Moon Phases Simulator — Sun-Earth-Moon Geometry Interactive

A plan-view Sun-Earth-Moon model paired with an enlarged Earth-facing lunar disk shaded from the same lighting geometry. Includes live charts, equations, guided experiments, a model verification bench and a knowledge-check quiz.

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About the Moon Phases Simulator

A plan-view Sun–Earth–Moon model is paired with an enlarged Earth-facing lunar disk. The disk is shaded from the same lighting geometry as the orbit. New, quarter and full phases result from the viewing angle, not Earth’s shadow.

What the simulator shows

• A real-time 3D scene with 5 inspectable parts (Earth observer, Orbiting Moon, Sunlight direction, Earth-view lunar disk, Viewing direction), with home view, focus-selected-part, auto-rotate, expand, instrument-cover and hide-labels scene tools, plus a model response curve beneath the scene. • Experiment controls: Starting synodic age (0-29 days); Lunar days per animation second (0-2 days/s); Observer orientation (Northern view / Southern view); pause/resume, 0.1 s and 1 s single-step buttons, four playback speeds and a restart button. • Live readouts: Synodic age; Sun–Moon elongation; Visible illuminated fraction; Lunar phase angle; Time to next full phase; Completed cycles. • A Geometry & measurements tab with a parameter-comparison chart, a live-measurements chart, the model equations and snapshot readouts. • An Experiments tab with 3 guided presets (First quarter; Full Moon; Southern orientation) and a Model verification bench that runs independent fresh models, plus a timestamped event log and a copyable trial report. • A Learn & assess tab with guided lessons, a knowledge-check quiz with reset and a written model-scope statement linking to a technical reference.

Model equations

θ=2π age/29.5306, measured from new Moon f=(1−cosθ)/2; phase angle=acos(−cosθ) Visible disk normal n=(x,y,sqrt(1−x²−y²)); brightness=max(0,n·s) s=(sinθ,0,−cosθ); southern view rotates the disk 180°

Model boundaries

Circular coplanar synodic geometry; orbital distance, eccentricity, libration and eclipses are omitted. Apparent sizes and distances are enlarged independently. The hemisphere control is a simplified orientation change, not a full altitude/parallactic-angle sky model.

Frequently asked questions

Are ordinary phases produced by Earth’s shadow?

No. Earth’s shadow produces a lunar eclipse, a separate alignment event.

Does changing observer orientation change illuminated fraction?

No. It rotates the view without changing Sun–Moon–Earth geometry.

What are the model limits of the Moon Phases simulator?

Circular coplanar synodic geometry; orbital distance, eccentricity, libration and eclipses are omitted. Apparent sizes and distances are enlarged independently. The hemisphere control is a simplified orientation change, not a full altitude/parallactic-angle sky model.

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