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Unit 3: Work, Energy, and Power

Physics C Mech cheatsheet

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Work measures energy transferred by a force acting through a displacement. For a constant force,

W=F⃗⋅Δr⃗=FΔrcos⁡θ.W = \vec{F}\cdot \Delta \vec{r} = F\Delta r\cos\theta.

Only the component of force parallel to displacement does work. A perpendicular force can change direction without changing speed, so it does no work at that instant. Due to this property, perpendicular forces like the normal force cannot exert any work.

For a variable force, use the line integral (just the integral over the path of an object) to evaluate work:

W=∫CF⃗⋅dr⃗.W = \int_C \vec{F}\cdot d\vec{r}.

In one dimension (which involves most AP Physics C problems) this becomes

W=∫xixfFx(x) dx,W = \int_{x_i}^{x_f} F_x(x)\, dx,

the signed area under the force-position graph.

WorkxF

Work is a scalar, so it has a sign but no direction. Since W=F⃗⋅Δr⃗=F Δrcos⁡θW = \vec{F}\cdot\Delta\vec{r} = F\,\Delta r\cos\theta, the sign of the work is set entirely by the angle θ\theta between the force and the displacement:

¢x~FFcosµµ
  • Positive work (0≤θ<90∘0\le\theta<90^\circ): the force has a component along the motion and speeds the object up (it transfers energy into the object). A horizontal push on a sliding box does positive work.
  • Negative work (90∘<θ≤180∘90^\circ<\theta\le180^\circ): the force opposes the motion and slows the object (it removes energy). Kinetic friction on a sliding box does negative work.
  • Zero work (θ=90∘\theta=90^\circ): a force perpendicular to the velocity does no work. The normal force on a block sliding along a floor, the tension on a ball in uniform circular motion, and the magnetic force on a charge all do zero work even though they are nonzero forces.

Example. A force directed along the xx-axis varies with position as follows: it is constant at F=20 NF=20\ \text{N} from x=0x=0 to x=3 mx=3\ \text{m}, then ramps linearly down to 0 N0\ \text{N} at x=5 mx=5\ \text{m}. Find the work done from x=0x=0 to x=5 mx=5\ \text{m}.

035020x(m)F(N)

The work is the area under the graph. Split it into a rectangle and a triangle:

W=(20 N)(3 m)⏟rectangle+12(2 m)(20 N)⏟triangle=60 J+20 J=80 J.W = \underbrace{(20\ \text{N})(3\ \text{m})}_{\text{rectangle}} + \underbrace{\tfrac{1}{2}(2\ \text{m})(20\ \text{N})}_{\text{triangle}} = 60\ \text{J} + 20\ \text{J} = 80\ \text{J}.

If the force had pointed in the −x-x direction over some interval, that area would count as negative. The graph method and the integral ∫Fx dx\int F_x\,dx are the same calculation; the graph just makes the geometry visible.

Example. A position-dependent force F(x)=αx2−βxF(x)=\alpha x^2-\beta x acts along the xx-axis, where α=6.0 N/m2\alpha=6.0\ \text{N/m}^2 and β=10 N/m\beta=10\ \text{N/m}. Find the work it does on a particle moving from xi=0.50 mx_i=0.50\ \text{m} to xf=3.0 mx_f=3.0\ \text{m}, and state whether the force adds or removes mechanical energy overall.

Use W=∫xixfF(x) dxW = \int_{x_i}^{x_f} F(x)\,dx:

W=∫0.503.0(αx2−βx) dx=[αx33−βx22]0.503.0.W=\int_{0.50}^{3.0}(\alpha x^2-\beta x)\,dx =\left[\frac{\alpha x^3}{3}-\frac{\beta x^2}{2}\right]_{0.50}^{3.0}.

Substitute values:

W=[2x3−5x2]0.503.0=(54−45)−(0.25−1.25)=10 J.W=\left[2x^3-5x^2\right]_{0.50}^{3.0} =(54-45)-\left(0.25-1.25\right)=10\ \text{J}.

