Engineering Mechanics – Dynamics

🏎️Engineering Mechanics – Dynamics Unit 7 – Energy and Momentum in Rigid Body Dynamics

Energy and momentum in rigid body dynamics explore how objects move and interact. This unit covers key concepts like center of mass, moment of inertia, and angular momentum. It also delves into energy types, conservation laws, and real-world applications. Understanding these principles is crucial for analyzing complex mechanical systems. From vehicle dynamics to robotics, this knowledge forms the foundation for solving engineering problems involving motion, forces, and energy transfer in rigid bodies.

Key Concepts and Definitions

  • Rigid body a solid object where the distance between any two points remains constant, regardless of external forces
  • Center of mass (COM) the point where the total mass of the body can be considered to be concentrated
  • Moment of inertia (MOI) a measure of an object's resistance to rotational acceleration, depends on the object's mass distribution
    • Calculated using the integral I=r2dmI = \int r^2 dm, where rr is the distance from the axis of rotation
  • Angular velocity ω\omega the rate of change of angular displacement, measured in radians per second
  • Angular momentum LL the product of an object's moment of inertia and its angular velocity, L=IωL = I\omega
  • Kinetic energy (KE) the energy an object possesses due to its motion, consists of translational and rotational components
    • Translational KE =12mv2= \frac{1}{2}mv^2, where mm is mass and vv is velocity
    • Rotational KE =12Iω2= \frac{1}{2}I\omega^2, where II is moment of inertia and ω\omega is angular velocity
  • Potential energy (PE) the energy an object possesses due to its position in a force field (gravitational, elastic, etc.)

Rigid Body Motion Basics

  • Rigid body motion involves both translation and rotation
  • Translation occurs when all points in the body move along parallel paths, described by the motion of the COM
  • Rotation occurs when the body spins about an axis, described by angular velocity and acceleration
  • Instantaneous center of rotation (ICR) the point about which a body appears to be rotating at a given instant
  • Pure translation no rotation, all points move with the same velocity and acceleration
  • Pure rotation no translation, the body rotates about a fixed axis
  • General plane motion a combination of translation and rotation in a single plane
  • Degrees of freedom (DOF) the number of independent parameters needed to describe a body's motion (maximum of 6 for a 3D rigid body)

Energy in Rigid Body Systems

  • Total energy the sum of kinetic and potential energy in a system
  • Work-energy principle states that the net work done on a system equals the change in its kinetic energy
    • Wnet=ΔKE=KEfKEiW_{net} = \Delta KE = KE_f - KE_i, where WnetW_{net} is net work, and KEfKE_f and KEiKE_i are final and initial kinetic energy
  • Power the rate at which work is done or energy is transferred, measured in watts (W)
    • P=dWdt=FvP = \frac{dW}{dt} = \vec{F} \cdot \vec{v}, where PP is power, WW is work, tt is time, F\vec{F} is force, and v\vec{v} is velocity
  • Conservative forces (gravity, springs) work done is independent of the path taken and can be stored as potential energy
  • Non-conservative forces (friction, air resistance) work done depends on the path and dissipates energy as heat
  • Mechanical energy the sum of kinetic and potential energy in a system, conserved in the absence of non-conservative forces

Momentum in Rigid Body Dynamics

  • Linear momentum pp the product of an object's mass and velocity, p=mv\vec{p} = m\vec{v}
  • Angular momentum LL the product of an object's moment of inertia and angular velocity, L=Iω\vec{L} = I\vec{\omega}
    • Calculated about a specific point or axis
  • Impulse the product of a force and the time over which it acts, equals the change in linear momentum
    • J=Fdt=Δp=m(vfvi)\vec{J} = \int \vec{F} dt = \Delta \vec{p} = m(\vec{v}_f - \vec{v}_i), where J\vec{J} is impulse, F\vec{F} is force, and vf\vec{v}_f and vi\vec{v}_i are final and initial velocity
  • Angular impulse the product of a torque and the time over which it acts, equals the change in angular momentum
    • H=τdt=ΔL=I(ωfωi)\vec{H} = \int \vec{\tau} dt = \Delta \vec{L} = I(\vec{\omega}_f - \vec{\omega}_i), where H\vec{H} is angular impulse, τ\vec{\tau} is torque, and ωf\vec{\omega}_f and ωi\vec{\omega}_i are final and initial angular velocity
  • Collisions interactions between bodies where forces are large and act over a short time
    • Elastic collisions conserve both kinetic energy and momentum
    • Inelastic collisions conserve momentum but not kinetic energy

