EARTH–MOON SIMULATION

Why two high tides a day instead of one? Tidal forces raise two symmetric bulges, one facing the Moon and one on the opposite side, and the spinning Earth passes through both. As the Moon nears perigee the tidal range grows, while its phase decides between spring and neap tides: the Sun adds roughly 46% of the Moon's tidal pull, reinforcing or cancelling it. All the while the Moon keeps receding 3.8 cm per year.

▸ Building the spinning Earth & the Moon…
▸ Tidal locking: one face toward Earth
▸ Computing the gravity gradient → two tidal bulges
▸ Adding the Sun: spring & neap tides
▸ Starting the orbit…
▸ Ready — Online. ✅
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Simulation room Earth – Moon

Earth–Moon & Tides
Online
tides · tidal locking
Earth – Moon system
🌍🌕 Tides
top view (Sun–Earth–Moon)
Moon distance—
Moon phase—
Tidal range—
Tidal force—
Tide type—
Tide level (observer)—
Clock & status
0 ngày
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Left-drag = rotate · right-drag = pan · scroll = zoom · click EARTH = tidal geometry
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Tide level & Moon phase over time tide levelphase
About Earth–Moon & Tides

Why two high tides a day instead of one? Tidal forces raise two symmetric bulges, one facing the Moon and one on the opposite side, and the spinning Earth passes through both. As the Moon nears perigee the tidal range grows, while its phase decides between spring and neap tides: the Sun adds roughly 46% of the Moon's tidal pull, reinforcing or cancelling it. All the while the Moon keeps receding 3.8 cm per year.

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