Even though the force is negative over part of the interval and positive later, the net work is positive, so it adds 10 J10\ \text{J} of kinetic energy. Whenever the force is not constant, you cannot use W=FdW = Fd; you must integrate.


Kinetic Energy and the Work-Energy Theorem

Section titled “Kinetic Energy and the Work-Energy Theorem”

Kinetic energy is defined as the energy of motion. Translational kinetic energy of a particle is defined as

K=12mv2.K = \frac{1}{2}mv^2.

An important relationship between kinetic energy and work is the Work-Energy Theorem.

Theorem (Work-Energy Theorem). The net work done on a particle equals the change in its kinetic energy, Wnet=ΔKW_{\text{net}} = \Delta K.

Proof (Work-Energy Theorem). Start with Newton’s second law and the definition of work:

Wnet=∫F⃗net⋅dr⃗=∫mdv⃗dt⋅v⃗ dt=∫mv⃗⋅dv⃗=12mvf2−12mvi2.W_{\text{net}} = \int \vec{F}_{\text{net}}\cdot d\vec{r} = \int m\frac{d\vec{v}}{dt}\cdot \vec{v}\,dt = \int m\vec{v}\cdot d\vec{v} = \frac{1}{2}mv_f^2-\frac{1}{2}mv_i^2.

Therefore,

Wnet=ΔK.W_{\text{net}}=\Delta K.

Example. A block of mass m=2.0 kgm = 2.0\ \text{kg} slides across a level floor with initial speed v0=6.0 m/sv_0 = 6.0\ \text{m/s}. The coefficient of kinetic friction is μk=0.30\mu_k = 0.30. How far does it slide before stopping? Use g=9.8 m/s2g = 9.8\ \text{m/s}^2.

The only horizontal force is kinetic friction, fk=μkFN=μkmgf_k = \mu_k F_N = \mu_k mg, directed opposite the motion. Over a distance dd it does negative work

Wnet=−fkd=−μkmg d.W_{\text{net}} = -f_k d = -\mu_k mg\, d.

By the work-energy theorem, Wnet=ΔK=0−12mv02W_{\text{net}} = \Delta K = 0 - \tfrac{1}{2}mv_0^2:

−μkmg d=−12mv02.-\mu_k mg\, d = -\tfrac{1}{2}mv_0^2.

The mass cancels, so the stopping distance does not depend on mm:

d=v022μkg=(6.0)22(0.30)(9.8)=365.88≈6.1 m.d = \frac{v_0^2}{2\mu_k g} = \frac{(6.0)^2}{2(0.30)(9.8)} = \frac{36}{5.88} \approx 6.1\ \text{m}.

Notice that the stopping distance scales with v02v_0^2: doubling the speed quadruples the distance.


Definition. A force is conservative if its work depends only on the initial and final positions, not on the path taken. Equivalently,

∮F⃗⋅dr⃗=0\oint \vec{F}\cdot d\vec{r} = 0

around any closed path. The integral (known as a surface integral) represents the integral around a path, and thus represents the fact that in a closed loop the work done is 00.

For a conservative force, define potential energy UU by

Wcons=−ΔU.W_{\text{cons}} = -\Delta U.

In one dimension,

Fx=−dUdx.F_x = -\frac{dU}{dx}.

This comes directly from comparing a tiny amount of conservative work to a tiny change in potential energy:

dW=Fx dx,dW=F_x\,dx,

and

dW=−dU.dW=-dU.

Therefore

Fx dx=−dU,F_x\,dx=-dU,

so

Fx=−dUdx.F_x=-\frac{dU}{dx}.

In three dimensions,

F⃗=−∇U.\vec{F} = -\nabla U.

The ∇\nabla symbol is just an extension of a derivative to all three dimensions. Potential energy is not an absolute property; it requires a reference level, which is usually set at some point at infinity or zero. Only changes in potential energy affect mechanics.

Near Earth’s surface, where gg is approximately constant, the gravitational potential energy of an object is

Ug=mgyU_g = mgy

if Ug=0U_g = 0 is chosen at y=0y=0. The change in gravitational potential energy is

ΔUg=mgΔy.\Delta U_g = mg\Delta y.

