⚙️ Physics · Mechanics

Memory tricks for forces and motion

Newton's laws, energy, momentum, rotational kinematics, and fluid mechanics — the foundations of classical mechanics made memorable.

⚙️ Mechanics

Memory Tricks

Proven Mnemonics & Acronyms — fast to learn, hard to forget.

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Newton's Second Law
F = ma
Newton's Second Law
Force equals mass times acceleration — the core of mechanics
Double the force → double the acceleration. Double the mass → half the acceleration. Units: Newtons = kg·m/s². The most-used equation in all of physics.
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🃏 Newton's Second Law
Newton's second law?
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🃏 Answer
F = ma
Double the force → double the acceleration. Double the mass → half the acceleration. Units: Newtons = kg·m/s². The most-used equation in all of physics.
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Law of Inertia
Newton's 1st: objects keep doing what they're doing unless a net force acts
Law of Inertia
An object in motion stays in motion — inertia explained
No net force = no change in motion. Friction is the real-world force that stops things. In space, an object thrown forward travels forever.
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🃏 Law of Inertia
Newton's first law?
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🃏 Answer
Newton's 1st: objects keep doing what they're doing unless a net force acts
No net force = no change in motion. Friction is the real-world force that stops things. In space, an object thrown forward travels forever.
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Action-Reaction Pairs
Newton's 3rd: every action has an equal and opposite reaction
Action-Reaction Pairs
Forces always come in pairs — rockets, swimming, and walking use this
Rocket pushes gas backward → gas pushes rocket forward. You push on a wall → wall pushes back on you equally. The pair acts on different objects.
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🃏 Action-Reaction Pairs
Newton's third law?
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Newton's 3rd: every action has an equal and opposite reaction
Rocket pushes gas backward → gas pushes rocket forward. You push on a wall → wall pushes back on you equally. The pair acts on different objects.
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Energy Formulas
KE = ½mv² PE = mgh
Energy Formulas
Kinetic and potential energy — two formulas every physics student needs cold
KE: kinetic energy. Doubling speed quadruples KE (squared). PE: gravitational potential energy — depends on height. Total mechanical energy = KE + PE (conserved without friction).
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🃏 Energy Formulas
Kinetic and potential energy — the formulas?
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🃏 Answer
KE = ½mv² PE = mgh
KE: kinetic energy. Doubling speed quadruples KE (squared). PE: gravitational potential energy — depends on height. Total mechanical energy = KE + PE (conserved without friction).
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Work Formula
Work = Force × distance × cosθ. Energy is transferred only when force has a component along motion.
Work Formula
Work is done only when force causes displacement in the direction of the force
W = Fd cosθ. If force is perpendicular to motion (θ=90°), no work is done — cos90°=0. Carrying a heavy box horizontally: you do no work on the box (you push up, it moves sideways). Units: Joules = Newton·meters.
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🃏 Work Formula
Work — the formula?
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🃏 Answer
Work = Force × distance × cosθ. Energy is transferred only when force has a component along motion.
W = Fd cosθ. If force is perpendicular to motion (θ=90°), no work is done — cos90°=0. Carrying a heavy box horizontally: you do no work on the box (you push up, it moves sideways). Units: Joules = Newton·meters.
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Conservation of Momentum
Conservation of momentum: m₁v₁ + m₂v₂ = m₁v₁' + m₂v₂' — total momentum unchanged in closed system
Conservation of Momentum
Total momentum before a collision equals total momentum after
Elastic collision: both momentum AND kinetic energy conserved (billiard balls). Inelastic collision: only momentum conserved, KE lost to heat/sound (car crash). Perfectly inelastic: objects stick together, maximum KE lost. Momentum is always conserved in a closed system.
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🃏 Conservation of Momentum
Conservation of momentum — the equation?
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🃏 Answer
Conservation of momentum: m₁v₁ + m₂v₂ = m₁v₁' + m₂v₂' — total momentum unchanged in closed system
Elastic collision: both momentum AND kinetic energy conserved (billiard balls). Inelastic collision: only momentum conserved, KE lost to heat/sound (car crash). Perfectly inelastic: objects stick together, maximum KE lost. Momentum is always conserved in a closed system.
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Centripetal Force
Circular motion: centripetal force = mv²/r, always directed toward center
Centripetal Force
