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Energy and Momentum of Rotating Systems

AP Physics 1 · Topic 6

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7:54

Energy and Momentum of Rotating Systems

Watch a skater spinning with her arms stretched out. She pulls them in — and suddenly she spins much faster. Nobody pushed her. No motor started. So where did…

English narration · English + 中文 subtitles burned in

6.1

Rotational Kinetic Energy

Syllabus
Learning ObjectiveEssential Knowledge

6.1.A
Describe the rotational kinetic energy of a rigid system in terms of the rotational inertia and angular velocity of that rigid system.

  • 6.1.A.1 The rotational kinetic energy of an object or rigid system is related to the rotational inertia and angular velocity of the rigid system and is given by the equation $K = \frac{1}{2} I \omega^2$.
    • 6.1.A.1.i The rotational inertia of an object about a fixed axis can be used to show that the rotational kinetic energy of that object is equivalent to its translational kinetic energy, which is its total kinetic energy.
    • 6.1.A.1.ii The total kinetic energy of a rigid system is the sum of its rotational kinetic energy due to its rotation about its center of mass and the translational kinetic energy due to the linear motion of its center of mass.
  • 6.1.A.2 A rigid system can have rotational kinetic energy while its center of mass is at rest due to the individual points within the rigid system having linear speed and, therefore, kinetic energy.
  • 6.1.A.3 Rotational kinetic energy is a scalar quantity.

Source: College Board AP Course and Exam Description

Roll a full can of soup and an empty can down the same slope, side by side. One reaches the bottom clearly first. Which one, and why, is the kind of question this unit answers with energy and angular momentum, not with forces.

A spinning object has rotational kinetic energy 转动动能, the rotational twin of $\tfrac12 mv^2$:

$$K_{\text{rot}}=\tfrac{1}{2}I\omega^2.$$
An object that both moves and spins (like a rolling ball) has both translational kinetic energy 平动动能 and rotational kinetic energy, and its total is $K=\tfrac12 mv^2+\tfrac12 I\omega^2$, with $v$ the centre-of-mass 质心 speed and $I$ measured about the centre of mass.

Three facts follow from this formula.

  • A spinning object can have kinetic energy while its center is at rest. A flywheel on a fixed axle does not go anywhere, but every point on it moves, so it stores energy.
  • $\tfrac12I\omega^2$ is not a new kind of energy. Add up $\tfrac12mv^2$ for every small piece of the object, with $v=r\omega$, and you get $\tfrac12\left(\sum mr^2\right)\omega^2=\tfrac12I\omega^2$.
  • Like all energy, rotational kinetic energy is a scalar: it has no direction.

Worked example (a rod swinging down). A rod with a sphere on its end has mass $M$ and length $L$, and its center of mass is $\tfrac34L$ from the axle. It is balanced pointing straight up, tapped, and swings down to point straight down. The center of mass falls from $\tfrac34L$ above the axle to $\tfrac34L$ below it, a drop of $\tfrac32L$, so the rod–sphere–Earth system gains

$$\Delta K=Mg\left(\tfrac32L\right)=\tfrac32MgL.$$
The rotational kinetic energy is greatest at the bottom, where the center of mass is lowest. If the Earth is not in the system, the answer is the same, but the reason changes: gravity is then an outside force that does positive work on the rod as its center of mass moves down.

Explore

Spin stores energy

Change how fast the angle sweeps to feel how spin rate feeds the rotational kinetic energy.

Vocabulary Train
English
rotational kinetic energy/rəʊˈteɪʃənl kɪˈnetɪk ˈenədʒi/
translational kinetic energy/trænˈsleɪʃənl kɪˈnetɪk ˈenədʒi/
centre-of-mass
6.2

Torque and Work

Syllabus
Learning ObjectiveEssential Knowledge

6.2.A
Describe the work done on a rigid system by a given torque or collection of torques.

