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🌊 Ocean Waves — The Secret Orbital Motion

🌊 Ocean Waves — The Secret Orbital Motion

Water in a swell doesn't travel — each parcel runs in a circle while the wave shape races on. Watch the orbit shrink with depth, then shallow the water until orbits squash and the wave breaks.

Wave speed
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Regime
deep water
📖 Key facts

A deep-water swell is a partitioned circle dance: each parcel loops forward at the crest, backward in the trough, and barely at all near the seabed — orbit radius decays as e^(−kz), so at depth λ/2 it's ~4% of the surface value. That's why submarines dive to escape storms. The deep-water speed formula is beautifully simple: c = 1.25√λ (λ in metres, c in m/s) — long swells outrun short chop, which is why big clean surf arrives first, hours ahead of the storm that made it.

Run the depth slider down: once depth < λ/2 the orbits flatten into ellipses, speed depends only on depth (c = √(gd)), the front slows before the back → wavelength shrinks, height grows, crest outpaces its base and the wave breaks when depth ≈ 1.3 × wave height. Tsunamis are the extreme shallow case: in 4,000 m ocean they're ordinary-looking waves moving at √(9.81×4000) ≈ 200 m/s — jet speed.

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