The inward force that keeps objects moving in a circle
Centripetal means 'center-seeking.' For circular motion, a net force must point toward the center. This is NOT a new force — it's provided by existing forces: tension in a string, gravity for orbiting satellites, friction for a car turning. Remove the centripetal force → object flies off in a straight line.
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🃏 Centripetal Force
Centripetal force — formula and direction?
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🃏 Answer
Circular motion: centripetal force = mv²/r, always directed toward center
Centripetal means 'center-seeking.' For circular motion, a net force must point toward the center. This is NOT a new force — it's provided by existing forces: tension in a string, gravity for orbiting satellites, friction for a car turning. Remove the centripetal force → object flies off in a straight line.
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Newton's Law of Gravitation
Gravitational force: F = Gm₁m₂/r². Double distance → force drops to ¼.
Newton's Law of Gravitation
Gravity between any two masses — follows an inverse square law
G = 6.674×10⁻¹¹ N·m²/kg². Force depends on product of masses and inversely on distance squared. Double the distance → (1/2)² = ¼ the force. The same law that makes apples fall also keeps the Moon in orbit.
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🃏 Newton's Law of Gravitation
Newton's law of gravitation — and what doubling the distance does?
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🃏 Answer
Gravitational force: F = Gm₁m₂/r². Double distance → force drops to ¼.
G = 6.674×10⁻¹¹ N·m²/kg². Force depends on product of masses and inversely on distance squared. Double the distance → (1/2)² = ¼ the force. The same law that makes apples fall also keeps the Moon in orbit.
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Simple Harmonic Motion
Simple harmonic motion: restoring force ∝ displacement. Period of pendulum: T = 2π√(L/g)
Simple Harmonic Motion
Oscillating systems where restoring force is proportional to displacement
Examples: pendulum, mass on spring. Restoring force always acts opposite to displacement. Period of simple pendulum T = 2π√(L/g) — depends only on length and gravity, NOT mass or amplitude (for small angles). Period of spring: T = 2π√(m/k) where k = spring constant.
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🃏 Simple Harmonic Motion
Simple harmonic motion — the restoring force, and a pendulum's period?
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🃏 Answer
Simple harmonic motion: restoring force ∝ displacement. Period of pendulum: T = 2π√(L/g)
Examples: pendulum, mass on spring. Restoring force always acts opposite to displacement. Period of simple pendulum T = 2π√(L/g) — depends only on length and gravity, NOT mass or amplitude (for small angles). Period of spring: T = 2π√(m/k) where k = spring constant.
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Projectile Motion
Projectile motion: horizontal and vertical motion are INDEPENDENT. Horizontal: constant. Vertical: gravity.
Projectile Motion
Two independent motions happening simultaneously
Horizontal: constant velocity (no acceleration, ignoring air resistance). Vertical: constant acceleration due to gravity (9.8 m/s² downward). At peak: vertical velocity = 0, horizontal velocity unchanged. Range formula: R = v²sin(2θ)/g. Maximum range at 45°.
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🃏 Projectile Motion
Projectile motion — the key idea?
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🃏 Answer
Projectile motion: horizontal and vertical motion are INDEPENDENT. Horizontal: constant. Vertical: gravity.
Horizontal: constant velocity (no acceleration, ignoring air resistance). Vertical: constant acceleration due to gravity (9.8 m/s² downward). At peak: vertical velocity = 0, horizontal velocity unchanged. Range formula: R = v²sin(2θ)/g. Maximum range at 45°.
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Torque
Torque = Force × lever arm. Clockwise = negative. Counterclockwise = positive.
Torque
The rotational equivalent of force
τ = r × F × sinθ. The longer the lever arm (r), the more torque for the same force. Opening a door: push near the hinges (short lever arm, little torque). Push at the handle (long lever arm, more torque). Torque causes angular acceleration just as force causes linear acceleration.
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🃏 Torque
Torque — formula and sign convention?
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🃏 Answer
Torque = Force × lever arm. Clockwise = negative. Counterclockwise = positive.
τ = r × F × sinθ. The longer the lever arm (r), the more torque for the same force. Opening a door: push near the hinges (short lever arm, little torque). Push at the handle (long lever arm, more torque). Torque causes angular acceleration just as force causes linear acceleration.
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Rotational Kinematics
Every linear equation has a rotational twin — swap x→θ, v→ω, a→α, m→I
Linear to rotational analogy — same equations, different variables
Rotational motion follows identical math to linear motion — just with angular quantities