  • 6.2.A.1 A torque can transfer energy into or out of an object or rigid system if the torque is exerted over an angular displacement.
  • 6.2.A.2 The amount of work done on a rigid system by a torque is related to the magnitude of that torque and the angular displacement through which the rigid system rotates during the interval in which that torque is exerted.
    • Equation: $W = \tau \Delta\theta$
  • 6.2.A.3 Work done on a rigid system by a given torque can be found from the area under the curve of a graph of torque as a function of angular position.

Source: College Board AP Course and Exam Description

A torque acting through an angular displacement does work 功, changing rotational kinetic energy:

$$W=\tau\,\Delta\theta,\qquad P=\tau\omega.$$
This is the rotational form of $W=Fd$ and $P=Fv$, and it extends the work–energy theorem 动能定理 to rotation.

Worked example. A motor applies a steady torque of $8.0\ \text{N m}$ to a flywheel 飞轮 while it turns through $10\ \text{rad}$. The work done is $W=\tau\,\Delta\theta=8.0\times10=80\ \text{J}$, and if the flywheel started from rest this all becomes rotational kinetic energy.

If the torque changes as the object turns, the work is the area under a graph of torque against angular position, just as linear work is the area under a force–position graph.

Worked example (pulling a string off a toy). A string of length $\ell_0$ is wrapped round the axle of a toy with rotational inertia $I_X$. A constant force $F_0$ pulls the string until it comes off. The force acts through a distance $\ell_0$, so it does work $F_0\ell_0$, and all of it becomes rotational kinetic energy:

$$F_0\ell_0=\tfrac12I_X\omega_X^2\;\Rightarrow\;\omega_X=\sqrt{\frac{2F_0\ell_0}{I_X}}.$$
A second toy with half the rotational inertia receives the same work, so it gets the same kinetic energy. With a smaller $I$, it needs a larger $\omega$ to hold that energy: $\omega_Y=\sqrt2\,\omega_X$.

Explore

Balance torques on a seesaw

Torque is force times perpendicular distance, $\tau = Fd$. The beam balances when the torques on each side are equal — move the forces and distances to find the balance point.

Vocabulary Train
English
work/wɜːk/
work–energy theorem/wɜːk ˈenədʒi ˈθɪərəm/
flywheel
6.3

Angular Momentum and Angular Impulse

Syllabus
Learning ObjectiveEssential Knowledge

6.3.A
Describe the angular momentum of an object or rigid system.

  • 6.3.A.1 The magnitude of the angular momentum of a rigid system about a specific axis can be described with the equation $L = I\omega$.
  • 6.3.A.2 The magnitude of the angular momentum of an object about a given point is $L = rmv \sin\theta$.
    • 6.3.A.2.i The selection of the axis about which an object is considered to rotate influences the determination of the angular momentum of that object.
    • 6.3.A.2.ii The measured angular momentum of an object traveling in a straight line depends on the distance between the reference point and the object, the mass of the object, the speed of the object, and the angle between the radial distance and the velocity of the object.

6.3.B
Describe the angular impulse delivered to an object or rigid system by a torque.

  • 6.3.B.1 Angular impulse is defined as the product of the torque exerted on an object or rigid system and the time interval during which the torque is exerted.
    • Equation: $\text{angular impulse} = \tau \Delta t$
  • 6.3.B.2 Angular impulse has the same direction as the torque exerted on the object or system.
  • 6.3.B.3 The angular impulse delivered to an object or rigid system by a torque can be found from the area under the curve of a graph of the torque as a function of time.

6.3.C
Relate the change in angular momentum of an object or rigid system to the angular impulse given to that object or rigid system.

