Study Notes: Gravity, Free Fall, and Terminal Velocity Review

Historical Theories of Motion and Falling Objects

  • Aristotle's Perspective (50 BC):     * Aristotle posited that heavier objects fall faster than lighter objects.     * He believed that this falling occurred at a constant speed.
  • Galileo's Perspective (1525 AD):     * Galileo challenged the Aristotelian view, suggesting that all objects, regardless of their mass, fall at the same rate of uniform acceleration.     * Experimental results using ticker tape analysis have historically supported Galileo's view of uniform acceleration over Aristotle's view of uniform motion (constant speed).
  • Comparison of Views:     * Aristotle: Heavier objects = Faster fall; Motion = Constant speed.     * Galileo: Different masses dropped from the same height reach the ground at the same time; Motion = Uniform acceleration.

Air Resistance and Drag Force

  • Definition of Air Resistance (Drag Force):     * All objects moving through a fluid, such as air, experience resistance.     * Air possesses mass; when an object encounters enough air mass, its fall is slowed.
  • Relationship with Velocity:     * The faster an object moves through a fluid, the more resistance or drag (FDF_D) it experiences.
  • Impact of Surface Area and Pathing:     * Objects with larger surface areas typically follow very indirect routes to the ground rather than a straight path.     * Increasing an object's surface area generally increases the drag forces acting upon it, which in turn decreases the object's terminal velocity.
  • Aerodynamics and Fluid Density:     * Improving an object's aerodynamics decreases its drag coefficient, thereby increasing its terminal velocity.     * The density of the fluid the object is traveling through also influences its maximum velocity.

Inertia and the Effect of Mass on Gravity

  • Mass and Attraction:     * More mass results in a greater pulling force downward.     * Relationship between mass (mm) and gravitational force (FgravF_{grav}):         * For a mass of 1.0kg1.0\,kg, Fgrav=10NF_{grav} = 10\,N.         * For a mass of 1000kg1000\,kg, Fgrav=10000NF_{grav} = 10000\,N.
  • Inertia:     * Inertia is defined as the ability of an object to resist changes in its motion.     * While heavier objects experience a greater force of gravity, they also possess more mass and thus more inertia, which is the resistance to being moved.

Terminal Velocity

  • Mechanism of Acceleration Decrease:     * As a person or object falls longer, they fall faster.     * Increased speed results in an increased drag force (FDF_D).     * As the drag force increases, the rate of acceleration of the object decreases.
  • Definition of Terminal Velocity:     * Terminal velocity is the maximum velocity an object reaches when its weight due to gravity (FgF_g) is exactly equal to the drag force (FDF_D).     * At this equilibrium point (Fg=FDF_g = F_D), the object stops accelerating and falls at a constant maximum velocity.
  • Example (Human Fall):     * At approximately t=12.0st = 12.0\,s, a falling human reaches terminal velocity at roughly 200km/h200\,km/h.

Free Fall and the Physics of a Vacuum

  • Definition of Free Fall:     * An object is in free fall when the only force acting upon it is gravity.
  • Falling in a Vacuum:     * If air is removed to create a vacuum, there is no air resistance.     * In a vacuum, all objects, regardless of mass, shape, or size, will fall at the exactly same rate.
  • Mathematical Proof of Mass Independence (gg):     * The force of gravity (FgF_g) equals the Universal Gravitational Force (FGF_G).     * Setting the equations equal: mg=GMmd2m g = \frac{G M m}{d^2}.     * The mass of the falling object (mm) appears on both sides of the equation and cancels out.     * Result: g=GMd2g = \frac{G M}{d^2}.     * Conclusion: The acceleration due to gravity (gg) is independent of the mass of the falling object.

Acceleration Due to Gravity (gg)

  • Dual Meaning of "g":     * gg represents both the Gravitational Field Strength (measured in N/kgN/kg, force per unit mass) and the Acceleration Due to Gravity (measured in m/s2m/s^2).
  • Variations by Location on Earth:     * The value of gg varies based on geographic location:         * Equator (sea level): 9.7805m/s29.7805\,m/s^2         * Mount Everest (8.8km8.8\,km peak): 9.7647m/s29.7647\,m/s^2         * Toronto: 9.8049m/s29.8049\,m/s^2         * North Pole (sea level): 9.8322m/s29.8322\,m/s^2
  • Standard Class Convention:     * For the purposes of this course, for objects near Earth, g=9.81m/s2[Down]g = 9.81\,m/s^2\, \text{[Down]}.     * Because gravity is constant near Earth's surface, the 5 uniform acceleration equations from kinematics are applicable.
  • Kinematics Calculation (Experiment Results):     * To find acceleration (aa), use the formula: Δd=viΔt+12aΔt2\Delta d = v_i \Delta t + \frac{1}{2} a \Delta t^2.     * Variables commonly used: vi=0v_i = 0, Δd=4.90m\Delta d = 4.90\,m, time (Δt\Delta t) based on average experimental measurement.