Conservation Laws and Principles

  • Conservation of energy energy cannot be created or destroyed, only converted between forms
    • In an isolated system, total energy remains constant
  • Conservation of linear momentum in the absence of external forces, the total linear momentum of a system remains constant
    • pinitial=pfinal\sum \vec{p}_{initial} = \sum \vec{p}_{final}
  • Conservation of angular momentum in the absence of external torques, the total angular momentum of a system remains constant
    • Linitial=Lfinal\sum \vec{L}_{initial} = \sum \vec{L}_{final}
  • Principle of work and energy the change in kinetic energy of a system equals the net work done on it
    • Applies to both translational and rotational motion
  • Parallel axis theorem allows the calculation of moment of inertia about any parallel axis, given the MOI about the COM
    • Iparallel=ICOM+md2I_{parallel} = I_{COM} + md^2, where dd is the distance between the parallel axis and the COM
  • Perpendicular axis theorem relates the moments of inertia about three mutually perpendicular axes
    • For a plane body, Iz=Ix+IyI_z = I_x + I_y, where zz is perpendicular to the xx-yy plane

Equations and Formulas

  • Rotational kinetic energy KErot=12Iω2KE_{rot} = \frac{1}{2}I\omega^2
  • Translational kinetic energy KEtrans=12mv2KE_{trans} = \frac{1}{2}mv^2
  • Gravitational potential energy PE=mghPE = mgh, where hh is the height above a reference level
  • Elastic potential energy PE=12kx2PE = \frac{1}{2}kx^2, where kk is the spring constant and xx is the displacement from equilibrium
  • Power P=FvP = \vec{F} \cdot \vec{v} (translational) or P=τωP = \vec{\tau} \cdot \vec{\omega} (rotational)
  • Linear momentum p=mv\vec{p} = m\vec{v}
  • Angular momentum L=Iω\vec{L} = I\vec{\omega}
  • Impulse-momentum theorem J=Δp\vec{J} = \Delta \vec{p}
  • Angular impulse-momentum theorem H=ΔL\vec{H} = \Delta \vec{L}
  • Parallel axis theorem Iparallel=ICOM+md2I_{parallel} = I_{COM} + md^2
  • Perpendicular axis theorem (for plane bodies) Iz=Ix+IyI_z = I_x + I_y

Real-World Applications

  • Vehicle dynamics analyzing the motion, stability, and control of cars, trucks, and motorcycles
    • Involves considering tire forces, suspension, and weight distribution
  • Robotics designing and controlling the motion of robotic arms, legs, and grippers
    • Requires understanding of joint torques, inertia, and control algorithms
  • Biomechanics studying the forces and motions in living organisms (human gait analysis, prosthetic design)
    • Applies rigid body dynamics principles to biological systems
  • Spacecraft dynamics modeling the attitude control and orbital mechanics of satellites and space vehicles
    • Involves analyzing torques from thrusters, reaction wheels, and environmental disturbances
  • Sports equipment design optimizing the performance of bats, clubs, rackets, and balls
    • Considers the effect of mass distribution and impact dynamics on player performance and equipment durability
  • Wind turbines predicting the loads and power output of wind turbine blades under various operating conditions
    • Requires modeling the coupled aerodynamic and structural dynamics of the blades and tower

Problem-Solving Strategies

  • Identify the system and draw a clear diagram showing all relevant forces, moments, and dimensions
  • Determine the type of motion (pure translation, pure rotation, or general plane motion) and choose appropriate coordinates
  • Isolate the body or system of interest and apply Newton's laws (force/moment balance) in each direction/axis
    • For translation F=ma\sum \vec{F} = m\vec{a}, where a\vec{a} is the acceleration of the COM
    • For rotation M=Iα\sum \vec{M} = I\vec{\alpha}, where α\vec{\alpha} is the angular acceleration about the axis of rotation
  • Use the work-energy principle to relate changes in kinetic and potential energy to the work done by forces
    • Identify conservative and non-conservative forces and calculate the corresponding work
  • Apply conservation of momentum (linear and angular) for systems with no external forces/torques
    • Determine initial and final momenta and solve for unknown velocities or angular velocities
  • Check units, signs, and orders of magnitude to ensure the solution is physically reasonable
  • Verify that the solution satisfies the original equations and constraints


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© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.