  • 6.3.C.1 The magnitude of the change in angular momentum can be described by comparing the magnitudes of the final and initial angular momenta of the object or rigid system: $\Delta L = L - L_0$
  • 6.3.C.2 A rotational form of the impulse–momentum theorem relates the angular impulse delivered to an object or rigid system and the change in angular momentum of that object or rigid system.
    • 6.3.C.2.i The angular impulse exerted on an object or rigid system is equal to the change in angular momentum of that object or rigid system.
      • Equation: $\Delta L = \tau \Delta t$
    • 6.3.C.2.ii The rotational form of the impulse–momentum theorem is a direct result of the rotational form of Newton's second law of motion for cases in which rotational inertia is constant: $\tau_{\text{net}} = \dfrac{\Delta L}{\Delta t} = I \dfrac{\Delta\omega}{\Delta t} = I\alpha$
  • 6.3.C.3 The net torque exerted on an object is equal to the slope of the graph of the angular momentum of an object as a function of time.
  • 6.3.C.4 The angular impulse delivered to an object is equal to the area under the curve of a graph of the net external torque exerted on an object as a function of time.

Boundary statement: While AP Physics 1 expects that students can mathematically manipulate the magnitude of angular momentum using one-dimensional vector conventions, the direction of angular momentum and angular impulse is beyond the scope of the course.

Source: College Board AP Course and Exam Description

Angular momentum 角动量 describes rotational motion. For a rigid body 刚体 rotating about a fixed principal axis, its component along that axis is:

$$L=I\omega.$$
A net torque acting over time delivers an angular impulse 角冲量 that changes it: $\tau_{\text{avg}}\,\Delta t=\Delta L$ – the rotational impulse–momentum theorem 冲量–动量定理.

Worked example (angular impulse). A motor applies a torque of $0.50\ \text{N m}$ for $4.0\ \text{s}$ to a wheel with $I=0.20\ \text{kg m}^2$, starting from rest. The angular impulse is $\tau\,\Delta t=2.0\ \text{kg m}^2/\text{s}$, so $\omega=\Delta L/I=2.0/0.20=10\ \text{rad/s}$.

The graph rules match the linear ones from the momentum unit. The angular impulse is the area under a graph of torque against time, and the net torque is the slope of a graph of angular momentum against time. For a fixed $I$, $\tau_{\text{net}}=\dfrac{\Delta L}{\Delta t}=I\dfrac{\Delta\omega}{\Delta t}=I\alpha$: the rotational form of Newton's second law.

Same angular momentum, different energy. A solid disk and a hoop of the same mass $M$ and radius $R$ are each turned by a string pulled with the same force $F_A$ for the same time $\Delta t$. Each receives the same angular impulse $F_AR\,\Delta t$, so each gains the same angular momentum $L$. But $K=\dfrac{L^2}{2I}$, and the disk has the smaller rotational inertia, so it gains more kinetic energy. In terms of work: the disk spins up faster, so its string is pulled through a longer distance in the same time, and the same force does more work on it.

A single small object moving in a straight line also has angular momentum about a chosen point: $L=mvr_\perp$, where $r_\perp$ is the perpendicular distance from the point to its line of motion. This is what lets a moving object set something spinning.

More generally, $L=rmv\sin\theta$, where $\theta$ is the angle between $\vec r$ (from the point to the object) and $\vec v$. The value depends on which point you choose. An object moving in a straight line at constant speed has constant angular momentum about any fixed point, because $r\sin\theta=r_\perp$ stays the same as it passes.

Explore

Spin carries angular momentum

Change the spin to feel how angular momentum L = Iω builds with faster rotation.

Vocabulary Train
English
Angular momentum/ˈæŋɡjʊlə məʊˈmentəm/
rigid body/ˈrɪdʒɪd ˈbɒdi/
angular impulse/ˈæŋɡjʊlə ˈɪmpʌls/
impulse–momentum theorem/ˈɪmpʌls məʊˈmentəm ˈθɪərəm/
6.4

Conservation of Angular Momentum

Syllabus
Learning ObjectiveEssential Knowledge

6.4.A
Describe the behavior of a system using conservation of angular momentum.

