1.2.20 · Physics › Newton's Laws & Dynamics
Intuition Badi picture (YEH idea KYUN exist karti hai)
Ek mass M apne aas-paas ke space mein "pahunchta" hai aur har doosre mass ko batata hai kis direction mein aur kitni force ke saath girna hai. Har baar naye test mass ke liye force recompute karne ki jagah, hum space ko hi ek quantity se describe karte hain: gravitational field intensity g . Yeh us choti test mass par lagni wali force per unit mass hai — yeh us location ki property hai, na ki wahan aane wale ki.
Definition Gravitational field intensity
Kisi point par gravitational field intensity g woh gravitational force per unit mass hai jo wahan rakhi gayi ek choti test mass m ko feel hoti hai:
g = m F
Units: N kg − 1 (equivalently m s − 2 ). Yeh ek vector hai, jo source mass ki taraf point karta hai.
"Per unit mass" KYUN? Kyunki test mass par force m ke proportional hoti hai. m se divide karne par visitor ka mass cancel ho jaata hai, aur ek aisi quantity bachti hai jo sirf source aur aap kahan khade hain par depend karti hai. Yahi ek field ka poora trick hai.
1/ r 2 specifically KYUN?
Field ko M se baahar failti lines ki tarah socho. Utni hi lines M ke around har sphere ko pierce karti hain. Ek sphere ka area 4 π r 2 hota hai, isliye line density (= field strength) 1/ r 2 ki tarah dilute hoti hai. Distance double karo → field quarter ho jaati hai. Yeh "sphere par failna" inverse-square law ka geometric core hai.
Worked example 1. Earth ki surface par field
M ⊕ = 5.97 × 1 0 24 kg , R ⊕ = 6.37 × 1 0 6 m .
g = R 2 GM = ( 6.37 × 1 0 6 ) 2 ( 6.67 × 1 0 − 11 ) ( 5.97 × 1 0 24 )
R kyun use karein? Surface par, Earth ke centre se aapki distance uski radius hai.
g = 4.06 × 1 0 13 3.98 × 1 0 14 ≈ 9.8 N kg − 1
Yeh jaana-pehchana 9.8 m s − 2 wapas milta hai — field intensity hi free-fall acceleration hai. YEH equal KYUN? Kyunki g = F / m aur F = ma ⇒ a = F / m = g .
Worked example 2. Twice the radius par field (altitude
= R )
Centre se r = 2 R par:
g ′ = ( 2 R ) 2 GM = 4 R 2 GM = 4 1 g surface ≈ 2.45 N kg − 1
1/4 KYUN? Inverse-square: distance ×2 → field ÷2 2 . Dhyan do ki humne scratch se recompute nahi kiya — humne ratio use kiya. (80/20: ratios 90% arithmetic bachate hain.)
Worked example 3. Earth aur Moon ke beech net field (vector addition)
Ek point par, Earth left mein g E = 2.0 × 1 0 − 3 se kheench rahi hai aur Moon right mein g M = 1.5 × 1 0 − 3 N/kg se kheench raha hai.
g net = g E − g M = 0.5 × 1 0 − 3 N kg − 1 toward Earth
Subtract KYUN? Fields vectors hain; opposite directions partially cancel hoti hain. Null point par g E = g M aur net field zero hoti hai.
Common mistake "Bhaari objects ek stronger field mein hote hain, isliye unka
g zyada hoga."
Sahi kyun lagta hai: bhaari cheezein zyada weightt karti hain, toh field bhi unke liye badi hogi.
Fix: Weight F = m g toh m ke saath badhta hai, lekin g = F / m mein m cancel ho jaata hai. Field source M aur distance r se set hoti hai, kabhi test mass se nahi. Ek feather aur ek brick ek hi point par same g feel karte hain.
Common mistake Centre se nahi, surface se radius use karna.
Sahi kyun lagta hai: "altitude" ground se measure hoti hai.
Fix: GM / r 2 mein r hamesha centre of mass M se measure hoti hai. Altitude h par, h nahi, r = R + h use karo.
g ko scalar treat karna aur sirf magnitudes add karna.
Sahi kyun lagta hai: numbers add karna easy hai.
Fix: g ek vector hai — direction ke saath add karo. Opposite fields subtract hoti hain; perpendicular ones ke liye Pythagoras use karo.
Recall Forecast-then-Verify: padhne se pehle predict karo
Agar M se apni distance triple karo, toh g ka kya hoga? → (forecast)
g ki units kya hain, aur do equivalent forms kyun hain?
Test mass final formula mein kyun nahi dikhti?
Answers: 1. g → g /9 (inverse-square, 3 2 ). 2. N kg − 1 = m s − 2 kyunki g free-fall acceleration ke barabar hota hai. 3. Yeh F / m mein cancel ho jaata hai; field source + location ki property hai.
Recall Feynman: ek 12-saal ke bache ko explain karo
Ek bahut badi magnetic ball socho (lekin weight ke liye, metal ke liye nahi). Yeh apne aas-paas invisible "kheenchne wali rays" banata hai. Paas mein, rays crowded hain aur zyada kheenchti hain; door mein yeh ek giant bubble par fail gayi hain, toh kaafi kam kheenchti hain. Yeh kheenchne ki strength hi field hai. Interesting part yeh hai: yeh ek marble aur ek bowling ball ko same strength per kilogram se kheenchti hai — sirf planet aur distance decide karte hain kitni strong hai, na ki kaun visit kar raha hai.
Mnemonic Formula yaad rakho
"Great Massive star, Radius Squared" → g = r 2 G M .
Aur 1/ r 2 falloff ke liye "Far = Faint, by the Square" .
Gravitational field intensity ki definition hai force per unit mass,
g = F / m Point/spherical mass M se distance r par g ka formula g = GM / r 2 , M ki taraf directed
Gravitational field intensity ki units N kg − 1 = m s − 2
g mein se test mass kyun cancel ho jaati hai?Force F ∝ m ; m se divide karne par sirf source-dependent quantity bachti hai
Distance r kahan se measure hoti hai? Source mass ke centre se, isliye altitude h par r = R + h
Distance 2 R par field surface value ki kitni fraction hogi? 1/4 (inverse-square, 2 2 )
Geometrically gravity inverse-square law kyun hai? Field lines sphere area 4 π r 2 ∝ r 2 par spread hoti hain
Field intensity aur free-fall acceleration ka relation Dono equal hain: a = F / m = g
Earth–Moon null point par net field zero (opposite fields magnitude mein equal hain)
r ^ ko M se door point karte hue field ka vector form
Newton law F = GMm - r squared
Definition g = F per unit m
Field lines over 4 pi r squared
Inverse-square 1 - r squared