
The Conservation of Angular Momentum is one of the most fundamental principles in rotational mechanics.
It states that if the net external torque acting on a system is zero, the total angular momentum of the system remains constant.
This principle explains phenomena ranging from spinning figure skaters and rotating platforms to planetary motion and galaxies.
Before studying conservation, recall that angular momentum for a rigid body rotating about a fixed axis is:
L=IωL = I\omegaL=Iω
where:
For a particle:
L⃗=r⃗×p⃗\vec{L} = \vec{r} \times \vec{p}L=r×p
where:
p⃗=mv⃗\vec{p}=m\vec{v}p=mv
Angular momentum is a vector quantity.
The rotational form of Newton’s Second Law is:
∑τ=dLdt\sum \tau = \frac{dL}{dt}∑τ=dtdL
This equation states that torque changes angular momentum.
It is analogous to:
∑F=dpdt\sum F = \frac{dp}{dt}∑F=dtdp
in linear motion.
Angular momentum is conserved whenever the net external torque is zero.
∑τexternal=0\sum \tau_{\text{external}} = 0∑τexternal=0
If:
dLdt=0\frac{dL}{dt}=0dtdL=0
then:
L=constantL=\text{constant}L=constant
This is the mathematical statement of angular momentum conservation.
For any isolated rotational system:
Li=LfL_i=L_fLi=Lf
For a rigid body:
Iiωi=IfωfI_i\omega_i = I_f\omega_fIiωi=Ifωf
where:
Angular momentum conservation means that a system cannot spontaneously gain or lose angular momentum.
If the moment of inertia changes, the angular velocity must adjust to keep angular momentum constant.
If:
I↓I\downarrowI↓
then:
ω↑\omega\uparrowω↑
If:
I↑I\uparrowI↑
then:
ω↓\omega\downarrowω↓
A spinning skater pulls their arms inward.
This decreases the moment of inertia.
If<IiI_f<I_iIf<Ii
Since angular momentum is conserved:
Iiωi=IfωfI_i\omega_i = I_f\omega_fIiωi=Ifωf
the angular velocity increases.
The skater spins faster without any external torque.
A person stands on a frictionless rotating platform holding dumbbells.
When the person pulls the dumbbells inward:
When the dumbbells are extended outward:
The total angular momentum remains unchanged.
Planets orbiting the Sun approximately conserve angular momentum.
For orbital motion:
L=mvrL=mvrL=mvr
When a planet moves closer to the Sun:
r↓r\downarrowr↓
its speed increases.
When a planet moves farther away:
r↑r\uparrowr↑
its speed decreases.
This behavior is a direct consequence of angular momentum conservation.
Angular momentum is often conserved during rotational collisions.
If external torque is negligible:
Li=LfL_i=L_fLi=Lf
This principle is especially useful when kinetic energy is not conserved.
Examples include:
A student stands on a frictionless turntable.
Initially:
Ii=8 kg⋅m2I_i = 8\,kg\cdot m^2Ii=8kg⋅m2 ωi=2 rad/s\omega_i = 2\,rad/sωi=2rad/s
The student pulls in their arms, reducing the moment of inertia to:
If=4 kg⋅m2I_f = 4\,kg\cdot m^2If=4kg⋅m2
Find the final angular velocity.
Using conservation of angular momentum:
Iiωi=IfωfI_i\omega_i = I_f\omega_fIiωi=Ifωf
Substitute values:
(8)(2)=(4)ωf(8)(2) = (4)\omega_f(8)(2)=(4)ωf 16=4ωf16 = 4\omega_f16=4ωf ωf=4 rad/s\omega_f = 4\,rad/sωf=4rad/s
The angular velocity doubles.
A common misconception is that conserving angular momentum automatically means conserving kinetic energy.
This is not true.
Angular momentum may remain constant while rotational kinetic energy changes.
For a rotating body:
Krot=12Iω2K_{\text{rot}} = \frac12 I\omega^2Krot=21Iω2
When a skater pulls in their arms:
The extra energy comes from the work done by the skater’s muscles.
For systems containing several interacting objects:
Ltotal,i=Ltotal,fL_{\text{total},i} = L_{\text{total},f}Ltotal,i=Ltotal,f
provided that:
∑τexternal=0\sum \tau_{\text{external}} = 0∑τexternal=0
Internal torques cancel in pairs and do not affect total angular momentum.
Objects moving toward or away from the axis.
Changing body configuration changes moment of inertia.
Orbital speed changes with distance from the central body.
Angular momentum often remains conserved even when kinetic energy does not.
Using conservation of angular momentum when external torque is present.
Always verify:
∑τexternal=0\sum \tau_{\text{external}}=0∑τexternal=0
Confusing angular momentum with rotational kinetic energy.
They are different physical quantities.
Ignoring the change in moment of inertia.
Angular velocity changes whenever the moment of inertia changes.
Identify the system.
Determine whether external torque is negligible.
Write:
Li=LfL_i=L_fLi=Lf
Substitute:
Iiωi=IfωfI_i\omega_i = I_f\omega_fIiωi=Ifωf
for rigid-body problems.
Solve for the unknown variable.
Angular momentum of a rotating rigid body:
L=IωL=I\omegaL=Iω
Rotational Newton’s Second Law:
∑τ=dLdt\sum\tau = \frac{dL}{dt}∑τ=dtdL
Conservation condition:
∑τexternal=0\sum\tau_{\text{external}}=0∑τexternal=0
Conservation equation:
Li=LfL_i=L_fLi=Lf
or
Iiωi=IfωfI_i\omega_i = I_f\omega_fIiωi=Ifωf
Key ideas:
The Conservation of Angular Momentum provides a unifying principle that explains rotational behavior across systems ranging from simple laboratory experiments to planetary and astronomical motion.
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