Classical-Mechanics Β· Unit 15 Β· Video 3 Β· Interactive Practice

Inverse-Square Forces and the Work-Energy Theorem in Three Dimensions

IKey Formulas

FormulaNameWhat you need
dW=Fβƒ—β‹…drβƒ—=Fr drdW = \vec{F}\cdot d\vec{r} = F_r\,drCentral-force work elementA force along r^\hat{r}; the sideways term Fr r dθ (r^β‹…ΞΈ^)F_r\,r\,d\theta\,(\hat{r}\cdot\hat{\theta}) dies because r^β‹…ΞΈ^=0\hat{r}\cdot\hat{\theta} = 0
W=C(1rfβˆ’1ri)W = C\left(\dfrac{1}{r_f} - \dfrac{1}{r_i}\right)Work of an inverse-square forceOnly the two radii, plus the constant: C=GmsmC = G m_s m for gravity, C=βˆ’q1q24πΡ0C = -\dfrac{q_1 q_2}{4\pi\varepsilon_0} for Coulomb
∫ifFβƒ—β‹…drβƒ—=Kfβˆ’Ki\int_i^f \vec{F}\cdot d\vec{r} = K_f - K_iWork-energy theorem in three dimensionsThe force along the path and the two speeds, K=12mv2K = \tfrac{1}{2}mv^2
P=F⃗⋅v⃗=dKdtP = \vec{F}\cdot\vec{v} = \dfrac{dK}{dt}Instantaneous powerForce and velocity at a single instant

Key Insight: Both inverse-square results are the same formula wearing a different constant β€” and whichever way the force points, a body that moves the way the force pushes it receives positive work. Gravity pulling a comet inward and repulsion driving two like charges apart both give W>0W > 0.

IIVisualization 1 β€” Which Part of the Step Does the Work

A central force can only work through the radial piece of a step; the sideways piece dots to zero.

πŸ’‘ Any other path joining the same two radii gives exactly the same work β€” the integral remembers rir_i and rfr_f and nothing else about the route.

IIIVisualization 2 β€” Attraction, Repulsion, and the Sign of WW

Opposite signs or like signs, a charge that moves the way the force pushes it gains energy.

πŸ’‘ Replace k q1q2k\,q_1 q_2 by βˆ’Gmsm-G m_s m and this panel becomes the gravitational case: gravity is the inverse-square force whose constant can never change sign.

IVVisualization 3 β€” Power, and the Force That Bends Without Working

Only the component of force along the velocity changes the speed; the rest merely bends the path.

VQuiz Questions

Problem 1 Β· Work Done by the Sun's Gravity

Given: A body falls along a curved orbital arc from ri=6.0Γ—1011Β mr_i = 6.0\times10^{11}\ \text{m} to rf=2.0Γ—1011Β mr_f = 2.0\times10^{11}\ \text{m} from the centre of the sun, with Gmsm=3.0Γ—1022Β Jβ‹…mG m_s m = 3.0\times10^{22}\ \text{J}\cdot\text{m} β€” find the work WW done by gravity.

βœ… Correct! The body moves inward, gravity points inward, and the bracket (1rfβˆ’1ri)\left(\tfrac{1}{r_f} - \tfrac{1}{r_i}\right) comes out positive β€” gravity feeds 1.0Γ—1011Β J1.0\times10^{11}\ \text{J} of kinetic energy in.
❌ Check the order of the reciprocals. The bracket is 1rfβˆ’1ri\tfrac{1}{r_f} - \tfrac{1}{r_i}, final first. Since rf<rir_f < r_i, the reciprocal 1rf\tfrac{1}{r_f} is the larger one, so the bracket β€” and the work β€” is positive.
❌ You dropped the second term. 1ri=1.67Γ—10βˆ’12Β mβˆ’1\tfrac{1}{r_i} = 1.67\times10^{-12}\ \text{m}^{-1} is not negligible; subtract it from 1rf=5.0Γ—10βˆ’12Β mβˆ’1\tfrac{1}{r_f} = 5.0\times10^{-12}\ \text{m}^{-1} before multiplying.
❌ The force is not constant. Treating FF as its final value Gmsm/rf2=0.75Β NGm_sm/r_f^2 = 0.75\ \text{N} over a displacement of 4.0Γ—1011Β m4.0\times10^{11}\ \text{m} overcounts badly β€” the force was far weaker over most of the fall, which is exactly why the integral is needed.
❌ Not quite. Use W=Gmsm(1rfβˆ’1ri)W = G m_s m\left(\tfrac{1}{r_f} - \tfrac{1}{r_i}\right) with the reciprocals of the two radii.
Show solution

