The lunar claim archive
Each investigation preserves the interesting observation, identifies the strongest test, and marks the point where evidence ends and inference begins.


Available now
Open the source record, inspect the mechanism, and leave knowing exactly what the test did and did not settle.
01No Earth-based consumer telescope resolves meter-scale hardware. Lunar orbiters can, and the scale difference is measurable.
Inspect the case
02Apollo impacts produced long seismic codas, but strong scattering and low attenuation explain the record without requiring a hollow shell.
Inspect the case
03Visual resemblance is easy to create. A useful version of the claim needs fixed geometry and predictions made in advance.
Inspect the case
04Some flashes are real impacts. A specific report still needs timing, fixed position, signal shape, and independent corroboration.
Inspect the case
05Simultaneous observations from separated locations can test distance, direction, and shadow geometry directly.
Inspect the case
06A simple nearby image conflicts with parallax, occultations, libration, and signal ranging; surviving versions must add a lunar-range physical system.
Inspect the case
07The perceived enlargement is real, but same-scale photographs usually preserve the Moon's horizontal diameter. The full perceptual mechanism remains debated.
Inspect the case
08Short exposures explain missing stars; calibrated reseau marks and shadow geometry require original-frame and 3D checks. Each effect is reproducible without a studio.
Inspect the caseQueued files stay visible so the scope is clear before a conclusion is written.
Field work
Match an observation goal, location, and budget to a practical route. No product is presented as proof.
Build an observation kit