For universal gravitation, the usual zero point is defined at infinity, resulting in:

Ug(r)=−GMmr.U_g(r) = -\frac{GMm}{r}.

The negative sign means a bound mass has less energy than it would have infinitely far away.

Proof (Near-Earth and Universal Gravitational Potential Energy). Near Earth’s surface, the gravitational force is approximately constant:

F⃗g=−mgy^.\vec{F}_g=-mg\hat{y}.

Since Wg=−ΔUgW_g=-\Delta U_g,

ΔUg=−Wg=−∫yiyf(−mg) dy=mg(yf−yi).\Delta U_g=-W_g=-\int_{y_i}^{y_f}(-mg)\,dy=mg(y_f-y_i).

So, choosing Ug=0U_g=0 at y=0y=0,

Ug=mgy.U_g=mgy.

For universal gravitation,

Fr=−GMmr2.F_r=-\frac{GMm}{r^2}.

Using Fr=−dU/drF_r=-dU/dr,

dUdr=GMmr2.\frac{dU}{dr}=\frac{GMm}{r^2}.

Integrate:

U(r)=−GMmr+C.U(r)=-\frac{GMm}{r}+C.

Choosing U(∞)=0U(\infty)=0 forces C=0C=0, so

Ug(r)=−GMmr.U_g(r)=-\frac{GMm}{r}.

The fact that we could even define a potential energy depends on gravity being conservative: the work it does between two points does not depend on the route taken.

Proof (gravity near Earth is path-independent). Near Earth’s surface F⃗g=−mg y^\vec{F}_g = -mg\,\hat{y}, a constant vector. For any path from point AA to point BB,

Wg=∫ABF⃗g⋅dr⃗.W_g=\int_A^B \vec{F}_g\cdot d\vec{r}.

Since F⃗g=−mgy^\vec{F}_g=-mg\hat{y} and dr⃗=dxx^+dyy^d\vec{r}=dx\hat{x}+dy\hat{y},

Wg=∫AB(−mgy^)⋅(dxx^+dyy^).W_g=\int_A^B (-mg\hat{y})\cdot(dx\hat{x}+dy\hat{y}).

The xx part vanishes because y^⋅x^=0\hat{y}\cdot\hat{x}=0, leaving

Wg=−mg∫yAyBdy=−mg(yB−yA).W_g=-mg\int_{y_A}^{y_B}dy=-mg(y_B-y_A).

The xx-displacement drops out because y^⋅x^=0\hat{y}\cdot\hat{x}=0, so only the change in height matters. A box carried straight up, or up a long ramp, or along a wiggling staircase to the same final height, all involve the same gravitational work. Around any closed loop (yB=yAy_B = y_A), Wg=0W_g = 0, which is the defining property of a conservative force.

Example. With what speed vescv_{\text{esc}} must a projectile leave a planet’s surface (mass MM, radius RR, no air) so that it just barely reaches infinity (aka escapes the gravitational pull of the planet)? Use Ug(r)=−GMm/rU_g(r) = -GMm/r.

“Just barely reaches infinity” means the projectile arrives at r→∞r\to\infty with zero speed. With only gravity acting, mechanical energy is conserved:

12mvesc2+(−GMmR)=0⏟K∞+0⏟U∞.\tfrac{1}{2}mv_{\text{esc}}^2 + \left(-\frac{GMm}{R}\right) = \underbrace{0}_{K_\infty} + \underbrace{0}_{U_\infty}.

Solving for vescv_{\text{esc}},

12mvesc2=GMmR,vesc=2GMR.\tfrac{1}{2}mv_{\text{esc}}^2 = \frac{GMm}{R}, \qquad v_{\text{esc}} = \sqrt{\frac{2GM}{R}}.

The mass of the projectile cancels, so escape speed is the same for a pebble or a rocket. Using g=GM/R2g = GM/R^2 at the surface, this can be rewritten as vesc=2gRv_{\text{esc}} = \sqrt{2gR}. For Earth (g=9.8 m/s2g = 9.8\ \text{m/s}^2, R=6.37×106 mR = 6.37\times10^6\ \text{m}), vesc≈1.12×104 m/sv_{\text{esc}}\approx 1.12\times10^4\ \text{m/s}, about 11.2 km/s11.2\ \text{km/s}.

