie Glatter Single 650nm Red Beam Laser Collimator establishes an exact optical axis, providing a reference line aligned to within 15 arc-seconds for precise telescope collimation. This Class IIIa laser fits both 1.25" and 2" eyepiece holders and uses a solid-state laser diode that does not fade or change with time and use, powered by an included 123A lithium battery. The 650 nm beam provides the reference line for aligning optics in Newtonian, refractor, and Cassegrain telescopes.
A laser collimator is useless if it can't hold its own alignment. Each Howie Glatter collimator is factory-aligned to a tolerance of 15 arc-seconds, which translates to a deviation of just 0.1 inches at a distance of 20 feet. To ensure this alignment holds, every unit is shock-tested by being struck at least a dozen times on three different axes before its alignment is re-verified, simulating a drop from the focuser of a large Dobsonian.
The beam from a raw laser diode is often fuzzy and elliptical, making it difficult to judge the exact center. This 650 nm collimator includes a removable 1 mm aperture stop that push-fits into the laser aperture, transforming the beam into a tiny, circular point. At a distance, this focused beam creates a star-like diffraction pattern, with a central dot surrounded by faint rings that allow for extremely accurate centering on your primary mirror's center mark.
This collimator fits both 1.25" and 2" eyepiece holders. The front of the laser features a 3/8-32 thread, allowing for the addition of optional accessories like holographic attachments (square grid, crosshair, or concentric circles) or a Barlow attachment for advanced collimation techniques.
This single-beam laser provides the essential reference line needed to align the optical train of most amateur telescopes. For Newtonians, it allows precise adjustment of the secondary and primary mirrors. On refractors, it verifies drawtube alignment and checks the objective's tilt. For Cassegrain systems, it helps align the back axis and secondary mirror, establishing the foundation for a well-collimated system.
While both the 650nm and 635nm lasers have the same 5 mW maximum power output, the human eye perceives the 635nm wavelength as two to three times brighter. This makes the 635nm version a better choice for collimating in early twilight or brighter ambient light. For collimating in darkness, however, the 650nm laser is perfectly adequate especially for single-beam collimators, which concentrate all the laser light in the central beam.
The key difference is its verified alignment and durability. Each Howie Glatter collimator is aligned to 15 arc-seconds and then subjected to a rigorous shock-testing procedure, struck at least a dozen times on three axes, to ensure it maintains that alignment even after being dropped or mishandled.
The 1 mm aperture stop simply push-fits into the laser opening. It sharpens the fuzzy, elliptical beam from the raw diode into a tiny, circular point. This produces a star-like diffraction pattern on your primary mirror, allowing for much more precise centering of the beam on your center mark.
Howie's instructions: the return spot on the collimator face can be seen from the front of the telescope, looking down the tube, by double reflection in the primary and secondary, and you may need a helper to turn the primary screws while you watch. The primary can also be adjusted by making the up-going and down-going beam impact points on the secondary coincide; with an open tube this can make solo collimation easier.
Yes. When placed in the focuser (without a diagonal), the Howie Glatter laser projects a beam through the objective lens. You can check that the focuser drawtube is aligned with the center of the objective. The reflection from the objective lens surfaces back to the collimator face is then used to adjust the objective cell's tilt. For safety, always place a beam stop, like a piece of masking tape, across the dew shield opening to prevent the beam from exiting the front of the telescope.
The front of the collimator has a 3/8-32 thread. This allows you to attach optional accessories sold separately, such as Howie Glatter's holographic attachments (square grid, concentric circles, etc.) or a Barlow attachment for more advanced collimation techniques.
| Model | LC2125-650 |
| Wavelength | 650 nm (red) |
| Beam | Single beam |
| Fits | 1.25" and 2" eyepiece holders |
| Laser Class | IIIa (maximum output 5 mW) |
| Alignment | Factory-aligned to 15 arc-seconds (0.1 in at 20 ft) |
| Laser Source | Solid-state laser diode |
| Shock Testing | Each collimator struck at least a dozen times on three axes, alignment rechecked |
| Battery | 123A lithium |
| Attachment Thread | 3/8-32 (current version, identified by a visible ring) |
| Optional Accessories | Holographic attachments (square grid, concentric circle, cross hair), Barlow attachment, Variable Laser Brightness cap |
| Use | Newtonian, refractor and Cassegrain collimation |
Howie Glatter 650 nm single-beam 1.25/2" laser collimator
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123A lithium battery
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1 mm aperture stop
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Protective case
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