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For telescopes where this ratio is relatively low (short, wide scopes) the sweet spot is small: for these scopes regular collimation is crucial so that objects at the centre of the view can be seen at their best.

Newtonian reflector telescopes are popular for amateurs for their relatively low cost for any given aperture and their naturally good colour correction. But due to the loose way in which the two mirrors are typically held, Newtonians can lose their optical alignment relatively easily.

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Collimation realigns the mirrors to bring the good area back to the middle of the eyepiece field, restoring the best star images and allowing you to see the most planetary detail.

[caption id="attachment_53954" align="alignleft" width="1200"] How to collimate a Newtonian telescope. Credit: Martin Lewis[/caption]

Familiarise yourself with the view through the collimating tool’s eyehole. What you see may be confusing at first, so compare your view with the labelled image above for a mis-collimated scope. This will help you to identify the features that need to be repositioned.

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Although the job of collimating a Newtonian may seem daunting if you’ve never done it, once you have the right tools and understand the principles, it becomes relatively quick and easy.

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Through the tool’s eyehole look for the centre ring on the primary mirror. Move the secondary mirror with the adjuster screws to bring this ring under the point where the shadow of the cross-wires intersect. You may need a screwdriver or other tools for this.

Our step-by-step guide below describes a relatively easy way to re-collimate your Newtonian telescope with simple tools, by making small adjustments to the secondary mirror assembly and to the primary mirror cell.

Our step-by-step guide will give you all the info you need to get your Newtonian collimated and offering clear, crisp views.

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If the mirrors in the telescope become slightly misaligned – as a result of a knock or changes in temperature – the sweet spot can move away from the middle of the eyepiece’s field of view and end up off-centre.

Next time you perform any fine-tuning collimation it may be at night. In this case, shine a red torch into the side of the collimating tool to illuminate the middle of the cross-wires and show the dark collimating tool’s eyehole.

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We’re not using a laser-based telescope collimation device here; these do allow precision alignment but add an extra layer of complexity.

Size of sweet spot is another aspect to bear in mind. In a Newtonian it is dependent on the ratio between the telescope’s focal length and the diameter of its main mirror.

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Now align the primary mirror using its adjustment screws, until the peephole spot is centred in the main mirror’s centre ring. If you moved the primary a lot you may need to re-check the secondary alignment, but otherwise your scope’s collimated and good to go!

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This sweet spot is where stars appear sharpest: it’s the circular area on a Newtonian’s main mirror where light is focused to maximum resolution.

Do your first collimation in the daytime, when you can see what’s going on. Secure your Cheshire eyepiece collimating tool in the focuser with the open side facing the sky to let light in. Next, point the scope at the bright sky, but well away from the Sun.

Outside the sweet spot star images appear larger and get distorted into V-shapes. This distortion away from the centre of the view is present in all Newtonians, even perfect ones.

Much more so than for Newtonians with a higher ratio (long and relatively thin): they will have a much larger sweet spot and will be far more forgiving of small amounts of misalignment.

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When the first stage of collimation is done the view should look like the one above, with the centre ring on the primary mirror right under the middle of the cross-wire shadows. Tighten up the secondary mirror screws, being careful to maintain alignment.

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