Concept 3 Notes - Newton's Laws

Newton's Laws

Concept: It's not Rocket Science


Force

  • Definition: A push or pull one object exerts on another.

    • Measured in Newtons (1 N = 1 kg*m/s²)

    • Forces can change an object’s motion.

    • Multiple forces can act on an object simultaneously.

  • Net Force: Combination of forces acting on an object.

    • Example: F = 2 N, F = 5 N

    • Net Force = 3 N to the left


Balanced and Unbalanced Forces

  • Balanced Forces: Equal in size, opposite in direction, resulting in a net force of 0.

    • Example: F = 4 N, F = 4 N → Net Force = 0 N

  • Unbalanced Forces: Not equal, causing motion in the direction of the larger force.

    • Example: F = 2 N, F = 3 N → Net Force = 6 N to the right


Newton’s 1st Law of Motion

  • Definition: An object will continue at constant velocity unless a net force acts on it.

    • Objects in motion remain in motion; objects at rest remain at rest.

  • Also known as the Law of Inertia.

    • Example: Slamming brakes causes body to lurch forward due to inertia.

    • Inertia: Resistance to change in motion; more mass = more inertia.


Forces Changing Motion

  • Friction: Resistance when two objects contact.

  • Air Resistance: Resistance an object experiences moving through air.

  • Gravity: Attraction between two masses, pulling objects towards Earth.


Factors Affecting Friction

  • Surface Roughness: Rougher surfaces increase friction due to more microwelds.

  • Normal Force: Greater force pushing together increases friction.

  • Surface Area: Increased contact area increases friction.


Types of Friction

  • Static Friction: Between surfaces not moving past each other.

  • Sliding Friction: Between surfaces sliding past each other.

  • Rolling Friction: Between a rolling object and the surface.


Air Resistance (Drag)

  • Determined by:

    • Speed: Greater speed increases resistance.

    • Size: Larger object increases resistance.

    • Shape: Flatter objects increase resistance.


Law of Universal Gravitation

  • Masses exert an attractive force on each other.

    • Depends on:

      • Mass: Greater mass = greater attraction.

      • Distance: Closer distance = greater attraction.


Gravity

  • Causes all falling objects to accelerate at 9.8 m/s², regardless of mass (ignoring air resistance).


Terminal Velocity

  • Maximum velocity a falling object can reach when gravity and air resistance balance each other.

    • Net force = 0, thus no acceleration.

    • Example: Terminal velocity of humans is approximately 55 m/s.


Newton’s 2nd Law of Motion

  • Definition: Net force causes an object to accelerate in the direction of the force.

    • Greater mass requires greater force to accelerate.

    • Greater net force results in greater acceleration.

  • Formula: F = ma


Example Calculations

  • If pushing a sled with a force of 40 N, and mass is 80 kg:

    • F = 40 N, m = 80 kg

    • Acceleration (a) = F/m = 0.5 m/s²


Weight

  • Definition: Force of gravity on an object.

    • Calculated using F = ma, with a = 9.8 m/s² for gravity.

  • Example Calculation:

    • Mass = 42 kg → Weight = (42)(9.8) = 411.6 N


Weight vs. Mass

  • Mass: Amount of matter in an object, constant regardless of location.

  • Weight: Changes based on gravitational pull; lower on moons, higher on larger planets.


Newton’s 3rd Law of Motion

  • Definition: Every action has an equal and opposite reaction.

    • Example: Jumping on a trampoline; the trampoline exerts equal force in opposite direction.


Law of Conservation of Momentum

  • Definition: Momentum (p) is the mass in motion; transferred in collisions.

    • Formula: p = mv (p = momentum, m = mass, v = velocity).


Example Calculations of Momentum

  • Car with mass of 1300 kg at 28 m/s has momentum:

    • p = (1300 kg)(28 m/s) = 36,400 kg*m/s.


Conservation of Momentum in Collisions

  • Momentum is conserved; transferred between colliding objects.


Example Collision Calculation

  • Ball #1 (11 m/s) collides with Ball #2 (0.17 kg) at 9 m/s:

    • Calculate mass of Ball #1 using conservation of momentum.

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