Linear → Rotational: displacement x → angle θ (radians). Velocity v → angular velocity ω (rad/s). Acceleration a → angular acceleration α (rad/s²). Mass m → moment of inertia I. Force F → torque τ. Newton's 2nd: F=ma → τ=Iα. Kinetic energy: ½mv² → ½Iω². Momentum: p=mv → L=Iω. Rolling without slipping: v_cm = ωr. Moment of inertia depends on mass distribution: solid cylinder = ½mr², hollow cylinder = mr², solid sphere = 2/5 mr².
τ = Iα
Rotational Newton's 2nd — torque = moment of inertia × angular acceleration
L = Iω
Angular momentum — conserved when net torque = 0
Rolling
v = ωr links linear and rotational — both KE terms add
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🃏 Rotational Kinematics
Linear to rotational motion — what swaps for what?
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🃏 Answer
Every linear equation has a rotational twin — swap x→θ, v→ω, a→α, m→I
τ = IαRotational Newton's 2nd — torque = moment of inertia × angular acceleration
L = IωAngular momentum — conserved when net torque = 0
Rollingv = ωr links linear and rotational — both KE terms add
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Friction Forces
STATIC is stronger — object hasn't moved yet. KINETIC is weaker — once sliding.
Static vs kinetic friction — and how to calculate each
Static friction adjusts up to its maximum; kinetic friction is fixed once sliding begins
Static friction: f_s ≤ μ_s × N — adjusts to match applied force until maximum reached. Once object starts moving, switches to kinetic friction: f_k = μ_k × N (constant). Always: μ_s > μ_k (static coefficient larger than kinetic — harder to START sliding than to keep sliding). Normal force N = mg cos θ on an incline. Direction: friction always opposes relative motion (or tendency of motion). Kinetic friction does negative work on the sliding object — converts KE to heat.
Static
Adjustable 0 to μₛN — object not yet moving
Kinetic
Fixed = μₖN — once sliding, always this value
μₛ > μₖ
Always — harder to start moving than to keep moving
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🃏 Friction Forces
Static vs kinetic friction — which is stronger?
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🃏 Answer
STATIC is stronger — object hasn't moved yet. KINETIC is weaker — once sliding.
StaticAdjustable 0 to μₛN — object not yet moving
KineticFixed = μₖN — once sliding, always this value
μₛ > μₖAlways — harder to start moving than to keep moving
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Impulse and Momentum
J = FΔt = Δp — impulse equals change in momentum
Impulse-momentum theorem — force × time changes momentum
A large force for a short time equals a small force for a long time — same impulse, same momentum change
Impulse J = F×Δt = Δp = m×Δv. Units: N·s = kg·m/s. Conservation of momentum: in a closed system, total momentum before = total momentum after. Elastic collision: both momentum AND kinetic energy conserved. Inelastic collision: only momentum conserved, KE lost. Perfectly inelastic: objects stick together — most KE lost. Real applications: airbags increase collision time Δt → reduce force F (same impulse = same momentum change). Crumple zones, catching a ball by pulling your hand back.
Elastic
Momentum AND kinetic energy both conserved
Inelastic
Only momentum conserved — KE converted to heat/deformation
Airbag logic
Larger Δt → smaller F — same impulse, safer stop
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🃏 Impulse and Momentum
Impulse — what does it equal?
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🃏 Answer
J = FΔt = Δp — impulse equals change in momentum
ElasticMomentum AND kinetic energy both conserved
InelasticOnly momentum conserved — KE converted to heat/deformation
Airbag logicLarger Δt → smaller F — same impulse, safer stop
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Fluid Mechanics Essentials
BPAC — Buoyancy, Pressure with depth, Archimedes, Continuity equation
Four core fluid mechanics concepts tested in introductory physics
Fluids follow pressure, buoyancy, and continuity — all connected by density
Pressure with depth: P = P₀ + ρgh — pressure increases linearly with depth. Archimedes' Principle: buoyant force = weight of fluid displaced = ρ_fluid × V_submerged × g. Object floats if ρ_object < ρ_fluid. Continuity equation: A₁v₁ = A₂v₂ — narrower pipe → faster flow (conservation of mass). Bernoulli's equation: P + ½ρv² + ρgh = constant — faster flow → lower pressure (explains lift, venturi effect). Pascal's Principle: pressure applied to enclosed fluid transmitted equally everywhere.
Buoyancy
F_b = ρ_fluid × V_sub × g — weight of displaced fluid
Continuity
A₁v₁ = A₂v₂ — narrow pipe, faster flow
Bernoulli
Faster flow → lower pressure — explains flight and carburetors
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🃏 Fluid Mechanics Essentials
BPAC — the fluid mechanics essentials?
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🃏 Answer
BPAC — Buoyancy, Pressure with depth, Archimedes, Continuity equation
BuoyancyF_b = ρ_fluid × V_sub × g — weight of displaced fluid
ContinuityA₁v₁ = A₂v₂ — narrow pipe, faster flow
BernoulliFaster flow → lower pressure — explains flight and carburetors
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🎓 Common Exam Questions