Motion and Forces — Quick Reference

Aristotle's Ideas of Motion

  • Natural motion: objects have a proper place (earth, water, air, fire) and strive to reach it; natural motion on Earth is straight, beyond Earth is circular.
  • Violent motion: produced by external pushes or pulls.

Galileo's Concept of Inertia

  • Objects of different weights fall at the same time in the absence of air resistance.
  • A moving object needs no force to keep moving in the absence of friction.
  • Inclined planes show: downward slopes add speed at the same rate for all balls; upward slopes slow them at the same rate; on a frictionless horizontal plane, speed remains constant.
  • Inertia: property of matter to resist changes in motion; depends on mass.
  • Galileo emphasized removing medium/friction to reveal the essence of motion.

The Moving Earth

  • Copernicus proposed Earth moving around the Sun; inertia keeps objects moving with Earth unless acted on.
  • Dropping a rock from rest keeps it moving with Earth's rotation while it falls.
  • In a moving vehicle, a tossed coin lands in your hand (demonstrates inertia).
  • Foucault's pendulum demonstrates Earth's rotation.

Newton's Laws of Motion

  • Model: Motion = Prediction via Cause and Effect; 3 laws.
  • 1st Law: If F_net = 0, velocity is constant (rest or straight-line motion).
  • 2nd Law: Fnet=maF_{net} = ma
  • 3rd Law: Action–reaction pairs are equal and opposite, acting on different objects.

The Net Force and Vectors

  • A force is a push or pull; acts on an object; is a vector with magnitude and direction; two types: contact and long-range.
  • Net force is the vector sum of all forces on an object.
  • Examples: two 5-N pulls in the same direction give a 10-N net; opposite directions cancel to 0.
  • Force vectors are represented by arrows: length = magnitude, direction = direction.
  • Example: a cart pulled 15N15\,\text{N} to the right and 20N20\,\text{N} to the left yields a net of 5N5\,\text{N} to the left.

The Equilibrium Rule

  • For a non-accelerating object: F=0\sum F = 0 (equivalently Fnet=0F_{net} = 0).
  • Example: standing on two scales with weight evenly distributed; each scale reads half your weight.

Mass, Weight, and Inertia

  • Mass: amount of matter; fundamental measure of inertia; independent of gravity.
  • Weight: gravitational force; W=mgW = mg.
  • Mass is the same on Earth and Moon; weight varies with gravity.
  • 1 kilogram ≈ 10N10\,\text{N}; 1 kg ≈ 2.2lb2.2\,\text{lb}; 1 lb ≈ 4.45N4.45\,\text{N}.

Free Fall and Air Resistance

  • Free fall (negligible air): acceleration ≈ g9.8 m/s2g \approx 9.8\ \mathrm{m/s^2}; all objects fall with the same acceleration.
  • Nonfree fall: air resistance depends on speed and frontal area.
  • Terminal velocity: when Fair=WF_{air} = W; net force is zero; velocity becomes constant.
  • Coin and feather: in air, coin lands first; in vacuum, they fall together.

Force and Acceleration

  • Acceleration is proportional to net force: a=Fnetma = \frac{F_{net}}{m}.
  • Greater mass → greater inertia; for the same net force, acceleration is smaller.

Friction

  • Friction depends on materials and contact force; arises from surface roughness and stickiness; opposes motion.

Newton's 3rd Law and Examples

  • For every action there is an equal and opposite reaction; action–reaction pairs act on different objects.
  • Examples: rocket and exhaust; wings deflect air to produce lift.