  • 6.4.A.1 The total angular momentum of a system about a rotational axis is the sum of the angular momenta of the system's constituent parts about that axis.
  • 6.4.A.2 Any change to a system's angular momentum must be due to an interaction between the system and its surroundings.
    • 6.4.A.2.i The angular impulse exerted by one object or system on a second object or system is equal and opposite to the angular impulse exerted by the second object or system on the first. This is a direct result of Newton's third law.
    • 6.4.A.2.ii A system may be selected so that the total angular momentum of that system is constant.
    • 6.4.A.2.iii The angular speed of a nonrigid system may change without the angular momentum of the system changing if the system changes shape by moving mass closer to or further from the rotational axis.
    • 6.4.A.2.iv If the total angular momentum of a system changes, that change will be equivalent to the angular impulse exerted on the system.

6.4.B
Describe how the selection of a system determines whether the angular momentum of that system changes.

  • 6.4.B.1 Angular momentum is conserved in all interactions.
  • 6.4.B.2 If the net external torque exerted on a selected object or rigid system is zero, the total angular momentum of that system is constant.
  • 6.4.B.3 If the net external torque exerted on a selected object or rigid system is nonzero, angular momentum is transferred between the system and the environment.

Source: College Board AP Course and Exam Description

If the net external torque 合外力矩 on a system is zero, its total angular momentum is conserved 守恒:

$$I_1\omega_1=I_2\omega_2.$$
So if $I$ decreases, $\omega$ increases to keep $L$ constant – this is why a spinning skater speeds up when pulling their arms in. It applies to collisions 碰撞 and explosions 爆炸 of rotating systems too.

Worked example. A skater spins at $2.0\ \text{rev/s}$ with rotational inertia $I_1=4.0\ \text{kg m}^2$. She pulls her arms in, dropping her rotational inertia to $I_2=1.6\ \text{kg m}^2$. With no external torque, angular momentum is conserved:

$$\omega_2=\frac{I_1}{I_2}\,\omega_1=\frac{4.0}{1.6}\times2.0=5.0\ \text{rev/s}.$$
Her kinetic energy actually rises – the extra energy comes from the work her muscles do pulling her arms in against the outward pull.

The skater is a nonrigid system: she changes shape. Her angular speed changes although her angular momentum does not, because she moves mass closer to the axis. Only an outside torque can change the angular momentum of a system. Inside it, the angular impulses are equal and opposite (Newton's third law), so they cancel.

Check it with numbers. Writing $K=\dfrac{L^2}{2I}$, kinetic energy is inversely proportional 成反比 to $I$ when $L$ is fixed. Before: $\tfrac12(4.0)(4.0\pi)^2=316\ \text{J}$. After: $\tfrac12(1.6)(10\pi)^2=790\ \text{J}$, which is $2.5$ times as much, the same factor by which $I$ fell.

Worked example (a collision that starts a spin). A uniform rod of mass $1.2\ \text{kg}$ and length $0.80\ \text{m}$ hangs from a pivot at its top end, at rest. A $0.10\ \text{kg}$ lump of clay moving horizontally at $5.0\ \text{m/s}$ hits the bottom end and sticks. Find the angular velocity just after.

  • About the pivot, gravity and the pivot force exert no torque during the brief collision, so angular momentum is conserved.
  • Before: only the clay, $L=mvr=(0.10)(5.0)(0.80)=0.40\ \text{kg m}^2/\text{s}$.
  • After: $I=\tfrac13(1.2)(0.80)^2+(0.10)(0.80)^2=0.256+0.064=0.320\ \text{kg m}^2$.
  • $\omega=L/I=0.40/0.320=1.25\ \text{rad/s}$.

Linear momentum is not conserved here: the pivot pushes on the rod during the collision. Angular momentum about the pivot is, because that push passes through the pivot and has no torque.

Where should it hit, and does bouncing help? A disk of mass $m$ slides at $v_0$ and sticks to a rod pivoted at one end, a distance $x$ from the pivot. Its angular momentum about the pivot is $mv_0x$, so hitting farther from the pivot gives the rod more angular momentum, and more spin. Conservation gives

$$mv_0x=\left(I+mx^2\right)\omega\;\Rightarrow\;\omega=\frac{mv_0x}{I+mx^2}.$$
If the disk bounces back instead of sticking, its angular momentum changes from $+mv_0x$ to a negative value. That is a larger change, so by the third law the rod receives a larger angular impulse and spins faster than when the disk sticks.

