A laser collimator is used to verify that a telescope’s optical axis is properly aligned. By projecting a narrow laser beam onto a distant target, the size of the illuminated spot reveals the angular deviation of the collimation.
The relationship between the measured spot diameter (d), the distance to the target (L), and the collimation error angle (ΞΈ) follows simple trigonometry. For small angles, the tangent of ΞΈ is approximately equal to the ratio of the spot size to the distance.
Because the angles involved are usually fractions of a degree, converting the result to arcβseconds provides a convenient unit for telescope alignment tolerances.
How do I use the laser collimator angle calculator?
What does the collimation error angle tell me?
Why is it important to check the collimation of my telescope?
Can I use this calculator for any type of laser collimator?
What is the relationship between spot size and collimation error angle?
How do I interpret the results from this calculator?
Is there a limit to how far I can use this calculator for?
Results are for informational purposes only and do not constitute professional advice.