For an ideal, massless spring, the potential energy stored in the spring is

Us=12kx2,U_s = \frac{1}{2}kx^2,

where xx is displacement from equilibrium.

Proof (Spring Potential Energy). Hooke’s law is

Fs=−kx.F_s=-kx.

For a conservative force,

Fs=−dUsdx.F_s=-\frac{dU_s}{dx}.

Therefore

−kx=−dUsdx,-kx=-\frac{dU_s}{dx},

so

dUsdx=kx.\frac{dU_s}{dx}=kx.

Integrating gives

Us=12kx2+C.U_s=\frac{1}{2}kx^2+C.

Choosing Us=0U_s=0 at equilibrium, where x=0x=0, makes C=0C=0. Thus

Us=12kx2.U_s=\frac{1}{2}kx^2.

Example. A spring has stiffness k=400 N/mk = 400\ \text{N/m}. How much work must an external agent do to stretch it from its natural length to x1=0.10 mx_1 = 0.10\ \text{m}, and then how much additional work to stretch it from x1x_1 to x2=0.20 mx_2 = 0.20\ \text{m}?

To stretch the spring slowly, the external force must balance the spring force, so Fext(x)=+kxF_{\text{ext}}(x) = +kx. The work done by this external force is

Wext=∫0xkx′ dx′=12kx2,W_{\text{ext}} = \int_{0}^{x} kx'\,dx' = \tfrac{1}{2}kx^2,

which is exactly the stored potential energy. For the first stretch,

W1=12(400)(0.10)2=2.0 J.W_1 = \tfrac{1}{2}(400)(0.10)^2 = 2.0\ \text{J}.

To reach x2=0.20 mx_2 = 0.20\ \text{m}, the total stored energy is

12(400)(0.20)2=8.0 J,\tfrac{1}{2}(400)(0.20)^2 = 8.0\ \text{J},

so the additional work is

W2=8.0 J−2.0 J=6.0 J.W_2 = 8.0\ \text{J} - 2.0\ \text{J} = 6.0\ \text{J}.

Stretching the second 10 cm10\ \text{cm} takes three times the work of the first, because the force grows with displacement — the energy goes as x2x^2, not xx. The spring itself does work −12kx2-\tfrac{1}{2}kx^2 during stretching (opposing the motion).


Defined mechanical energy as

Emech=K+U.E_{\text{mech}} = K + U.

If only conservative forces do work (e.g. no friction), mechanical energy is conserved:

Ki+Ui=Kf+Uf.K_i + U_i = K_f + U_f.

Proof (Conservation of Mechanical Energy). The work-energy theorem says

Wnet=ΔK.W_{\text{net}}=\Delta K.

If only conservative forces do work,

Wnet=Wcons.W_{\text{net}}=W_{\text{cons}}.

By definition of potential energy,

Wcons=−ΔU.W_{\text{cons}}=-\Delta U.

Therefore

ΔK=−ΔU,\Delta K=-\Delta U,

or

Δ(K+U)=0.\Delta(K+U)=0.

So

Ki+Ui=Kf+Uf.K_i+U_i=K_f+U_f.

Example. A bob on a string of length L=1.5 mL = 1.5\ \text{m} is released from rest at an angle θ=60∘\theta = 60^\circ from vertical. Find its speed at the lowest point. Ignore air resistance.

The tension is always perpendicular to the bob’s velocity, so it does no work; only gravity does work, and mechanical energy is conserved. The bob’s height above the lowest point when the string makes angle θ\theta is

h=L−Lcos⁡θ=L(1−cos⁡θ).h = L - L\cos\theta = L(1-\cos\theta).

Taking the lowest point as U=0U = 0 and using Ki=0K_i = 0:

mgh=12mv2  ⇒  v=2gh=2gL(1−cos⁡θ).mgh = \tfrac{1}{2}mv^2 \;\Rightarrow\; v = \sqrt{2gh} = \sqrt{2gL(1-\cos\theta)}.