Pulling mass inward lowers I, so ω rises to conserve L = Iω
Pulling mass inward lowers I, so ω rises to conserve L = Iω
Vocabulary Train
English
net external torque
conserved/kənˈsɜːvd/
collisions/kəˈlɪʒnz/
explosions/ekˈspləʊʒnz/
inversely proportional/ɪnˈvɜːsli prəˈpɔːʃənl/
6.5

Rolling

Syllabus
Learning ObjectiveEssential Knowledge

6.5.A
Describe the kinetic energy of a system that has translational and rotational motion.

  • 6.5.A.1 The total kinetic energy of a system is the sum of the system's translational and rotational kinetic energies.
    • Equation: $K_{\text{tot}} = K_{\text{trans}} + K_{\text{rot}}$

6.5.B
Describe the motion of a system that is rolling without slipping.

  • 6.5.B.1 While rolling without slipping, the translational motion of a system's center of mass is related to the rotational motion of the system itself with the equations:
    • Equation: $\Delta x_{\text{cm}} = r\Delta\theta$
    • Equation: $v_{\text{cm}} = r\omega$
    • Equation: $a_{\text{cm}} = r\alpha$
  • 6.5.B.2 For ideal cases, rolling without slipping implies that the frictional force does not dissipate any energy from the rolling system.

6.5.C
Describe the motion of a system that is rolling while slipping.

  • 6.5.C.1 When slipping, the motion of a system's center of mass and the system's rotational motion cannot be directly related.
  • 6.5.C.2 When a rotating system is slipping relative to another surface, the point of application of the force of kinetic friction exerted on the system moves with respect to the surface, so the force of kinetic friction will dissipate energy from the system.

Boundary statement: Rolling friction is beyond the scope of AP Physics 1.

Boundary statement: The precise mathematical relationships between linear and angular quantities while a rigid body is rolling while slipping are beyond the scope of AP Physics 1 and 2, and students will not be expected to model those relationships quantitatively. However, students are expected to qualitatively explain the changes to linear and angular quantities while a rigid body is rolling while slipping.

Source: College Board AP Course and Exam Description

Rolling without slipping 纯滚动 links the translational and rotational motions: the contact point 接触点 is momentarily at rest, so

$$v=r\omega \qquad\text{and}\qquad a=r\alpha.$$
A rolling object's energy splits between translation and rotation, so on an incline 斜面 it accelerates more slowly than a frictionless sliding object – some energy goes into spin.

Worked example. For a solid disk ($I=\tfrac12 mR^2$) that rolls without slipping, what fraction of its kinetic energy is rotational? Using $v=R\omega$, the rotational part is $\tfrac12 I\omega^2=\tfrac12(\tfrac12 mR^2)\omega^2=\tfrac14 mv^2$, while the translational part is $\tfrac12 mv^2$. So the total is $\tfrac34 mv^2$ and the rotational share is $\tfrac{1/4}{3/4}=\tfrac13$. A hoop, with its mass farther out, stores half its energy in spin and rolls down a ramp even more slowly.

Friction in rolling. When an object rolls without slipping, the contact point is at rest for an instant, so static friction acts at a point that does not move: ideally it does no work and takes no energy from the system. Its job is to provide the torque that makes the object spin. When an object slips (skids), $v\ne r\omega$, the contact point slides over the surface, and kinetic friction turns some kinetic energy into thermal energy.

Worked example (a sphere pushed through its center). A plunger pushes a sphere with a force aimed at its center, from A to B, on a frictionless floor. The sphere then crosses a frictionless stretch B to C, a rough patch C to D, and a frictionless stretch D to E. Where does its angular velocity change?

  • A to B: the push passes through the center, so it has no torque. The sphere slides without spinning.
  • B to C: no horizontal force at all, so nothing changes.
  • C to D: kinetic friction at the bottom acts backward, and it has a torque about the center. The sphere slows down and starts to spin. This is the only place $\omega$ changes.
  • D to E: no friction again, so $v$ and $\omega$ both stay constant.