Gravity is central, so the line integral collapses to a one-dimensional integral in rr with Fr=βˆ’Gmsm/r2F_r = -Gm_sm/r^2:

W=∫rirf(βˆ’Gmsmr2)dr=Gmsmr∣rirf=Gmsm(1rfβˆ’1ri)W = \int_{r_i}^{r_f}\left(-\frac{G m_s m}{r^2}\right)dr = \left.\frac{G m_s m}{r}\right|_{r_i}^{r_f} = G m_s m\left(\frac{1}{r_f} - \frac{1}{r_i}\right)

Substituting the numbers:

W=(3.0Γ—1022)(12.0Γ—1011βˆ’16.0Γ—1011)=(3.0Γ—1022)(3.33Γ—10βˆ’12)=1.0Γ—1011Β JW = (3.0\times10^{22})\left(\frac{1}{2.0\times10^{11}} - \frac{1}{6.0\times10^{11}}\right) = (3.0\times10^{22})(3.33\times10^{-12}) = 1.0\times10^{11}\ \text{J}

Sign check: rf<ri⇒1rf>1ri⇒W>0r_f < r_i \Rightarrow \tfrac{1}{r_f} > \tfrac{1}{r_i} \Rightarrow W > 0. The force points inward and the body moves inward, so gravity does positive work — the same sign as a stone falling toward the earth.

Note that the shape of the curved arc never entered the calculation: only the two radii did.

Problem 2 Β· Two Like Charges Flying Apart

Given: q1=+2.0Β ΞΌCq_1 = +2.0\ \mu\text{C} is held fixed while q2=+3.0Β ΞΌCq_2 = +3.0\ \mu\text{C} moves from ri=0.10Β mr_i = 0.10\ \text{m} out to rf=0.30Β mr_f = 0.30\ \text{m}. Take 14πΡ0=9.0Γ—109Β Nβ‹…m2/C2\dfrac{1}{4\pi\varepsilon_0} = 9.0\times10^{9}\ \text{N}\cdot\text{m}^2/\text{C}^2 β€” find the work done by the electric force on q2q_2. The formula carries a leading minus sign β€” and so does the bracket here.

βœ… Correct! Two minus signs meet: the bracket is negative because rf>rir_f > r_i, and the formula's own leading minus flips it back β€” repulsion driving the charges apart does positive work.
❌ One minus sign too few (or too many). Here q1q2>0q_1q_2 > 0 and 1rfβˆ’1ri=3.33βˆ’10=βˆ’6.67Β mβˆ’1<0\tfrac{1}{r_f} - \tfrac{1}{r_i} = 3.33 - 10 = -6.67\ \text{m}^{-1} < 0; the leading minus in W=βˆ’q1q24πΡ0(1rfβˆ’1ri)W = -\tfrac{q_1q_2}{4\pi\varepsilon_0}\left(\tfrac{1}{r_f}-\tfrac{1}{r_i}\right) turns that product positive.
❌ Both reciprocals belong in the bracket. Compute 10.30βˆ’10.10=3.33βˆ’10=βˆ’6.67Β mβˆ’1\tfrac{1}{0.30} - \tfrac{1}{0.10} = 3.33 - 10 = -6.67\ \text{m}^{-1} β€” not one term alone.
❌ Not quite. Apply W=βˆ’q1q24πΡ0(1rfβˆ’1ri)W = -\dfrac{q_1q_2}{4\pi\varepsilon_0}\left(\dfrac{1}{r_f} - \dfrac{1}{r_i}\right) with q1q2=+6.0Γ—10βˆ’12Β C2q_1q_2 = +6.0\times10^{-12}\ \text{C}^2.
Show solution

Coulomb's law gives Fr=14πΡ0q1q2r2F_r = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q_1q_2}{r^2} along r^\hat{r}, with no built-in minus sign β€” the sign lives in the charge product. The central-force collapse then gives

W=∫rirf14πΡ0q1q2r2 dr=βˆ’14πΡ0q1q2(1rfβˆ’1ri)W = \int_{r_i}^{r_f}\frac{1}{4\pi\varepsilon_0}\frac{q_1q_2}{r^2}\,dr = -\frac{1}{4\pi\varepsilon_0}q_1q_2\left(\frac{1}{r_f} - \frac{1}{r_i}\right)

