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Setup and alignment 2 min read

How to collimate a Newtonian reflector

Why reflector mirrors need occasional alignment, how to check it, and the three steps to collimate with a collimation cap or laser.

A Newtonian reflector uses two mirrors: a large primary at the bottom of the tube and a small, tilted secondary near the top. If they are not lined up with each other and with the focuser, stars look like smudges and planets never become sharp. Lining them up is called collimation. Travel and knocks upset it, so check it every few sessions.

Do you need to collimate?

Point at a bright star, centre it at high magnification and turn the focus slightly out. You see a bright ring with a dark shadow in the middle (the secondary mirror). If the shadow sits in the centre of the ring, the telescope is collimated. If it is off to one side, collimate.

Two out-of-focus stars: on the left the dark shadow sits off to one side of the bright ring, so the telescope needs collimating; on the right it sits in the centre.
Needs collimating
The dark shadow sits off to one side
Collimated
The shadow is in the centre of the ring
A bright star at high magnification, turned slightly out of focus.

What you need

  • A collimation cap (a cap with a small central hole) or a laser collimator. A laser must itself be accurate - rotate it in the focuser: the dot on the primary should not move in a circle.
  • A small screwdriver or Allen key for the secondary screws, and daylight or a lamp.
  • Most primary mirrors have a small centre spot; it is a target, not a defect.
Collimation cap view, step 1: the secondary mirror sits off to one side in the focuser, then round and centred.
Step 1: centre the secondary
Before
Secondary off to one side in the focuser
After
Round and centred
Collimation cap view, step 2: the reflection of the primary mirror is off-centre in the secondary, then centred with all three clips in view.
Step 2: tilt the secondary
Before
The primary's reflection is off-centre
After
Whole primary centred, all three clips in view
Collimation cap view, step 3: the dark reflection of the secondary sits off the primary's centre spot, then centred on it.
Step 3: tilt the primary
Before
The secondary's shadow is off the centre spot
After
Shadow centred on the centre spot
Seen through a collimation cap. Each step moves one part: adjust until the view on the right.

Step 1 - Centre the secondary under the focuser

Point the tube horizontally. Look through the cap. The secondary should appear round and centred in the focuser. If not, adjust the secondary's central bolt (moves it up and down the tube) and rotate it gently. Most telescopes keep this setting for years.

Step 2 - Tilt the secondary towards the primary

Adjust the three small screws on the secondary holder, a quarter-turn at a time, until the reflection of the whole primary mirror is centred in the secondary. With a laser: until the red dot lands on the primary's centre spot.

Step 3 - Tilt the primary

At the bottom of the tube the primary cell has adjustment screws and locking screws. Loosen the locking screws slightly. Adjust the others until the reflection of the secondary (or the returning laser dot) sits in the centre - with a laser, until the dot returns to the centre of the laser's target. Retighten the locking screws gently and check again.

Confirm on a star

Repeat the defocused-star test. Small corrections with the primary screws while looking at the star give the best result.

Good habits

  • Make small turns and check after each one.
  • Never touch the mirror surfaces.
  • Short, fast telescopes (f/5 and below) need more careful collimation than long ones.

If a mirror is loose, a screw is stripped or the view does not improve, request a service check.

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