The Moon, for real · flyable terrain

Apollo 15 · Hadley Rille

The valley Scott and Irwin drove — the descent stage still there, pinned.

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Where every bump comes fromPROCESSED

LRO NAC stereo DTM, 2 m/px (shown at 2.5 m/px) · product NAC_DTM_APOLLO15_E261N0036 · NASA/GSFC/Arizona State University. Scene 5.1 × 5.1 km, elevation -2,243 m to -1,889 m against the 1,737.4 km lunar reference sphere. Surface color: LROC NAC orthophoto M111571816 (grayscale — this camera's single band). Gaps at the stereo swath's rotated edges are filled by interpolating neighboring measurements; nothing is sculpted.

No generative models anywhere on this page — the pipeline crops, resamples down, and normalizes; it never invents a bump the instrument didn’t measure.

FLY

The other terrains

Olympus Mons

The tallest volcano in the solar system, measured summit to plain.

Valles Marineris

Twelve kilometers floor to rim — a canyon that would cross a continent.

Jezero Delta

The river delta Perseverance is reading, meter by meter.

Tycho Crater

The Moon's freshest great crater — terraced walls and a central peak, laser-measured.

Caloris Basin

A 1,500-kilometer impact scar flooded by lava — Mercury's biggest event, in stereo.

Apollo 17 · Taurus-Littrow

The last valley humans walked, massif to massif — Challenger's spot pinned.

Copernicus Crater

The textbook terraced crater — 93 kilometers of collapse, step by step.

Shackleton Crater

The south pole's shadowed crater, measured by laser in the dark — where Artemis aims.

Rheasilvia Basin

A mountain rivaling Olympus Mons, at the south pole of an asteroid.

Occator Crater

The crater with the famous bright spots — salt where briny water reached vacuum.

Sputnik Planitia

Pluto's nitrogen-ice heart, ringed by water-ice mountains — in stereo from one flyby.

All the terrains →Back to the Atlas of Worlds →