Numerically, h=1.5(1−cos⁡60∘)=1.5(1−0.5)=0.75 mh = 1.5(1-\cos 60^\circ) = 1.5(1-0.5) = 0.75\ \text{m}, so

v=2(9.8)(0.75)=14.7≈3.8 m/s.v = \sqrt{2(9.8)(0.75)} = \sqrt{14.7} \approx 3.8\ \text{m/s}.

The same v=2ghv = \sqrt{2gh} result holds for a block sliding down any frictionless ramp or curved track through the same height drop, regardless of the shape of the path — only the vertical drop hh matters.

If nonconservative forces such as kinetic friction, air drag, or applied pushes do work, then

Ki+Ui+Wnc=Kf+Uf.K_i + U_i + W_{\text{nc}} = K_f + U_f.

Equivalently,

Wnc=ΔEmech.W_{\text{nc}} = \Delta E_{\text{mech}}.

Friction usually decreases mechanical energy and converts it into thermal energy, so WfW_f is usually negative for a sliding object.

It is worth being careful about two different “totals.” Total mechanical energy Emech=K+UE_{\text{mech}} = K + U counts only kinetic and potential energy, and it is not conserved when nonconservative forces act — friction, drag, and inelastic deformation all lessen it away. Total energy, however, is always conserved: the mechanical energy lost to friction does not vanish, it reappears as thermal energy (and a little sound). If we write

ΔEmech+ΔEthermal+⋯=0,\Delta E_{\text{mech}} + \Delta E_{\text{thermal}} + \cdots = 0,

energy is conserved overall, with any mechanical energy lost usually being converted to heat or sound. This ensures that we don’t violate the Law of Conservation of Energy.

Example. A block of mass m=3.0 kgm = 3.0\ \text{kg} is released from rest and slides a distance d=4.0 md = 4.0\ \text{m} down a 30∘30^\circ incline with coefficient of kinetic friction μk=0.20\mu_k = 0.20. Find its speed at the bottom of that slide. Use g=9.8 m/s2g = 9.8\ \text{m/s}^2.

Gravity (conservative) and friction (nonconservative) both do work. Use Ki+Ui+Wnc=Kf+UfK_i + U_i + W_{\text{nc}} = K_f + U_f with the bottom of the slide as U=0U = 0. The block drops a height h=dsin⁡θh = d\sin\theta, so Ui=mgdsin⁡θU_i = mgd\sin\theta. The normal force is FN=mgcos⁡θF_N = mg\cos\theta, so friction does work

Wnc=−fkd=−μkmgcos⁡θ d.W_{\text{nc}} = -f_k d = -\mu_k mg\cos\theta\,d.

With Ki=0K_i = 0:

mgdsin⁡θ−μkmgcos⁡θ d=12mv2.mgd\sin\theta - \mu_k mg\cos\theta\,d = \tfrac{1}{2}mv^2.

Mass cancels, and solving for vv:

v=2gd(sin⁡θ−μkcos⁡θ).v = \sqrt{2gd(\sin\theta - \mu_k\cos\theta)}.

Plugging in, sin⁡30∘=0.500\sin 30^\circ = 0.500 and cos⁡30∘=0.866\cos 30^\circ = 0.866:

v=2(9.8)(4.0)(0.500−0.20(0.866))=78.4(0.327)=25.6≈5.1 m/s.v = \sqrt{2(9.8)(4.0)\big(0.500 - 0.20(0.866)\big)} = \sqrt{78.4(0.327)} = \sqrt{25.6} \approx 5.1\ \text{m/s}.

For comparison, a frictionless incline would give v=2gdsin⁡θ=39.2≈6.3 m/sv = \sqrt{2gd\sin\theta} = \sqrt{39.2}\approx 6.3\ \text{m/s}; friction has carried away the difference as heat.

