1.2.19 · D2 · HinglishNewton's Laws & Dynamics

Visual walkthroughNewton's law of gravitation — universal, action at distance

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1.2.19 · D2 · Physics › Newton's Laws & Dynamics › Newton's law of gravitation — universal, action at distance

Hum sirf wahi words use karte hain jo aap pehle se jaante ho: stuff (matter), pull, distance, aur area. Neeche har symbol theek usi waqt introduce kiya jaata hai jab uski zaroorat hoti hai, ek step pehle nahi.


Step 1 — Do lumps of stuff, ek invisible pull

KYA. Do objects ko empty space mein rakho. Har ek mein kitna "stuff" hai usse uski mass kaho. Pehli mass ko aur doosri ko likho. Chhota "1" aur "2" sirf name-tags hain — yeh batate hain ki hum kaun sa lump mean kar rahe hain, bas itna hi.

KYUN. Kisi bhi formula se pehle, hum cast of characters pe agree karna chahte hain. Poora law in do lumps aur unke beech ki empty gap ke baare mein ek sentence hai. Woh gap — ek ke centre se doosre ke centre tak ki straight-line distance — hum ise naam dete hain (range ke liye).

PICTURE. Figure dekho: do orange dots, unke centres ko join karta hua ek dotted teal line jis par likha hai, aur do arrows (har lump par ek) us line ke saath, ek doosre ki taraf point karte hue. Arrows woh pull hai. Dhyan do ki woh exactly joining line par lie karte hain — kabhi sideways nahi. Yeh gravity ka pehla fact hai: pull hamesha line of centres ke along hoti hai.

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

Step 2 — Zyada stuff matlab zyada pull

KYA. Poochho: agar main lump 1 mein stuff double kar doon, toh pull ka kya hoga? Lump 1 ko do identical half-lumps ki tarah socho jo ek saath glued hain. Har half akele lump 2 ko pull karta hai. Do halves side by side double itna pull karte hain. Toh double karne se force double ho jaati hai.

KYUN. Matter ka har chhota sa tukda apna pulling karta hai, aur pulls add up hote hain. Double matter = double pulling bits = double pull. Symbols mein hum yeh likhte hain Wiggly sign ka matlab hai "ke saath saath badhta hai" — agar right side double ho, toh bhi double hoga. Yahan pull ka size (magnitude) hai.

Yehi argument lump 2 ke liye bhi kaam karta hai. double karne se bhi pull double hoti hai, toh . Dono ko saath mein rakhke:

Product kyun, sum kyun nahi? Figure yeh dikhata hai: lump 1 ki copies stack karna force ko lump 1 ki side se multiply karta hai, aur independently lump 2 ko stack karna doosri side se multiply karta hai. Do independent doublings chaar-guna pull par multiply hote hain — yeh exactly wahi hai jo deta hai (), jabki sirf add karta. (Parent note mein 3rd-law symmetry woh deeper reason hai ki dono masses ek hi tarah se enter karni chahiye.)

PICTURE. Left panel: ek lump 1 → lump 2 ki taraf pull-lines ka ek bundle. Right panel: lump 1 doubled → pull-lines ka bundle visibly double ho gaya. Teal lines gino: woh stuff ke saath scale karte hain.

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

Step 3 — Pull kyun fade hoti hai, aur ki tarah kyun

KYA. Ab lumps ko alag karo aur poochho ki pull kitni jaldi weak hoti hai. Socho ki pull lump 1 se ek fixed number ki straight "influence lines" ki tarah har direction mein bahar spray ho rahi hai — jaise kisi point se spray ki gayi paint.

