1.2.19Newton's Laws & Dynamics

Newton's law of gravitation — universal, action at distance

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WHY does such a law exist?

WHY does the force depend on both masses? By Newton's 3rd law, the pull of body A on B equals the pull of B on A. If the force depended on m1m_1 only, the two pulls couldn't be equal for unequal masses. The symmetric way to make F12=F21F_{12}=F_{21} is to make it depend on the product m1m2m_1 m_2.

WHY inverse-square? Picture the gravitational "influence" spreading out from a point source over the surface of an expanding sphere of radius rr. The surface area is 4πr24\pi r^2. The same total influence is diluted over a larger area, so its intensity 1/r2\propto 1/r^2. This is the same geometry behind light intensity and sound.


Building the formula from scratch

Step 1 — Force grows with each mass. Why? More matter = more "pulling stuff." Doubling m1m_1 doubles every attracting bit, so Fm1F \propto m_1. Same for m2m_2. Together: Fm1m2F \propto m_1 m_2

Step 2 — Force dilutes geometrically. Why? Influence spreads over a sphere of area 4πr24\pi r^2: F1r2F \propto \frac{1}{r^2}

Step 3 — Combine and insert a constant. Why a constant? Proportionalities need a unit-fixing number found by experiment (Cavendish): F=Gm1m2r2\boxed{F = \frac{G\, m_1 m_2}{r^2}}

Step 4 — Make it a vector (direction matters). Force on mass 1 due to mass 2 points from 1 toward 2. Let r^12\hat{r}_{12} point from 1 to 2: F12=+Gm1m2r2r^12\vec{F}_{12} = +\frac{G m_1 m_2}{r^2}\,\hat{r}_{12} The ++ with r^12\hat r_{12} pointing toward the other mass encodes attraction.

Figure — Newton's law of gravitation — universal, action at distance

What is "action at a distance"?

Field reformulation (the 80/20 upgrade): g=Fmtest=GMr2 (toward M)\vec g = \frac{\vec F}{m_{\text{test}}} = \frac{GM}{r^2}\ (\text{toward } M) Now the field exists in space; a test mass just samples it locally. This kills the "instant action" worry conceptually.


Worked Examples


Common Mistakes (Steel-manned)


Active Recall

Recall Quick self-test (cover answers)
  • Why product m1m2m_1m_2 and not m1+m2m_1+m_2? → Newton's 3rd law symmetry.
  • Why inverse-square? → Influence diluted over sphere area 4πr24\pi r^2.
  • Why do all objects fall at the same gg? → mass cancels in a=GM/r2a=GM/r^2.
  • What is "action at a distance"? → force across empty space, no contact.
  • Difference between gg and GG? → GG universal constant; gg local field strength.
Recall Feynman: explain to a 12-year-old

Imagine everything that has stuff in it is a tiny magnet that only pulls (never pushes). Big things pull harder. And the pull gets weaker fast the farther you move away — go twice as far, the pull becomes four times weaker. The Earth is so huge that its pull keeps you stuck to the ground, keeps the Moon circling us, and keeps Earth circling the Sun. Spookiest part: nothing touches — the pull just reaches across empty space, like an invisible rope you can't see or cut.


Connections

  • Newton's Third Law — gives the m1m2m_1m_2 symmetry and equal-and-opposite pulls.
  • Gravitational Field & Potential — the field cure for action-at-a-distance.
  • Kepler's Laws — emerge from inverse-square gravity + circular/elliptical motion.
  • Circular Motion & Centripetal Force — used in the "falling Moon" check.
  • Shell Theorem — why rr is centre-to-centre for spheres.
  • General Relativity — replaces instant action with curved spacetime at speed cc.
  • Weight vs MassW=mgW=mg, and g=GM/R2g=GM/R^2.
Newton's law of gravitation formula?
F=Gm1m2r2F = \dfrac{G m_1 m_2}{r^2}, attractive, along the line joining the masses.
Why does FF depend on the product of masses, not sum?
To satisfy Newton's 3rd law: the symmetric form m1m2m_1m_2 makes F12=F21F_{12}=F_{21} automatically.
Why inverse-square and not inverse-rr?
The influence spreads over a sphere of surface area 4πr24\pi r^2, so intensity falls as 1/r21/r^2.
Value and units of GG?
6.674×1011 Nm2kg26.674\times10^{-11}\ \mathrm{N\,m^2\,kg^{-2}}, universal everywhere/everytime.
Difference between gg and GG?
GG is the universal constant; g=GM/r2g=GM/r^2 is the local field strength (varies with planet and altitude).
Why do all objects fall with the same acceleration?
a=F/m=GM/r2a=F/m=GM/r^2 — the falling object's mass cancels.
Derive gg at Earth's surface.
mg=GMm/R2g=GM/R29.8mg=GM_\oplus m/R_\oplus^2 \Rightarrow g=GM_\oplus/R_\oplus^2\approx 9.8 m/s².
What is "action at a distance"?
Force exerted across empty space with no contact and (in Newton's model) instantaneously.
For two spheres, what is rr?
Distance between their centres (shell theorem).
What was Newton's "falling Moon" argument?
Moon's orbital acceleration g/602\approx g/60^2 matches 4π2r/T24\pi^2r/T^2, proving the apple-force = Moon-force.

Concept Map

leads to

forces symmetric

dilution

combine

combine

fixes constant

inserted into

is

vector form

acts via

means

Newton's insight: same force everywhere

Universal Gravitation

Newton's 3rd law

F depends on product m1 m2

Influence over sphere 4 pi r squared

F proportional to 1 over r squared

F equals G m1 m2 over r squared

Cavendish experiment

G gravitational constant

Always attractive

F12 along line joining masses

Action at a distance

No contact, instantaneous across space

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, Newton ka gravitation ka law bolta hai ki universe ki har cheez har doosri cheez ko kheechti hai — sirf attract karti hai, push kabhi nahi. Force ka formula hai F=Gm1m2/r2F = G m_1 m_2 / r^2. Iska matlab: dono masses jitne bade, force utna zyada (isliye product m1m2m_1 m_2), aur distance jitna zyada, force utna kam — aur woh bhi square ke hisaab se. Yaani distance double karo to force ek-chauthai (1/4) ho jaata hai. Yeh "square" isliye aata hai kyunki gravity ka asar ek sphere par failta hai jiska area 4πr24\pi r^2 hota hai.

"Universal" word ka matlab — yahi rule apple ke girne par bhi laagu hota hai aur Moon ke Earth ke around ghoomne par bhi. Newton ne yahi prove kiya: jis force se apple girti hai, usi force se Moon Earth ke around tika hua hai. Bas Moon itni tezi se side me move karta hai ki woh girte-girte Earth ko miss karta rehta hai — isi ko orbit kehte hain.

"Action at a distance" ka matlab — koi rassi nahi, koi touch nahi, phir bhi force lag raha hai khaali space ke aar-paar. Yeh baat khud Newton ko bhi ajeeb lagti thi. Modern physics isko field aur curved spacetime (General Relativity) se samjhati hai, par exam aur normal problems ke liye Newton ka law bilkul perfect chalta hai.

Sabse important trick: g=GM/R2g = GM/R^2. Yahaan girne wali cheez ka mass cancel ho jaata hai, isliye bhaari ya halki — sab ek hi acceleration (9.89.8 m/s²) se girte hain. Aur dhyaan rakho — GG universal constant hai (har jagah same), jabki gg planet aur height ke saath badalta hai. Dono ko confuse mat karna!

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Connections