Example. A 0.50 kg0.50\ \text{kg} block is pressed against a spring (k=800 N/mk = 800\ \text{N/m}) compressed by x=0.12 mx = 0.12\ \text{m} on a horizontal surface. After release, the block crosses a rough patch of length L=1.2 mL = 1.2\ \text{m} with μk=0.25\mu_k=0.25, then climbs a frictionless ramp that rises by height h=0.40 mh=0.40\ \text{m}. Find whether the block reaches the top of the ramp, and if it does, find its speed there.

The spring force is conservative, so its stored energy Us=12kx2U_s = \tfrac{1}{2}kx^2 is the initial energy. Friction is the only nonconservative force. Apply

Ki+Ui+Wnc=Kf+Uf.K_i + U_i + W_{\text{nc}} = K_f + U_f.

Here Ki=0K_i=0 and the initial spring energy is Us=12kx2U_s=\tfrac12kx^2. Friction removes μkmgL\mu_kmgL on the rough patch, and climbing the ramp requires gravitational potential energy mghmgh. If the remaining energy is positive, the block reaches the top:

12kx2−μkmgL−mgh=12mv2.\tfrac{1}{2}kx^2-\mu_kmgL-mgh=\tfrac{1}{2}mv^2.

Compute each energy term:

12kx2=12(800)(0.12)2=5.76 J,\tfrac{1}{2}kx^2=\tfrac{1}{2}(800)(0.12)^2=5.76\ \text{J}, μkmgL=(0.25)(0.50)(9.8)(1.2)=1.47 J,\mu_kmgL=(0.25)(0.50)(9.8)(1.2)=1.47\ \text{J},

and

mgh=(0.50)(9.8)(0.40)=1.96 J.mgh=(0.50)(9.8)(0.40)=1.96\ \text{J}.

The remaining kinetic energy is

12mv2=5.76−1.47−1.96=2.33 J.\tfrac12mv^2=5.76-1.47-1.96=2.33\ \text{J}.

Since this is positive, the block reaches the top. Its speed there is

v=2(2.33)0.50=9.32≈3.1 m/s.v=\sqrt{\frac{2(2.33)}{0.50}}=\sqrt{9.32}\approx3.1\ \text{m/s}.

The clean strategy: spring energy in, friction and gravitational potential out, kinetic energy is whatever remains.


In one-dimensional systems, a graph of U(x)U(x) contains lots of useful information about force and an object’s current state. As a reminder, Fx=−dUdx.F_x = -\frac{dU}{dx}. Equilibrium occurs where

dUdx=0,\frac{dU}{dx}=0,

and at that point, the object has zero acceleration (since force is zero). The equilibrium is stable if U(x)U(x) has a local minimum (d2Udx2>0\frac{d^2 U}{dx^2} > 0), unstable if it has a local maximum (d2Udx2<0\frac{d^2 U}{dx^2} < 0), and neutral if small displacements do not change UU to second order (d2Udx2=0\frac{d^2 U}{dx^2} = 0). A metastable (neutral) equilibrium is a local minimum that is stable for small disturbances but can escape if the total energy is high enough to cross a nearby barrier.

stableunstableneutral

Example. A particle of mass m=0.20 kgm = 0.20\ \text{kg} moves in one dimension under the potential

U(x)=2x2−x4U(x) = 2x^2 - x^4

(in joules, with xx in meters). Find the equilibrium positions and classify them, find the force at x=0.5 mx = 0.5\ \text{m}, and if the particle has total energy E=0.5 JE = 0.5\ \text{J} and is at x=0x=0, find its speed there.

Equilibria. Set dU/dx=0dU/dx = 0:

dUdx=4x−4x3=4x(1−x2)=0  ⇒  x=0, ±1.\frac{dU}{dx} = 4x - 4x^3 = 4x(1 - x^2) = 0 \;\Rightarrow\; x = 0,\ \pm 1.

To classify, use the second derivative U′′(x)=4−12x2U''(x) = 4 - 12x^2:

  • At x=0x = 0: U′′=4>0U'' = 4 > 0, a local minimum → stable equilibrium.
  • At x=±1x = \pm 1: U′′=4−12=−8<0U'' = 4 - 12 = -8 < 0, local maxima → unstable equilibria.