KYUN. Woh lines lump 1 ke centre par ek imaginary sphere ki surface par spread ho jaati hain. Radius ke sphere ki surface area hoti hai Yahan sirf ek fixed number hai () jo spheres ke saath aata hai; ka matlab hai . Lines ka wahi fixed spray ab is area par smear ho gaya hai. Toh lines ka concentration — woh strength jo aap feel karte ho — yeh hai

Squared kyun, sirf kyun nahi? Kyunki sphere ki skin ke saath badhti hai, ke saath nahi. Double door jao aur wahi lines guna area cover karti hain, toh pull chaar guna kamzor hoti hai — do guna nahi. Yahi inverse-square ka matlab hai.

PICTURE. Do nested spheres. Paas wala (chhota radius) mein lines tight packed hain — strong pull. Door wala (double radius) mein wahi lines 4× skin par thin pheli hain — weak pull. Shaded patch dekho: same number of lines, chaar guna area.

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

Step 4 — "" ko "" mein badalna constant ke saath

KYA. Symbol humein law ki shape batata hai lekin scale nahi. Real numbers (force ke newtons) paane ke liye, hum ek fixed number se multiply karte hain, jise kehte hain:

KYUN. Nature humein nahi batata ki ek kilogram ki pull kitni strong hai — hum ise measure karna padta hai. Henry Cavendish ne exactly yahi kiya do masses ko ek delicate rod ko gently twist karte hue dekh ke. Usne jo number paaya woh tiny hai: Woh (ek decimal point jiske baad das zeros) isiliye hai ki gravity everyday objects ke beech itni weak lagti hai — poora formula ek almost-nothing number se multiply ho jaata hai.

Term-by-term, theek wahan jahan har ek live karta hai:

PICTURE. Ek "dial" figure: relationship ek fixed curve shape hai; woh knob hai jo uski height set karta hai. Bada → tall curve (strong gravity); real, tiny → ek curve jo axis ke paas almost flat press ho gayi hai. Shape fixed hai; sirf ise scale karta hai.

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

Step 5 — Pull ko direction dena (ise vector banana)

KYA. Ab tak sirf ek size hai — newtons ki ek number. Lekin ek pull ki direction bhi hoti hai. Hum length 1 ka ek arrow lagate hain jo lump 1 se seedha lump 2 ki taraf point karta hai, aur ise naam dete hain (chhota hat "^" matlab "length exactly one — ek pure direction, koi size nahi"). Tab lump 1 par full pull hai

KYUN. ke upar arrow kehta hai "yeh ek full arrow hai, size aur direction." Size ko unit arrow se multiply karna sahi size par sahi direction glue kar deta hai. Plus sign ke saath, jo doosre mass ki taraf point karta hai, wahi gravity ko attractive banata hai — force usi direction mein point karti hai jis taraf arrow point karta hai, yaani lump 2 ki taraf.

Sirf number kyun nahi chhod dete? Kyunki agar koi teesra lump aata, toh humein pulls ko add karna padta, aur aap arrows ko sahi se tabhi add kar sakte ho jab har ek apni direction carry kare. Vector form future-proof hai.

PICTURE. Joining line jis par chhota unit arrow drawn hai (length exactly 1), phir full force arrow same line par drawn hai lekin force ki sachi size tak scaled. Same direction; alag length.

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

Step 6 — Edge case: extremes par kya hota hai?

KYA. Ek achha law corners mein bhi sensibly behave karta hai. Teen check karo:

  1. (lumps infinitely door). Neeche wala explode karta hai, toh . Gravity kabhi exactly zero nahi hoti kisi finite distance par — woh sirf fade hoti hai — lekin woh tezi se khatam hoti hai.
  2. (lumps merge). Neeche wala zero ho jaata hai, toh formula chilla-ta hai. Yeh ek warning sign hai: law point masses ke liye likha gaya hai (ya spheres ke liye centre-to-centre). Real objects ka size hota hai, toh aap actually nahi lagate — ek real planet ke liye sabse meaningful uska radius hai (shell theorem guarantee karta hai ki ek solid sphere aise act karta hai jaise uska saara stuff uske centre par ho).
  3. Ek mass zero (). Upar wala ho jaata hai, toh . Koi stuff nahi, koi pull nahi — bilkul sahi.

