Physics circular motion

Understanding Circular Motion

  • Circular motion involves an object moving in a circular path.

Forces in Circular Motion

  • Normal Force: The force acting on the object from the wall of the track, which keeps it moving in a circular path.
    • The normal force changes the direction of the object's velocity, keeping it pointed inward toward the center of the circle.
    • If the object loses contact with the wall (normal force), it will stop moving in a circle and will not accelerate since there are no forces acting on it horizontally.

Counterintuitive Observations

  • When an object is spun (e.g., a ball on a string) and then released, it appears to fly away in a curved path due to the observer's perspective (rotating frame of reference).
    • From the observer’s perspective, the object moves straight, illustrating how motion can appear different based on the frame of reference.

Forces Acting on a Car at the Top of a Circular Hill

  • Acceleration Direction: When analyzing the forces acting on a car moving at constant speed over the top of a hill, the acceleration must point inward (downward toward the center of the circle).
  • Force Diagram: At the top of the hill:
    • The total force must point down, which includes:
      • Force of gravity pulling down (greater than or equal to the normal force).
      • The normal force from the road, which must be less than the gravitational force since the car is in circular motion.

Newton’s Second Law

  • Understanding that:
    • If acceleration points inward, net force also points inward (toward the center of the circle).
    • Application of Newton's Second Law: $F_{ ext{net}} = m imes a$ where
      • Letting acceleration, $a = rac{v^2}{r}$, we can derive the net force involved in circular motion.

Viewing Forces on a Flat Surface vs. Circular Motion

  • On a flat surface:
    • If an object is moving at a constant speed, there are no forces acting in the horizontal direction.
    • No left/right or upward/downward acceleration happens.
    • Static Friction: Keeps the vehicle from slipping, along with some air resistance.
  • As the car moves over the top of a hill:
    • The velocity changes direction, indicating there is an acceleration involved even though the speed is constant.

Comparative Situations

  • Elevator Example: When an elevator moves up and slows down, the forces acting on a person can illustrate similar principles of acceleration and net forces:
    • Tension vs. force of gravity, where tension is less than gravitational force when decelerating.
    • Feeling lighter or a push up due to differing normal forces and acceleration effects.

Forces on the Car at the Highest Point of the Hill

  • Magnitude of Force of Gravity: Use the formula $F_g = mg$ where:
    • Mass of the car ($m = 1,500 ext{ kg}$) and gravitational acceleration ($g = 9.8 ext{ m/s}^2$).
    • Resulting force of gravity is $F_g = 1,500 ext{ kg} imes 9.8 ext{ m/s}^2 = 14,700 ext{ N}$.
  • Direction of the Net Force: At the top, net force must also point downward:
    • Since acceleration points downward (toward the center of the circle), $F_{ ext{net}} = mb^2/r$ can be utilized to calculate net force downward.
    • Example given: If $ ext{speed} = 20 ext{ m/s}$, radius = 60m, then:
      • $F_{ ext{net}} = 1,500 ext{ kg} imes rac{(20 ext{ m/s})^2}{60m} = 10,000 N$.
      • Therefore, $F_{ ext{net,y}} = -10,000 N$ (as it points downward).

Calculation of Normal Force at the Top of the Hill

  • Total downward force (net force) = 10,000 N down.
  • Force of gravity = 14,700 N down.
  • Using balance of forces:
    • Directional comparison gives the normal force as:
      • $F{ ext{normal}} + 10,000 = 14,700 ightarrow F{ ext{normal}} = 4,700 ext{ N (up)}$.

Summary of Principles

  • For circular motion and problems involving forces, setting one axis toward the center of the circle can simplify calculations and analysis of forces.
  • Recap of fundamental elements:
    • Acceleration points toward center of the circle for circular motion.
    • Use appropriate equations of motion (e.g., $a = rac{v^2}{r}$) to assist in understanding dynamics of circular movements.