Wheel against block on a ramp. A wheel rolls down a ramp, with static friction equal to $40\%$ of the gravity component along the slope. Newton's second law along the slope gives $Ma=Mg\sin\theta-0.4\,Mg\sin\theta$, so $a=0.6\,g\sin\theta$. A block sliding down a frictionless ramp of the same angle reaches the bottom faster. In terms of forces: the net force down the slope is larger on the block. In terms of energy: the wheel's $Mgh$ is shared between translation and rotation, while all of the block's goes into translation.

A rolling cylinder and a block on a rough ramp can reach the bottom with the same speed. The cylinder puts part of its energy into spinning; the block loses part of its energy as thermal energy through kinetic friction. If those two parts are equal, the translational kinetic energy at the bottom is the same.

In rolling without slipping the contact point is at rest, so v = rω
In rolling without slipping the contact point is at rest, so v = rω

Energy graphs for a block turning a wheel. A block hangs from a string wound round a wheel on a fixed axle. As the block falls a distance $d$, the system loses $mgd$ of gravitational potential energy. The block gets part of it as translational kinetic energy; the rest is the wheel's rotational kinetic energy, the gap between the two lines below.

Energy against distance fallen for a block turning a wheel: the decrease in gravitational potential energy, mgd, is the steepest straight line; the wheel's rotational kinetic energy is a straight line with 60 percent of that slope, and the block's translational kinetic energy a line with 40 percent
The energy the block loses is shared: some goes into the block's motion, the rest into spinning the wheel

To measure the wheel's rotational inertia, record $\omega$ and $K_{\text{rot}}$ at several points and plot $K_{\text{rot}}$ against $\omega^2$. The points lie on a straight line through the origin with slope $\tfrac12I$, so $I=2\times\text{slope}$. A slope of $0.015\ \text{J s}^2$ gives $I=0.030\ \text{kg m}^2$.

Similarly, for a cylinder rolling down a ramp and then along a level floor, the total kinetic energy grows in a straight line with the distance travelled down the ramp ($K=mg\,s\sin\theta$), then stays constant along the floor.

Explore

Rolling without slipping

For a wheel that rolls without slipping, v = r omega. Sort each case.

Vocabulary Train
English
Rolling without slipping/ˈrəʊlɪŋ wɪˈðaʊt ˈslɪpɪŋ/
contact point
incline/ɪnˈklaɪn/
6.5

The rolling race

Release several round objects from rest at the top of the same ramp, height $h$. Energy conservation with $v=R\omega$ gives

$$mgh=\tfrac12mv^2+\tfrac12I\omega^2=\tfrac12mv^2\left(1+\frac{I}{mR^2}\right)\;\Rightarrow\;v=\sqrt{\frac{2gh}{1+I/(mR^2)}}.$$
Neither mass nor radius appears on its own: only the shape factor 形状因子 $I/(mR^2)$ matters. For $h=1.2\ \text{m}$:

Object $I/(mR^2)$ Speed at the bottom
block sliding without friction 0 $4.9\ \text{m/s}$
solid sphere 2/5 $4.1\ \text{m/s}$
solid disk (full can) 1/2 $4.0\ \text{m/s}$
hoop (empty can, roughly) 1 $3.4\ \text{m/s}$

The full can wins against the empty one: less of its energy goes into spinning, so more goes into speed.

Vocabulary Train
English
shape factor
6.6

Motion of Orbiting Satellites

Syllabus
Learning ObjectiveEssential Knowledge

6.6.A
Describe the motions of a system consisting of two objects interacting only via gravitational forces.