Kyun matter karta hai. Yahi checks hain jinse aap ek formula trust karte ho: jab kuch pull karne ko nahi hota toh zero dena chahiye, aur jis ek jagah ise use karna allowed nahi wahan infinity flag karna chahiye. Everyday bhi is curve par hi hai — woh simply ki value hai jo (Earth's surface) par evaluate ki gayi hai:

PICTURE. Poora -versus- curve: ke paas ek steep wall (forbidden ), ek smooth downhill jo ki taraf flatten hoti jaati hai jaise badhta hai, aur par ek marker drop kiya gaya hai jo dikhata hai ki "surface gravity " isi curve par kahan baithti hai.

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

Ek-picture summary

Upar ki sab cheez ek single labelled diagram mein collapse ho jaati hai: do masses, joining line , andar ki taraf attraction arrows, aur assembled formula jisme har piece us jagah se match karne ke liye coloured hai jahan se woh aaya — Step 2 se (stuff), Step 3 se (sphere par spreading), Step 4 se (measured scale), arrow Step 5 se (direction).

Figure — Newton's law of gravitation — universal, action at distance
Recall Feynman retelling — poora walkthrough plain words mein

Do blobs of stuff empty space mein baithe hain (Step 1). Har blob actually tiny pulling grains ki ek crowd hai, toh zyada stuff proportionally zyada pull karta hai — aur kyunki dono blobs independently apni pull multiply karte hain, force product follow karta hai, sum nahi (Step 2). Ab socho ki woh pull ek point se paint ki tarah bahar spray ho rahi hai; woh ek badhte sphere ki skin par smear ho jaati hai jiska area hai, toh double door jaane ka matlab hai chaar guna thinner matlab chaar guna weaker — inverse-square (Step 3). Isse humein law ki shape milti hai, aur ek measured knob uski sachi, absurdly-tiny height set karta hai (Step 4). Ek arrow blob-to-blob point karta glue karo aur yeh ek proper pulling vector ban jaata hai (Step 5). Aakhir mein hum corners sanity-check karte hain: door jaane par pull kuch nahi ho jaati, zero separation par formula (sahi tarike se) jawab dene se mana kar deta hai kyunki wahan point-mass thinking toot jaati hai, aur koi stuff nahi matlab koi pull nahi — aur everyday bas yahi curve hai jo Earth's surface par read ki gayi hai (Step 6).

Recall Khud rebuild karo (answers cover karo)

Product kyun, sum kyun nahi ::: Do independent doublings multiply karte hain; aur dono apni apni side par force scale karte hain. kyun, kyun nahi ::: Pull sphere ki skin par spread hoti hai, area ; area ke saath badhta hai. kya karta hai ::: Fixed proportional shape ki sachi scale (height) set karta hai; Cavendish ne measure kiya. mein hat ka matlab kya hai ::: Ek pure direction — length exactly one ka ek arrow, mass 1 se mass 2 ki taraf point karta hua. par kya toot jaata hai ::: Formula infinity deta hai; yeh point masses / centre-to-centre ke liye bana hai, toh kisi real body ke liye kabhi use mat karo.


Connections

  • Parent topic — woh full statement jise yeh page derive karta hai.
  • Newton's Third Law — woh deeper reason ki dono masses symmetrically enter karti hain (Step 2).
  • Shell Theorem — kyun centre-to-centre hai aur kyun forbidden hai (Step 6).
  • Gravitational Field & Potential — woh field view jo vector form se bahar nikalti hai (Step 5).
  • Weight vs Mass seedha Step 6 curve se padha gaya.
  • Circular Motion & Centripetal Force & Kepler's Laws — jahan yeh force apna orbital kaam karta hai.
  • General Relativity — cosmic scale par "instant" arrow ki jagah kya aata hai.