LIGO (Laser Interferometer Gravitational Wave Observatory) is a scientific facility dedicated to detecting…
| Category | Aerospace & Astronomy |
|---|---|
| Standard size | Custom size |
| Supply | Single unit or batch · OEM to your drawing |
| Lead time | Standard 4–8 weeks after deposit (confirmed per contract) |
| Warranty | 1 year, structure and control |
| Documents | Specification sheet · control diagram · spare-part list |
A standard catalogue model: the dimensions, control package and finish are fixed, which is what keeps the price and the lead time predictable. Size, colour and interface language can be adapted without a new design cycle.
Standard models from this range are also listed in our online store, priced in USD — see the price yourself ↗
LIGO (Laser Interferometer Gravitational Wave Observatory) is a scientific facility dedicated to detecting gravitational waves, capturing spatiotemporal ripples in the universe through laser interferometers.
The unit is designed for unsupervised public use: controls are recessed or shielded, moving parts are enclosed, and the interface is operable by a child of about six with no instruction. Where a screen is used, the language can be switched without changing the hardware, and the content can be replaced on site.
Gravitational waves are a type of matter wave generated by the intense motion and change of matter and energy. LIGO is an international observatory used for detecting gravitational waves. LIGO uses lasers to measure the impact of gravitational waves on two interferometers located far away from Earth. After passing through two interferometers, the laser's rays interfere with each other, resulting in an interference pattern. The core equipment of LIGO is a Michelson laser interferometer. It consists of laser, beam splitter, mirror, and photoelectric cell. By utilizing the interference effect of light waves, gravitational waves cause small changes in arm length that are converted into changes in light intensity measured by phototubes, providing us with the observation data we need.
Every unit leaves the factory after a running test: mechanisms cycled, electronics burned in, edges dressed, fixings torqued and marked. Wear parts — bearings, sliders, lamps, belts, touch panels — are modular and listed on the spare-part sheet, so a venue technician can replace them without returning the exhibit. Crating is plywood with foam blocking; the loading plan and packing list travel with the shipment.
Other models from the Aerospace & Astronomy line, all held to the same specification and the same control package.

A curved screen and twelve seats for a six-minute flight.

Move a planet across the band and watch liquid water survive or boil.

A comet model whose tail always points away from the light source.

Real meteorite samples beside a simulated entry trail.
Attach a theme outline, a floor plan, or nothing at all — a photo of the space is enough to start. Quotations are issued against a real exhibit list, not per-square-metre guesses.
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