Newton's Third Law — Question 7

Section 5-7 · Physics pages 744–745

Question 7 Earth responds to the same mutual gravitational force A 2 kg object and an idealized Earth of mass 6 × 1024 kg exert equal gravitational forces of 20 N on one another. Ignore all other forces for this comparison. Earth: 6 × 1024 kg object: 2 kg 20 N 20 N The gravitational forces act on different bodies and point toward one another. (a) Find each acceleration magnitude. (b) Find their ratio. (c) Explain why treating Earth as nearly stationary does not deny the third law.
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Question 7 - Solution Earth responds to the same mutual gravitational force Earth: 6 × 1024 kg object: 2 kg 20 N 20 N (a) Apply the same force to different masses. ao = 20/2 = 10, aE = 20 6 × 1024 = 3.333 × 10−24 m/s2 The object has acceleration 20/2 = 10 m/s2. Earth has acceleration 20/(6 × 1024) ≈3.333 × 10−24 m/s2, toward the object. (b) Compare responses. ao aE = ME mo = 6 × 1024 2 = 3 × 1024 The object-to-Earth acceleration ratio is 3 × 1024, equal to the inverse mass ratio. (c) State the approximation. Fo→E = FE→o = 20 N (magnitudes), aE ≪ao Earth’s enormous inertia makes its response negligible at ordinary precision. Approximating its motion as fixed concerns the size of its acceleration, not the existence or magnitude of the force on it. These are supplied idealized values, not a local-field measurement.

Question 7

Earth responds to the same mutual gravitational force

A 2 kg object and an idealized Earth of mass 6×10246\times10^{24} kg exert equal gravitational forces of 20 N on one another. Ignore all other forces for this comparison.

Diagram shown in the original SVG worksheet.

  1. Find each acceleration magnitude.

  2. Find their ratio.

  3. Explain why treating Earth as nearly stationary does not deny the third law.

Question 7 - Solution

Earth responds to the same mutual gravitational force

Diagram shown in the original SVG worksheet.

(a) Apply the same force to different masses.

ao=20/2=10,aE=206×1024=3.333×10−24m/s2a_o=20/2=10,\quad\boxed{a_E=\frac{20}{6\times10^{24}}=3.333\times10^{-24}}\quad\mathrm{m/s^2} The object has acceleration 20/2=1020/2=10 m/s2^2. Earth has acceleration 20/(6×1024)≈3.333×10−2420/(6\times10^{24})\approx3.333\times10^{-24} m/s2^2, toward the object.

(b) Compare responses.

aoaE=MEmo=6×10242=3×1024\frac{a_o}{a_E}=\frac{M_E}{m_o}=\frac{6\times10^{24}}2=3\times10^{24} The object-to-Earth acceleration ratio is 3×10243\times10^{24}, equal to the inverse mass ratio.

(c) State the approximation.

Fo→E=FE→o=20N(magnitudes),aE≪aoF_{o\to E}=F_{E\to o}=20\,\mathrm N\quad\text{(magnitudes)},\qquad a_E\ll a_o Earth’s enormous inertia makes its response negligible at ordinary precision. Approximating its motion as fixed concerns the size of its acceleration, not the existence or magnitude of the force on it. These are supplied idealized values, not a local-field measurement.