Field · Mechanical

Classical Mechanics

Motion, forces, momentum and gravity — hands-on simulations that turn the formulas of classical mechanics into something you can launch, tune, and explore in real time.

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Experiments

23 sims + 1 concept · all systems go
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Projectile Motion

kinematicsgravity

Launch a ball, rocket, comet or dart. Tune velocity, angle, height and gravity, then probe any point of the arc for its exact coordinates.

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Newton's First Law

inertiafriction

Give a puck a push and see it coast. On ice or in space, with no net force, it glides on forever — the law of inertia made plain.

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a = F/m

Newton's Second Law

F = maacceleration

Apply a force to a mass and watch it accelerate. Bigger force, faster pickup; heavier mass, slower — with a live velocity graph.

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Newton's Third Law

action–reactionmomentum

Release two carts on a compressed spring and watch them recoil with equal, opposite forces — the lighter one flying off faster.

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Atwood Machine

pulleytension

Hang two masses over a pulley and watch the heavier one fall gently — a = (m₁−m₂)g/(m₁+m₂). Add pulley mass and the tensions split.

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Double Pendulum

chaosbutterfly effect

One pendulum on the end of another — deterministic rules, wildly unpredictable motion. Turn on the chaos twin and watch them diverge.

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Standing Waves on a String

harmonicsresonance

Clamp a string at both ends and see the harmonics — nodes, antinodes, and how two travelling waves add up to a standing one.

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Projectile with Air Drag

air resistanceterminal velocity

Compare the ideal vacuum parabola with the real, drag-shortened path — lower, shorter, and steeper on the way down.

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The Doppler Effect

soundsonic boom

Move a source and watch its wavefronts bunch ahead and stretch behind — the siren effect, right up to the Mach-cone sonic boom.

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Beats

superpositiontuning

Play two close frequencies and hear the loudness throb at their difference — the effect musicians use to tune by ear.

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Pendulum

oscillationenergy

Swing a bob through small or wide arcs, add damping, and watch the period shift and energy trade between motion and height.

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Mass on a Spring

oscillationSHM

Pull a mass on a spring and release it — explore simple harmonic motion, damping, period, and the kinetic–potential energy exchange.

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Conservation of Energy

energyKE ↔ PE

Release a ball on a hilly track and watch kinetic and potential energy trade while the total stays fixed — until friction turns it to heat.

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Circular Motion

centripetaldynamics

Whirl a mass in a circle to see the inward centripetal force — then cut the string and watch it fly off along the tangent.

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Rolling Without Slipping

rotationmoment of inertia

Roll spheres, discs and hoops down a ramp and race them — which wins depends only on how the mass is distributed, not on size or weight.

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Angular Momentum

conservationrotation

Pull spinning weights inward and watch the platform whirl faster — the skater effect, with L = Iω held constant.

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Orbital Mechanics

gravitationtwo-body

Launch a satellite around a star and shape its orbit — circle, ellipse, or escape — while Kepler's laws play out before you.

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Gravity: Force & Energy

gravitationpotential energy

Two masses attract with F = Gm₁m₂/r². Explore the potential well U(r) and release them to watch energy convert and conserve.

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Concept

Kepler's Three Laws

ellipsesequal areasT²∝a³

One animated visual for each of Kepler's laws — the ellipse and its foci, equal areas in equal times, and the harmonic law.

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Collisions

momentumenergy

Send two bodies at each other and compare elastic, inelastic and perfectly inelastic impacts — watch momentum hold while energy is lost.

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Torque & Levers

equilibriumτ = F·d

Balance a seesaw by trading mass for distance — find the exact spot where m₁d₁ = m₂d₂ and the beam floats level.

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f₀

Driven Oscillator & Resonance

resonanceA(ω)

Push a spring-mass at different rhythms and sweep across the towering resonance peak — the mechanical twin of the RLC circuit.

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θ

Friction on an Incline

static vs kinetictanθ = μs

Tilt the ramp degree by degree until static friction snaps at the critical angle — then watch weaker kinetic friction take over.

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Center of Mass

momentumcollisions

Collide or explode two bodies and watch the gold × of their center of mass sail on in a straight line, untouched by the chaos.

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