4.2 Work and Mechanical Energy

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4.2 Work and Mechanical Energy


Key Concepts in Work and Mechanical Energy


Changes in Kinetic Energy

Kinetic energy (KEKE) represents the energy of motion. It depends on an object’s mass and velocity:

KE=12mv2

Where:

  • mm: Mass of the object (kg).
  • vv: Velocity of the object (m/s).

Key Points:

  • Proportional Relationship: Kinetic energy increases with the square of velocity. Doubling velocity quadruples KEKE.
  • External Forces: Changes in KEKE occur when forces like friction, gravity, or collisions act on an object.
  • Formula for Change in Kinetic Energy:

ΔKE=KEfinalKEinitial


Changes in Total Energy

Interactions with external objects or systems can transfer energy, altering a system’s total energy.

  • Work: Transfers energy to or from a system when a force acts over a displacement.
  • Mechanical Energy: Sum of KEKE and potential energy (PEPE).

Forces and Work

The work done on an object depends on:

  1. The force applied.
  2. The displacement of the object.
  3. The angle between the force and displacement vectors.

Work is calculated as:

W=Fdcosθ

Where:

  • FF: Force (N).
  • dd: Displacement (m).
  • θ\theta: Angle between force and displacement.

Types of Energy

Kinetic Energy (KEKE)

Work can increase KEKE, demonstrated by the work-energy principle:

W=ΔKE

Derivation:

For an object of mass mm acted upon by a net force FF over a displacement dd:

  1. Use Newton’s Second Law: F=maF = ma.
  2. Use kinematic equations to relate acceleration and displacement.
  3. Substitute into the work formula to derive ΔKE\Delta KE.

Gravitational Potential Energy (PEgPE_g)

Work done to change an object’s position relative to a reference point increases its gravitational potential energy:

PEg=mgh

Where:

  • mm: Mass of the object (kg).
  • gg: Gravitational acceleration (9.8m/s29.8 \, \text{m/s}^2).
  • hh: Height above the reference point (m).

In gravitational systems beyond Earth, PEgPE_g can also be calculated using:

PEg=Gm1m2r

Where rr is the distance between the two masses’ centers.


Elastic Potential Energy (PEePE_e)

Elastic potential energy is stored in deformable objects like springs. For an ideal spring:

PEe=12kx2

Where:

  • kk: Spring constant (N/m).
  • xx: Displacement from equilibrium (m).

The spring constant can be determined from a plot of force (FsF_s) vs. displacement (xx), where the area under the curve represents the work done.


Thermal Energy

Thermal energy is a catch-all for non-mechanical energy, such as heat or sound:

  • Often arises from friction or collisions.
  • In AP Physics 1, no formal equation is required, but it’s a vital part of energy conservation in systems.

Mechanical Energy Conservation

For a closed system with no non-conservative forces:

KEinitial+PEinitial=KEfinal+PEfinal


Key Takeaways on Energy Types

  1. Kinetic Energy: Motion energy proportional to mass and velocity squared.
  2. Potential Energy:
    • Gravitational: Depends on height and mass.
    • Elastic: Stored in springs or deformable materials.
  3. Thermal Energy: Energy dissipated as heat or sound.
  4. Mechanical Energy: Sum of KEKE and PEPE.

Real-World Applications

  1. Roller Coasters:

    • Convert PEgPE_g at the top of a hill into KEKE as the coaster descends.
  2. Springs:

    • Elastic potential energy powers systems like trampolines or shock absorbers.
  3. Heat from Friction:

    • Tires heating up as they skid due to friction.

Practice Problem

Problem:

A 2 kg object moves at 3 m/s. How much work is required to increase its velocity to 6 m/s?

Solution:

  1. Calculate initial KEKE:

KEinitial=12(2)(3)2=9JKE_{\text{initial}} = \frac{1}{2}(2)(3)^2 = 9 \, \text{J}

  1. Calculate final KEKE:

KEfinal=12(2)(6)2=36JKE_{\text{final}} = \frac{1}{2}(2)(6)^2 = 36 \, \text{J}

  1. Work done (WW):

W=ΔKE=KEfinalKEinitial=369=27JW = \Delta KE = KE_{\text{final}} – KE_{\text{initial}} = 36 – 9 = 27 \, \text{J}


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