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๐ŸŽกAP Physics 1

Newton's Laws of Motion

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Why This Matters

Newton's Laws aren't just three statements you memorize for the examโ€”they're the foundation for everything in mechanics. When you see problems about objects on ramps, cars rounding curves, collisions, or rockets launching, you're really being tested on whether you understand how forces cause (or don't cause) changes in motion. The AP Physics 1 exam loves to probe your conceptual understanding: Can you draw a correct free-body diagram? Do you know which forces form Newton's Third Law pairs? Can you explain why an object accelerates or stays in equilibrium?

These laws connect directly to Unit 2: Force and Translational Dynamics and Unit 4: Linear Momentum, showing up in multiple-choice questions and nearly every mechanics FRQ. You'll need to apply them to inclined planes, circular motion, collisions, and systems of objects. Don't just memorize "F=maF = ma"โ€”know what each law tells you about the relationship between forces and motion, and practice identifying which law applies in different scenarios.


The Three Laws: Foundations of Dynamics

Each of Newton's Laws addresses a different aspect of how forces relate to motionโ€”from what happens when forces are absent, to how forces cause acceleration, to how objects interact with each other.

Newton's First Law (Law of Inertia)

  • An object maintains its velocityโ€”whether at rest or movingโ€”unless a net external force acts on it
  • Inertia is the property that quantifies an object's resistance to changes in motion; more mass means more inertia
  • Zero net force means zero acceleration, not zero motionโ€”a common exam misconception to avoid

Newton's Second Law (F=maF = ma)

  • Net force equals mass times acceleration (ฮฃFโƒ—=maโƒ—\Sigma \vec{F} = m\vec{a})โ€”this is the quantitative heart of dynamics
  • Acceleration is directly proportional to force and inversely proportional to mass; doubling mass halves acceleration for the same force
  • This law defines the newton: 1ย N=1ย kgโ‹…m/s21 \text{ N} = 1 \text{ kg} \cdot \text{m/s}^2, connecting force units to fundamental quantities

Newton's Third Law (Action-Reaction)

  • Forces always come in pairsโ€”if object A pushes on B, then B pushes on A with equal magnitude and opposite direction
  • Third Law pairs act on different objects, so they never cancel each other in a free-body diagram
  • Common exam trap: Normal force and weight are not a Third Law pairโ€”they act on the same object

Compare: First Law vs. Second Lawโ€”both involve net force, but the First Law describes the special case when ฮฃF=0\Sigma F = 0 (constant velocity), while the Second Law handles all cases quantitatively. If an FRQ asks "why does the object move at constant speed," invoke the First Law explicitly.


Analyzing Forces: Tools and Techniques

Before applying Newton's Laws, you need to correctly identify and represent all forces acting on an object. Free-body diagrams are your most important problem-solving tool.

Free-Body Diagrams

  • Show only forces acting ON the objectโ€”never include forces the object exerts on other things
  • Each arrow's direction shows force direction, and length should roughly indicate relative magnitude
  • Start every dynamics problem here; the exam awards points for correct FBDs even if your final answer is wrong

Common Force Types

  • Gravitational force (weight): Fโƒ—g=mgโƒ—\vec{F}_g = m\vec{g}, always points toward Earth's center (straight down near the surface)
  • Normal force: Perpendicular to the contact surface, adjusts magnitude to prevent objects from passing through each other
  • Friction: Opposes relative motion (or attempted motion) between surfaces; fsโ‰คฮผsNf_s \leq \mu_s N for static, fk=ฮผkNf_k = \mu_k N for kinetic
  • Tension: Pulls along a rope or string; for a massless rope, tension is the same throughout

Compare: Static friction vs. kinetic frictionโ€”static friction can vary from zero up to ฮผsN\mu_s N and prevents sliding, while kinetic friction has a fixed value ฮผkN\mu_k N once sliding begins. FRQs often ask you to determine whether an object will slide by comparing applied force to maximum static friction.


Mass, Weight, and Equilibrium

Understanding the distinction between mass and weightโ€”and knowing when forces balanceโ€”is essential for solving statics problems and understanding apparent weight.

Mass vs. Weight

  • Mass (mm) measures the amount of matter in kilograms; it's an intrinsic property that doesn't change with location
  • Weight (Fg=mgF_g = mg) is the gravitational force on an object, measured in newtons
  • Apparent weight equals normal force, which can differ from true weight in accelerating systems (elevators, free fall)

Equilibrium and Net Force

  • Static equilibrium means ฮฃFโƒ—=0\Sigma \vec{F} = 0 and vโƒ—=0\vec{v} = 0; the object is at rest and stays at rest
  • Dynamic equilibrium means ฮฃFโƒ—=0\Sigma \vec{F} = 0 but vโƒ—โ‰ 0\vec{v} \neq 0; the object moves at constant velocity
  • For equilibrium problems, set up equations where forces in each direction sum to zero: ฮฃFx=0\Sigma F_x = 0 and ฮฃFy=0\Sigma F_y = 0

Compare: Mass vs. weightโ€”mass stays constant whether you're on Earth, the Moon, or in orbit, but weight changes with gravitational field strength. If an FRQ mentions an astronaut "feeling weightless," they still have mass; their apparent weight (normal force) is zero because they're in free fall.


