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17-Phys-A1 Classical Mechanics · May 2016

Question 5 of 6: Torque-Free Rigid-Body Rotation — Euler's Equations After an Impulsive Moment

Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)

Notes on this paper

98-Phys-A1, Classical Mechanics — National Exam, May 2016. 3-hour closed-book exam; FIVE (5) questions constitute a complete paper and only the first five questions as they appear in a candidate's answer book are marked, each of equal value. All six printed questions are solved below as a complete study resource.

Reference texts: Goldstein, Classical Mechanics (3rd ed.) — Lagrangian/Hamiltonian mechanics, constraints, rigid-body rotation (Euler's equations); Hibbeler, Engineering Mechanics: Dynamics (14th ed.) — relative-motion kinematics of rigid bodies, impulse and momentum.

Question 5: Torque-Free Rigid-Body Rotation — Euler's Equations After an Impulsive Moment (20 marks)

Question text not reproduced: the examination questions are © Engineers and Geoscientists BC. Open the official past paper (linked at the top of this page) to read the question, then follow the worked solution below.

Given. A rigid body spinning about its own C.M., described in its principal-axis body frame by Euler's equations of torque-free rotation for $t>0$ (the moment is an instantaneous impulse at $t=0$ only): $$I_{xx}\dot\omega_x=(I_{yy}-I_{zz})\omega_y\omega_z,\quad I_{yy}\dot\omega_y=(I_{zz}-I_{xx})\omega_z\omega_x,\quad I_{zz}\dot\omega_z=(I_{xx}-I_{yy})\omega_x\omega_y.$$ The impulsive moment sets the initial angular velocity via $\Delta\vec L=\vec M_0=\int\vec M\,dt$, i.e.\ $\omega_i(0^+)=M_{0,i}/I_{ii}$.

Find. Qualitative behaviour of $\vec\omega(t)$ for $t>0$ in each of the two inertia cases.

Approach. Compute $\vec\omega(0^+)$ from the impulse, then examine whether that state is a fixed point (steady spin) of the torque-free Euler equations for each inertia distribution, using the two conserved quantities of torque-free motion — kinetic energy $2T=I_{xx}\omega_x^2+I_{yy}\omega_y^2+I_{zz}\omega_z^2$ and angular momentum magnitude $L^2$ — to characterize the resulting motion.

  1. Part (a) — spherical inertia, $I_{xx}=I_{yy}=I_{zz}=I$. The impulse gives $\vec\omega(0^+)=\vec M_0/I=(a/I,b/I,c/I)$. Because all three principal moments are equal, every term $(I_{yy}-I_{zz})$, $(I_{zz}-I_{xx})$, $(I_{xx}-I_{yy})$ in Euler's equations vanishes identically — regardless of the direction of $\vec\omega$. The equations collapse to $I\dot{\vec\omega}=0$, i.e.\ $\vec\omega$ is exactly constant for all $t>0$. The body immediately settles into steady, unchanging rotation about the fixed axis along $\vec M_0=(a,b,c)$, with constant magnitude $|\vec M_0|/I$ — no wobble, no precession. This is because a spherically symmetric inertia tensor treats every axis identically: there is no gyroscopic coupling between components to drive any change, so whatever axis the impulse sets up is automatically a permanent axis of rotation (confirmed: integrating Euler's equations from this initial condition returns $\vec\omega(t)\equiv\vec\omega(0^+)$ to machine precision).
  2. Part (b) — asymmetric (triaxial) inertia, $I_{xx}>I_{yy}>I_{zz}$. The impulse gives $\vec\omega(0^+)=(a/I_{xx},\,0,\,c/I_{zz})$ — zero component along the intermediate-inertia axis $y$, nonzero along both the maximum ($x$) and minimum ($z$) inertia axes. Check whether $\omega_y\equiv 0$ can persist: from the middle Euler equation, $$I_{yy}\dot\omega_y\big|_{t=0^+} = (I_{zz}-I_{xx})\,\omega_z\omega_x\Big|_{t=0^+} = (I_{zz}-I_{xx})\cdot\frac{c}{I_{zz}}\cdot\frac{a}{I_{xx}} \neq 0$$ because $I_{zz}\neq I_{xx}$ and $a,c>0$ are both nonzero by hypothesis. So $\omega_y=0$ is not maintained — the state $(\omega_x,0,\omega_z)$ with both $\omega_x,\omega_z\neq0$ is not an equilibrium of Euler's equations (only the two pure states, spin about $x$ alone or about $z$ alone, are steady). The $y$-component is therefore driven away from zero immediately, while kinetic energy $2T$ and $|\vec L|$ stay exactly conserved (no external torque for $t>0$) — confirmed: $\omega_y$ grows from 0 to a magnitude comparable to $\omega_x(0),\omega_z(0)$ within a few characteristic periods, while $2T$ and $|\vec L|$ drift by less than $10^{-6}$ over that time. The rotation does not settle into steady spin about a fixed axis; it develops a genuine, time-varying $y$-component and nutates/tumbles, tracing a closed (bounded) polhode curve on Poinsot's construction around whichever of the two stable axes ($x$ or $z$) the particular energy/momentum combination favours — qualitatively different from part (a)'s permanently steady rotation, precisely because the gyroscopic coupling terms in Euler's equations no longer vanish when the three principal moments are distinct.
Final results
CaseBehaviour for $t>0$
(a) $I_{xx}=I_{yy}=I_{zz}$$\vec\omega(t)\equiv\vec M_0/I$ — permanently steady rotation, no wobble
(b) $I_{xx}>I_{yy}>I_{zz}$, $\omega_y(0)=0$$\omega_y$ immediately departs from 0; body nutates on a bounded polhode (energy & $|L|$ conserved, not a fixed axis)