Step 1 β€” the prefactor. q1q2=(2.0Γ—10βˆ’6)(3.0Γ—10βˆ’6)=6.0Γ—10βˆ’12Β C2q_1q_2 = (2.0\times10^{-6})(3.0\times10^{-6}) = 6.0\times10^{-12}\ \text{C}^2, so

q1q24πΡ0=(9.0Γ—109)(6.0Γ—10βˆ’12)=0.054Β Jβ‹…m\frac{q_1q_2}{4\pi\varepsilon_0} = (9.0\times10^{9})(6.0\times10^{-12}) = 0.054\ \text{J}\cdot\text{m}

Step 2 β€” the bracket. 10.30βˆ’10.10=3.33βˆ’10=βˆ’6.67Β mβˆ’1\dfrac{1}{0.30} - \dfrac{1}{0.10} = 3.33 - 10 = -6.67\ \text{m}^{-1}

Step 3 β€” combine.

W=βˆ’(0.054)(βˆ’6.67)=+0.36Β JW = -(0.054)(-6.67) = +0.36\ \text{J}

Why positive? Like charges repel, so outward is the direction the force pushes. A body moving the way the force pushes it always receives positive work β€” attraction moving inward and repulsion moving outward give the same verdict.

Problem 3 Β· Arc, Then Plunge β€” Work and Final Speed

Given: A 1000Β kg1000\ \text{kg} probe runs along a frictionless guide that first sweeps a quarter circle at fixed radius ri=3.0Γ—1011Β mr_i = 3.0\times10^{11}\ \text{m} about a star, then runs radially inward to rf=1.0Γ—1011Β mr_f = 1.0\times10^{11}\ \text{m}. The guide always pushes perpendicular to the motion, so it does no work. With Gmsm=2.4Γ—1023Β Jβ‹…mG m_s m = 2.4\times10^{23}\ \text{J}\cdot\text{m} and an initial speed vi=2.0Γ—104Β m/sv_i = 2.0\times10^{4}\ \text{m/s} β€” find the work done by gravity and the final speed.

Total work done by gravity?

Final speed?

βœ… Correct! The quarter circle contributes nothing, the plunge contributes 1.6Γ—1012Β J1.6\times10^{12}\ \text{J}, and the work-energy theorem turns that into a final speed of 6.0Γ—104Β m/s6.0\times10^{4}\ \text{m/s}.
❌ Check the work. The circular arc holds rr fixed, so dr=0dr = 0 and it contributes zero; only the change of radius counts, through Gmsm(1rfβˆ’1ri)G m_s m\left(\tfrac{1}{r_f} - \tfrac{1}{r_i}\right) with both reciprocals.
❌ Check the speed. The theorem gives Kf=Ki+WK_f = K_i + W β€” the probe was already moving, and K=12mv2K = \tfrac{1}{2}mv^2 carries the factor 12\tfrac{1}{2} on both ends.
Show solution

Step 1 β€” the quarter circle. On it rr never changes, so dr=0dr = 0 and dW=Fr dr=0dW = F_r\,dr = 0 at every point. Gravity stays perpendicular to the motion and does no work on that leg.

Step 2 β€” the radial plunge.

W=Gmsm(1rfβˆ’1ri)=(2.4Γ—1023)(11.0Γ—1011βˆ’13.0Γ—1011)W = G m_s m\left(\frac{1}{r_f} - \frac{1}{r_i}\right) = (2.4\times10^{23})\left(\frac{1}{1.0\times10^{11}} - \frac{1}{3.0\times10^{11}}\right) W=(2.4Γ—1023)(6.67Γ—10βˆ’12)=1.6Γ—1012Β JW = (2.4\times10^{23})(6.67\times10^{-12}) = 1.6\times10^{12}\ \text{J}

Step 3 β€” the work-energy theorem. The guide does no work, so gravity's work is the total:

Ki=12(1000)(2.0Γ—104)2=2.0Γ—1011Β JK_i = \tfrac{1}{2}(1000)(2.0\times10^{4})^2 = 2.0\times10^{11}\ \text{J} Kf=Ki+W=2.0Γ—1011+1.6Γ—1012=1.8Γ—1012Β JK_f = K_i + W = 2.0\times10^{11} + 1.6\times10^{12} = 1.8\times10^{12}\ \text{J}