Applications: Inclined Planes and Circular Motion

These two scenarios appear constantly on AP Physics 1 because they require you to decompose forces, choose coordinate systems wisely, and apply Newton's Second Law in component form.

Objects on Inclined Planes

  • Tilt your coordinate system so x is parallel to the incline and y is perpendicular; this simplifies force decomposition
  • Weight components: Fg,โˆฅ=mgsinโกฮธF_{g,\parallel} = mg\sin\theta (causes acceleration down the ramp), Fg,โŠฅ=mgcosโกฮธF_{g,\perp} = mg\cos\theta (balanced by normal force)
  • Normal force equals mgcosโกฮธmg\cos\theta on a simple incline, which is less than the object's full weight

Centripetal Force and Circular Motion

  • Centripetal force is not a new forceโ€”it's the net force directed toward the center of the circular path
  • Magnitude: Fc=mv2r=mฯ‰2rF_c = \frac{mv^2}{r} = m\omega^2 r, where vv is tangential speed and rr is radius
  • Identify what provides centripetal force in each scenario: tension (ball on string), friction (car on curve), gravity (satellite in orbit), normal force (loop-the-loop)

Compare: Inclined planes vs. circular motionโ€”both require force decomposition, but inclines use tilted Cartesian coordinates while circular motion uses radial/tangential directions. In both cases, the key is identifying which force components cause acceleration and which balance out.


Momentum and Impulse: Extending Newton's Laws

Newton's Second Law can be rewritten in terms of momentum, revealing the impulse-momentum theorem and conservation principles that dominate Unit 4.

Momentum

  • Momentum is pโƒ—=mvโƒ—\vec{p} = m\vec{v}, a vector quantity measured in kgโ‹…m/s\text{kg} \cdot \text{m/s}
  • Newton's Second Law in momentum form: ฮฃFโƒ—=dpโƒ—dt\Sigma \vec{F} = \frac{d\vec{p}}{dt}; force equals the rate of change of momentum
  • Total momentum is conserved in isolated systems (no external forces), making this essential for collision problems

Impulse

  • Impulse equals change in momentum: Jโƒ—=ฮ”pโƒ—=Fโƒ—avgฮ”t\vec{J} = \Delta \vec{p} = \vec{F}_{avg} \Delta t
  • Impulse-momentum theorem connects force, time, and motion change; longer contact time means smaller average force for the same momentum change
  • Graphically, impulse equals the area under a force vs. time graphโ€”a common AP exam question type

Compare: Momentum vs. impulseโ€”momentum is a state of an object at an instant (p=mvp = mv), while impulse is a process that changes momentum over time (J=Fฮ”tJ = F\Delta t). FRQs often ask you to explain how airbags reduce injury by increasing collision time, thereby reducing force.


Quick Reference Table

ConceptBest Examples
Inertia and First LawObjects at constant velocity, seatbelt necessity, tablecloth trick
F=maF = ma applicationsAccelerating elevators, pushing boxes, rocket thrust
Third Law pairsEarth-object gravity, foot-ground while walking, rocket exhaust
Equilibrium (ฮฃF=0\Sigma F = 0)Hanging signs, objects at rest on surfaces, constant-velocity motion
Inclined plane analysisBlocks on ramps, friction on slopes, component decomposition
Centripetal force sourcesTension (ball on string), friction (car on curve), gravity (orbits)
Impulse-momentumCollisions, catching a ball, airbag physics
Mass vs. weightAstronaut scenarios, elevator problems, different planets

Self-Check Questions

  1. A book sits motionless on a table. Identify the forces acting on the book and explain why the normal force and the book's weight are not a Newton's Third Law pair.

  2. Two objects experience the same net force, but object A has twice the mass of object B. Compare their accelerations and explain your reasoning using Newton's Second Law.

  3. A car rounds a flat curve at constant speed. What force provides the centripetal acceleration, and what would happen if this force suddenly disappeared?

  4. An object slides down a frictionless incline at angle ฮธ\theta. Derive an expression for its acceleration and explain why the acceleration is independent of the object's mass.

  5. Compare and contrast momentum and kinetic energy: Which is conserved in all collisions? Which can be negative? How does each quantity depend on velocity?