Basics of Earth's motions
Phase 1 · Required course 1 Modules 01–05Module 01 Released
EarthRotation
Earth Rotation
Real-time photorealistic 3D Earth: local time and time zones, circle of illumination, rotation and Coriolis force, tropics and polar circles. Live dashboard for city time differences, day length, and the subsolar point.
Local time
Time zones
Circle of illumination
Coriolis force
Tropics
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Module 02 Released ✓
EarthRevolution
Earth Revolution & Seasons
Elliptical orbit · Obliquity · Equinoxes and solstices · Subsolar-point migration. Adjustable obliquity — drag to 0° to remove the seasons and visualize their cause.
Obliquity
Equinoxes and solstices
Subsolar point
Perihelion and aphelion
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Module 03 Released
Solar noonSolar altitude
Solar Noon Altitude
Geometric intuition for H = 90° − |φ − δ|. Latitude × date → live solar-altitude plot. Demonstrates that the poles do not always have the lowest solar altitude.
H = 90°−|φ−δ|
Latitude effect
Seasonal effect
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Module 04 Released
ShadowDirection and length
Shadow Direction & Length
3D geometric demonstration of L = h/tan(H). At the equator on the March equinox, noon shadow length is zero. In the Southern Hemisphere, noon shadows point due north — challenging the "shadows always point north" misconception.
Shadow-length formula
Shadow direction rules
Northern vs. Southern Hemisphere
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Module 05 Released
SunApparent motion
Apparent Solar Motion
Celestial-dome view: simultaneously displays three arcs (June solstice · equinox · December solstice). Sunrise and sunset azimuths change live with latitude and date.
Sunrise direction
Celestial arcs
Polar-day path
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Atmosphere and oceans
Phase 2 · Required courses 1/2 combined Modules 06–08Module 06 Released
Day and nightChanging duration
Day Length Variation
Latitude–date day-length heatmap. Seasonal changes in polar-day and polar-night coverage within the polar circles. Visualization of cos H₀ = −tan φ·tan δ.
Day-length formula
Polar day and night
Latitude effect
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Module 07 Released
Pressure beltsand wind belts
Pressure Belts & Wind Zones
Planetary wind systems migrate north–south seasonally. Coriolis switch: off, winds cross isobars; on, winds run parallel to isobars — helping explain monsoon formation.
Planetary wind system
Coriolis force
Monsoon
Hadley circulation
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Module 08 Released
GlobalOcean currents
Ocean Currents
Global warm- and cold-current streamlines, with fishing grounds and deserts labeled. Compare the Atlantic and Pacific — demonstrating that gyre patterns are governed by planetary winds rather than topography.
Subtropical gyres
Warm and cold currents
Fishing ground
Climate effects
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Astronomy and space
Phase 3 · University · Competitions Modules 09–12Module 09 Released
EquatorCoordinate system
Equatorial Coordinates
Celestial sphere, equatorial plane, ecliptic plane (angle 23.4°), and definition of the vernal equinox. Animation of the Sun's annual motion along the ecliptic, linking declination to seasons.
Right ascension and declination
Ecliptic
Vernal equinox
Equinoxes and solstices
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Module 10 Released
KeplerThree laws
Kepler's Laws of Orbital Motion
Elliptical orbit with adjustable eccentricity; real-time area sweep; T²∝a³ scatter plot. Speed peaks at perihelion — Earth actually travels faster in late December than in June!
Elliptical orbit
Law of equal areas
T²∝a³
Orbital speed
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Module 11 Released
Solar SystemScale model
Solar System Scale Model
Switch between linear and logarithmic scales. In linear mode, Neptune is at the screen edge and the Earth–Moon distance is almost invisible — a striking demonstration of scale. True relative sizes of the 8 planets.
True scale
Logarithmic scale
Planetary orbits
Asteroid belt
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Module 12 Released
Magnetosphere andsolar wind
Magnetosphere & Solar Wind
Earth's dipole field lines · Solar-wind flow around Earth · Auroral oval. Auroras occur around magnetic latitudes 60-70°, rather than at the geographic poles — illustrating the distinction between magnetic and geographic poles.
Magnetosphere
solar wind
Auroral belt
Magnetic poles
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