  • 6.6.A.1 In a system consisting only of a massive central object and an orbiting satellite with mass that is negligible in comparison to the central object's mass, the motion of the central object itself is negligible.
  • 6.6.A.2 The motion of satellites in orbits is constrained by conservation laws.
    • 6.6.A.2.i In circular orbits, the system's total mechanical energy, the system's gravitational potential energy, and the satellite's angular momentum and kinetic energy are constant.
    • 6.6.A.2.ii In elliptical orbits, the system's total mechanical energy and the satellite's angular momentum are constant, but the system's gravitational potential energy and the satellite's kinetic energy can each change.
    • 6.6.A.2.iii The gravitational potential energy of a system consisting of a satellite and a massive central object is defined to be zero when the satellite is an infinite distance from the central object.
      • Equation: $U_g = -G\dfrac{m_1 m_2}{r}$
  • 6.6.A.3 The escape velocity of a satellite is the satellite's velocity such that the mechanical energy of the satellite–central-object system is equal to zero.
    • 6.6.A.3.i When the only force exerted on a satellite is gravity from a central object, a satellite that reaches escape velocity will move away from the central body until its speed reaches zero at an infinite distance from the central body.
    • 6.6.A.3.ii The escape velocity of a satellite from a central body of mass $M$ can be derived using conservation of energy laws.
      • Equation (derived): $v_{\text{esc}} = \sqrt{\dfrac{2GM}{r}}$

Source: College Board AP Course and Exam Description

Orbital motion (Kepler's 2nd law)

A satellite 卫星 in orbit 轨道 is in free fall 自由落体: gravity curves its path. For a circular orbit, gravity provides the centripetal force 向心力, so

$$\frac{GMm}{r^2}=\frac{mv^2}{r}\ \Rightarrow\ v=\sqrt{\frac{GM}{r}}.$$
So a larger orbit means a slower speed. For a circular orbit, angular momentum and mechanical energy 机械能 are both constant; for an elliptical 椭圆的 orbit, angular momentum is conserved (no torque about the planet) while speed varies – fastest when closest.

Gravity provides the centripetal force that keeps a satellite in orbit
Gravity provides the centripetal force that keeps a satellite in orbit

Worked example. Find the speed of a satellite in a low orbit just above the Earth, radius $r=6.4\times10^{6}\ \text{m}$, with $GM=4.0\times10^{14}\ \text{m}^3/\text{s}^2$:

$$v=\sqrt{\frac{GM}{r}}=\sqrt{\frac{4.0\times10^{14}}{6.4\times10^{6}}}=\sqrt{6.25\times10^{7}}\approx 7.9\times10^{3}\ \text{m/s},$$
about $7.9\ \text{km/s}$ – and notice that the satellite's mass cancels, so all low orbits share this speed.

A photograph of the International Space Station orbiting Earth
The International Space Station: a real satellite held in orbit by gravity alone

Escape velocity 逃逸速度 is the launch speed that just lets an object leave for good: its total mechanical energy is exactly zero, so it slows to zero speed only at infinite distance. Setting $\tfrac12 mv^2 - \dfrac{GMm}{r}=0$ (using the general gravitational PE $U_g=-GMm/r$) and solving for $v$,

$$v_{\text{esc}}=\sqrt{\frac{2GM}{r}}.$$
It is $\sqrt2$ times the circular-orbit speed at the same radius, and (like orbital speed) does not depend on the escaping object's mass.

What stays constant in an orbit. When a satellite's mass is tiny compared with the planet's, the planet's own motion can be ignored. Gravitational potential energy is defined to be zero when the two are infinitely far apart, so for any orbit it is negative.

Circular orbit Elliptical orbit
total mechanical energy of the system constant constant
satellite's angular momentum constant constant
gravitational potential energy constant changes
satellite's kinetic energy constant changes

In an ellipse, as the satellite moves closer, $U_g$ becomes more negative and $K$ grows by the same amount. Angular momentum $L=mvr_\perp$ explains the same thing: a smaller $r_\perp$ needs a larger $v$.

Explore

Compare orbits at different radii

A satellite is in free fall, its gravity supplying the centripetal force. A larger orbit means a slower speed and a longer period — Kepler's third law.