Force at x=0.5x = 0.5. The force is

Fx=−dUdx=−(4x−4x3)=−4(0.5)+4(0.5)3=−2+0.5=−1.5 N.F_x = -\frac{dU}{dx} = -(4x - 4x^3) = -4(0.5) + 4(0.5)^3 = -2 + 0.5 = -1.5\ \text{N}.

The force points toward −x-x, i.e. back toward the stable minimum at the origin — a restoring force, as expected near a potential well.

Speed at x=0x = 0. Here U(0)=0U(0) = 0, so all the energy is kinetic:

12mv2=E−U(0)=0.5 J  ⇒  v=2(0.5)0.20=5≈2.2 m/s.\tfrac{1}{2}mv^2 = E - U(0) = 0.5\ \text{J} \;\Rightarrow\; v = \sqrt{\frac{2(0.5)}{0.20}} = \sqrt{5} \approx 2.2\ \text{m/s}.

The particle is trapped in the well as long as EE is below the barrier height U(±1)=2−1=1 JU(\pm 1) = 2 - 1 = 1\ \text{J}; its turning points are where U(x)=EU(x) = E. With E=0.5 J<1 JE = 0.5\ \text{J} < 1\ \text{J}, it oscillates back and forth inside the well.


Power is defined as the rate of energy transfer:

P=dWdt.P = \frac{dW}{dt}.

For a constant force acting on an object with instantaneous velocity v⃗\vec{v},

P=F⃗⋅v⃗.P = \vec{F}\cdot \vec{v}.

Average power over a time interval is also defined as

Pˉ=ΔEΔt.\bar{P} = \frac{\Delta E}{\Delta t}.

Power is not a new kind of energy; it is how quickly energy is transferred or transformed.

Example. A car of mass m=1200 kgm = 1200\ \text{kg} drives up a 5.0∘5.0^\circ incline at a constant v=25 m/sv = 25\ \text{m/s}. Neglecting friction and drag, what power must the engine deliver? Use g=9.8 m/s2g = 9.8\ \text{m/s}^2.

At constant speed there is no change in kinetic energy, so the engine’s drive force must exactly balance the component of gravity along the incline:

F=mgsin⁡θ=(1200)(9.8)sin⁡5.0∘=(11760)(0.0872)≈1.03×103 N.F = mg\sin\theta = (1200)(9.8)\sin 5.0^\circ = (11760)(0.0872) \approx 1.03\times 10^3\ \text{N}.

Since the drive force is along the velocity, P=FvP = Fv:

P=(1.03×103 N)(25 m/s)≈2.6×104 W≈26 kW.P = (1.03\times 10^3\ \text{N})(25\ \text{m/s}) \approx 2.6\times 10^4\ \text{W} \approx 26\ \text{kW}.

Equivalently, the engine supplies gravitational potential energy at the rate P=mg vsin⁡θ=mg vyP = mg\,v\sin\theta = mg\,v_y, where vy=vsin⁡θv_y = v\sin\theta is the rate of gain of height. Both routes give the same answer because P=F⃗⋅v⃗P = \vec{F}\cdot\vec{v} counts only the force component along the motion.


  1. A force is always perpendicular to a particle’s velocity. The force can change the particle’s

(A) speed but not direction

(B) direction but not speed

(C) kinetic energy only

(D) total mechanical energy only

  1. A block slides up a rough incline and comes momentarily to rest. Compared with its mechanical energy at launch, its mechanical energy at the top is

