How to open and reconfigure a cube
Task-oriented. You need an empty cube, a rotated mirror, or a flipped lens.
Every UC2 cube consists of two halves holding a sliding insert that carries the optics (lens, mirror, sample holder…). Because the halves come apart, one cube can play any role.
You'll typically do this when:
- a build needs an empty cube as a spacer (e.g. the Kepler telescope),
- a mirror or lens must be rotated 90° (e.g. the eyepiece looking upward),
- a lens must be flipped so its curved side faces the right way,
- you want to see how the system works inside — which is the whole point of UC2.
Steps
- Hold the lower half of the cube and pull the upper half straight up. No tools needed for the standard cubes.
- Slide the insert out sideways along its rails. Don't force it; if it sticks, wiggle gently.
- Do what you came for: rotate the insert 90°, flip it, swap it for another one, or leave the cube empty.
- Slide the insert back in until it seats fully, and press the upper half back on until the corners click flush.
cube-open-sequence.jpgTODO (Benedict): a 4-step photo sequence (well-lit, on neutral background): closed cube → halves separated → insert half-way out → insert rotated and re-seated. The old schematic exists in the Didaktikkonzept; real photos beat it.
Getting it right
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Check the optical axis: after reassembly the lens/mirror centre must line up with the cube's face openings. A tilted insert shows up immediately as a shifted or smeared image — which is a great error-hunting exercise, but not what you want mid-experiment.
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Lens orientation matters: for the plano-convex CoreBox lenses the image is sharper when the curved side faces the parallel (collimated) light — towards the distant side. If edge sharpness looks bad, flip the insert.
✏️ TODO — BenedictConfirm and document the intended orientation of each lens insert (50/100/−50 mm) once, with one labelled macro photo per lens. This directly addresses the feedback that "you can't tell which way round a lens is mounted".
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Don't over-squeeze. The halves are designed to hold by friction; forcing them can tilt the insert.
Why the tolerance matters (a 30-second detour)
The insert seats reproducibly to within ~0.1 mm. That's not perfectionism: a lens tilted by a degree or displaced by half a millimetre visibly degrades the image. Professional modular systems (cage systems, Thorlabs-style mounts) fight exactly the same battle with steel rods — UC2 does it with printed rails and magnet/screw kinematics. Letting students feel this tolerance is a feature, not a bug.
Related
- Build a telescope — first build that needs empty cubes
- Parts and parameters — what's inside each module