Natural satellite

The Moon

Dark seas, bright highlands and a record of impacts

The Moon, photographed through a small telescope
580 × 580 px
The Moon, photographed through a small telescope
Scroll or pinch to zoom · drag to move
Captured
25 September 2026

1 of 2: 25 September · enhanced colour

What is it?

Earth’s natural satellite. Unlike the faint nebulae, the Moon is bright because it reflects sunlight and is comparatively close.

What can you see?

The dark areas are maria — ancient volcanic plains, not liquid seas. Brighter highlands carry many craters. Bright streaks around some impacts are rays of ejected material.

Why do the two dates look different?

The Sun’s angle changes as the Moon moves around Earth. Low sunlight makes shadows and relief stand out near the day–night boundary. Processing also affects sharpness and colour; these two finished images are not a controlled experiment.

The main view has enhanced colour. It can emphasise subtle differences across the surface, but it is not how the Moon normally appears to an eye.

Behind the photo · optional experiment

Move the sunlight, change the Moon

Take control of the Sun’s direction. Watch the day–night boundary sweep across a textured globe while the Moon itself stays whole.

Journey illustration · not a photograph
Change something. See why.

Move the sunlight

This experiment changes the physics or the viewpoint. Your photograph stays as the reference observation.

Open the full Lab view ↗
Sources & further reading

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