(A) greater

(B) smaller

(C) the same

(D) zero

  1. A force F(x)=3x2−2xF(x)=3x^2-2x acts on a particle from x=0x=0 to x=Lx=L. The work done is

(A) L3−L2L^3-L^2

(B) 3L2−2L3L^2-2L

(C) L3+L2L^3+L^2

(D) 3L3−L23L^3-L^2

  1. If U(x)=ax4−bx2U(x)=ax^4-bx^2 with a,b>0a,b>0, the force is

(A) Fx=4ax3−2bxF_x=4ax^3-2bx

(B) Fx=−4ax3+2bxF_x=-4ax^3+2bx

(C) Fx=ax4−bx2F_x=ax^4-bx^2

(D) Fx=−a/x4+b/x2F_x=-a/x^4+b/x^2

  1. A particle moves in one dimension with potential energy U(x)U(x). At a stable equilibrium,

(A) U′=0U'=0 and U′′>0U''>0

(B) U′=0U'=0 and U′′<0U''<0

(C) U′>0U'>0 and U′′=0U''=0

(D) U<0U<0 only

  1. A block starts from rest at height HH above a horizontal spring, slides on a frictionless track, and compresses the spring a distance xx. If the block instead starts from height 4H4H, the new maximum compression is

(A) x/2x/2

(B) xx

(C) 2x2x

(D) 4x4x

  1. A spring with constant kk is cut into two equal halves. One half is used as a spring. Compared with the original spring, the energy stored for the same stretch xx is

(A) half as large

(B) the same

(C) twice as large

(D) four times as large

  1. A block moves through a region where a force F(x)=F0e−x/LF(x)=F_0e^{-x/L} acts in the direction of motion. The work done from x=0x=0 to x=2Lx=2L is

(A) F0L(1−e−2)F_0L(1-e^{-2})

(B) 2F0L2F_0L

(C) F0Le−2F_0L e^{-2}

(D) F0/LF_0/L

  1. A cart of mass mm moves under constant power PP from rest, with no resistive forces. Its speed after time tt is

(A) Pt/mPt/m

(B) 2Pt/m\sqrt{2Pt/m}

(C) 2Pt/m2Pt/m

(D) Pt/(2m)\sqrt{Pt/(2m)}

  1. A satellite moves outward from radius rr to radius 2r2r around a planet of mass MM. The work done by gravity during this motion is

(A) −GMm2r-\dfrac{GMm}{2r}

(B) −GMmr-\dfrac{GMm}{r}

(C) GMm2r\dfrac{GMm}{2r}

(D) zero, because gravity is perpendicular to orbital motion

  1. A particle in potential U(x)=Ax2−BxU(x)=\dfrac{A}{x^2}-\dfrac{B}{x}, with A,B>0A,B>0, has a stable equilibrium at

(A) x=A/Bx=A/B

(B) x=2A/Bx=2A/B

(C) x=B/Ax=B/A

(D) x=A/Bx=\sqrt{A/B}

  1. A projectile is launched upward from the surface of a planet of radius RR with speed vesc/2v_{\text{esc}}/2. Neglect air resistance. Its maximum distance from the planet’s center is

(A) 4R/34R/3

(B) 3R/23R/2

(C) 2R2R

(D) 4R4R

  1. A block of mass mm starts from rest at height HH on a frictionless curved track, then crosses a rough horizontal patch of length LL with coefficient of kinetic friction μk\mu_k before compressing a spring of constant kk.

    (A)(A) Derive the speed of the block just before the rough patch.

    (B)(B) Determine the speed just after the rough patch.

    (C)(C) Find the maximum spring compression.

    (D)(D) Determine the condition on HH for the block to reach the spring.

  1. A particle of mass mm moves in the potential U(x)=ax4−bx2U(x)=ax^4-bx^2, where a,b>0a,b>0

    (A)(A) Find all equilibrium positions.

    (B)(B) Classify each equilibrium as stable or unstable.

    (C)(C) If the particle has total energy E=0E=0, find its turning points.

    (D)(D) If the particle has total energy E=0E=0, determine where its speed is greatest and justify your answer using the energy diagram.

  1. A small spacecraft of mass mm moves radially away from a planet of mass MM. Its engine supplies constant power PP for time t0t_0, starting from rest at radius RR. Ignore air resistance and the changing mass of the spacecraft.

    (A)(A) Write an energy equation relating the spacecraft’s speed and radius after the burn.

    (B)(B) Determine the minimum engine energy needed for escape if the burn ends at radius rfr_f.

    (C)(C) Explain whether delivering the same energy quickly or slowly changes the escape condition in this idealized model.

    (D)(D) Identify one assumption in the model that would fail for a real rocket.