Vocabulary Train
English
satellite/ˈsætəlaɪt/
orbit/ˈɔːbɪt/
free fall/friː fɔːl/
centripetal force/senˈtrɪpɪtl fɔːs/
mechanical energy/mɪˈkænɪkl ˈenədʒi/
elliptical
Escape velocity/eˈskeɪp vəˈlɒsɪti/
6.6

Practice

Answer each before reading the answers below. Take $g=9.8\ \text{m/s}^2$.

  1. A flywheel with $I=2.0\ \text{kg m}^2$ spins at $30\ \text{rad/s}$. Find its rotational kinetic energy.
  2. A hoop and a solid disk of equal mass and radius roll from rest down the same ramp. Which reaches the bottom first? Explain without calculating.
  3. A skater spinning at $1.5\ \text{rev/s}$ reduces her rotational inertia from $3.0$ to $1.2\ \text{kg m}^2$. Find her new rate of spin.
  4. One satellite orbits at four times the radius of another. Compare their orbital speeds.
  5. A student says: "Angular momentum is conserved when the skater pulls her arms in, so her kinetic energy is conserved too." Correct the student.
6.6

Answers

  1. $K=\tfrac12(2.0)(30)^2=900\ \text{J}$.
  2. The disk. A hoop has all its mass at the rim, so a larger share of its energy goes into rotation and less into speed. The disk's shape factor is $\tfrac12$, the hoop's is 1.
  3. $\omega_2=\dfrac{3.0}{1.2}(1.5)=3.75\ \text{rev/s}$.
  4. $v\propto1/\sqrt{r}$, so the outer satellite moves at half the speed.
  5. With $L$ fixed, $K=L^2/2I$ rises as $I$ falls. Her muscles do work pulling her arms inward, and that work becomes the extra kinetic energy. Angular momentum is conserved; kinetic energy is not.
6.6

Exam tips

  • Conserve angular momentum $L=I\omega$ when no external torque acts: a smaller $I$ (arms pulled in) gives a larger $\omega$.
  • A rolling object splits its energy between $\tfrac12 mv^2$ and $\tfrac12 I\omega^2$, linked by $v=r\omega$ — so it accelerates down a ramp more slowly than a sliding one.
  • For a circular orbit set gravity equal to the centripetal requirement: $v=\sqrt{GM/r}$, so a larger orbit is slower and the satellite's mass cancels.
  • Pulling in raises the spin and the kinetic energy — the extra energy comes from the work done pulling inward; $L$ is unchanged.
  • Watch which rotational quantity is conserved: $L$ (no torque) versus energy (no friction) are different conditions.

Common mistakes

  • Leaving out rotational kinetic energy for a rolling object. Its total kinetic energy is $\tfrac12 mv^2 + \tfrac12 I\omega^2$, so it reaches the bottom of a ramp slower than a sliding block.
  • Using $\omega$ in rev/s inside $\tfrac12 I\omega^2$. Change to rad/s first ($\times 2\pi$); in $I_1\omega_1 = I_2\omega_2$ any unit works, because it cancels.
  • Saying a skater's kinetic energy stays the same when she pulls her arms in. Angular momentum stays the same; kinetic energy rises, supplied by the work her muscles do.
  • Conserving linear momentum when an object hits a pivoted rod. The pivot exerts an external force; conserve angular momentum about the pivot instead.
  • Thinking a heavier ball rolls down faster. For rolling from rest, only the shape factor $I/(mR^2)$ decides the speed.
  • Writing that "there is no gravity" on an orbiting satellite. Gravity is the centripetal force; the satellite is in free fall.
  • Saying static friction takes energy from a rolling object. Without slipping, the contact point does not move, so static friction does no work.
  • Thinking that the same angular impulse gives the same kinetic energy. It gives the same angular momentum; the object with the smaller $I$ gets more energy.
  • Saying a disk that sticks to a rod gives it more spin than one that bounces. Bouncing reverses the disk's angular momentum, so it gives the larger angular impulse.
  • Saying the potential energy of a satellite in an elliptical orbit stays constant. Only the total energy and the angular momentum are constant.

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