Step 4 β€” back to a speed.

vf=2Kfm=2(1.8Γ—1012)1000=3.6Γ—109=6.0Γ—104Β m/sv_f = \sqrt{\frac{2K_f}{m}} = \sqrt{\frac{2(1.8\times10^{12})}{1000}} = \sqrt{3.6\times10^{9}} = 6.0\times10^{4}\ \text{m/s}

Dropping KiK_i would have given 5.7Γ—104Β m/s5.7\times10^{4}\ \text{m/s}, and forgetting the 12\tfrac{1}{2} in KK would have given 4.5Γ—104Β m/s4.5\times10^{4}\ \text{m/s}.

Problem 4 Β· A Force That Does Nothing At All

Given: At one instant a 2.0Β kg2.0\ \text{kg} drone has velocity vβƒ—=(6.0 i^βˆ’3.0 j^)Β m/s\vec{v} = (6.0\,\hat{i} - 3.0\,\hat{j})\ \text{m/s} while the net force on it is Fβƒ—=(4.0 i^+8.0 j^)Β N\vec{F} = (4.0\,\hat{i} + 8.0\,\hat{j})\ \text{N} β€” find the instantaneous power and say what is happening to the drone's speed.

Instantaneous power?

The drone's speed at this instant is…

βœ… Excellent! Fβƒ—β‹…vβƒ—=0\vec{F}\cdot\vec{v} = 0, so the force is perpendicular to the velocity: it bends the path hard while leaving the speed untouched.
❌ Watch the sign of the j^\hat{j} term. vy=βˆ’3.0Β m/sv_y = -3.0\ \text{m/s}, so Fyvy=(8.0)(βˆ’3.0)=βˆ’24Β WF_yv_y = (8.0)(-3.0) = -24\ \text{W} β€” it cancels the xx term instead of doubling it.
❌ That is ∣Fβƒ—βˆ£βˆ£vβƒ—βˆ£|\vec{F}||\vec{v}|. The scalar product carries a cos⁑θ\cos\theta: P=∣Fβƒ—βˆ£βˆ£vβƒ—βˆ£cos⁑θ=(8.94)(6.71)cos⁑90Β°=0P = |\vec{F}||\vec{v}|\cos\theta = (8.94)(6.71)\cos 90\degree = 0. Multiplying magnitudes alone assumes the vectors are parallel.
❌ Not quite. Use components: P=Fβƒ—β‹…vβƒ—=Fxvx+FyvyP = \vec{F}\cdot\vec{v} = F_xv_x + F_yv_y.
❌ Not quite. The theorem governs speed through energy, not through the size of the force: dK/dt=Fβƒ—β‹…vβƒ—dK/dt = \vec{F}\cdot\vec{v}, and here that rate is zero even though Fβƒ—\vec{F} is large and vβƒ—\vec{v} is nonzero.
Show solution

Step 1 β€” the power.

P=Fβƒ—β‹…vβƒ—=Fxvx+Fyvy=(4.0)(6.0)+(8.0)(βˆ’3.0)=24βˆ’24=0Β WP = \vec{F}\cdot\vec{v} = F_xv_x + F_yv_y = (4.0)(6.0) + (8.0)(-3.0) = 24 - 24 = 0\ \text{W}

Step 2 — read it as a rate of energy. Since dKdt=F⃗⋅v⃗=P=0\dfrac{dK}{dt} = \vec{F}\cdot\vec{v} = P = 0, the kinetic energy — and therefore the speed — is momentarily unchanging.

Step 3 β€” what the force is doing. Neither vector is zero: ∣vβƒ—βˆ£=36+9=6.71Β m/s|\vec{v}| = \sqrt{36+9} = 6.71\ \text{m/s} and ∣Fβƒ—βˆ£=16+64=8.94Β N|\vec{F}| = \sqrt{16+64} = 8.94\ \text{N}. Their scalar product vanishes only because they are perpendicular, so the whole force goes into turning the velocity:

aβŠ₯=∣Fβƒ—βˆ£m=8.942.0=4.5Β m/s2a_\perp = \frac{|\vec{F}|}{m} = \frac{8.94}{2.0} = 4.5\ \text{m/s}^2

This is the punchline of the three-dimensional theorem: work governs speed, not direction. A force can bend a path all day and never transfer a joule β€” which is exactly why gravity does zero work on a circular orbit.

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