1.2.14 · D3 · Physics › Newton's Laws & Dynamics › Rotating frames — centrifugal force, Coriolis force
Intuition Yeh page kis liye hai
Foundations ne humein do fictitious-force formulas diye. Visual walkthrough ne dikhaya ki woh dikhte kaise hain. Ab hum har tarah ke case ke through grind karte hain jo ek problem tumhare saamne rakh sakti hai — cross product ke har sign ke liye, carousel ke har quadrant ke liye, degenerate "standing still" case ke liye, limiting "far from axis" case ke liye, aur ek real weather problem ke liye. Jab tum finish karo, koi bhi exam scenario naya nahi lagna chahiye.
Kuch bhi shuru karne se pehle, do tools ko fresh tarike se anchor karte hain jo hum baar baar use karte rahe, seedhe saadhe words mein:
Is topic ka har problem neeche diye gaye cells mein se ek hai (ya blend). Har worked example us cell ke saath tagged hai jo woh cover karta hai.
Cell
Case class
Covered by
C1
Centrifugal, position-only, standard magnitude
Ex 1
C2
Coriolis, velocity radially outward (z ^ × r ^ ka sign)
Ex 2
C3
Coriolis, velocity tangential (z ^ × θ ^ ka sign) — opposite handedness
Ex 3
C4
Degenerate : frame mein object at rest (v rot = 0 ) → Coriolis vanishes
Ex 4
C5
Dono forces ek saath , vectors ke roop mein add karna, aur sizes compare karna
Ex 5
C6
Limiting behaviour : axis par (r ⊥ → 0 ) aur bahut door
Ex 6
C7
Real-world word problem : Earth, hemisphere sign, time ke saath accumulation
Ex 7
C8
Exam twist : velocity axis ke along (v ∥ ω ) → Coriolis zero hai
Ex 8
Hum ek convention fix karte hain jo poore note mein use hogi: spin axis z ^ hai (turntable se upar bahar ki taraf point karta hua), ω = ω z ^ jahan ω > 0 matlab upar se dekha jaye toh counter-clockwise . Flat turntable par hum polar directions use karte hain: r ^ (centre se seedha baahir) aur θ ^ (spin direction mein r ^ se 90° aage). Yeh right-hand rules follow karte hain:
z ^ × r ^ = θ ^ , z ^ × θ ^ = − r ^ , r ^ × θ ^ = z ^ .
Figure dekho: r ^ red outward arrow hai, θ ^ green sideways arrow (spin mein 90° ghuma hua), z ^ page se bahar blue. Right-hand ki ungliyan z ^ se r ^ ki taraf curl karo aur thumb θ ^ par land karta hai — yahi poori wajah hai ki neeche ke answers apna sign kyun lete hain.
Worked example Carousel par baithna
Tum r ⊥ = 2 m par merry-go-round ke centre se baith gaye ho jo ω = 1.5 rad/s par spin kar raha hai. Tumhara mass m = 60 kg hai. Tumhe kaisa outward centrifugal force feel hota hai, aur seat ko kaunsi real force supply karni padegi?
Forecast: bada radius ya zyada fast spin → bada fling. Aage padhne se pehle number guess karo.
Step 1 — sahi tool chuno. Seat ke relative koi velocity mention nahi hai (tum still baithe ho), toh sirf centrifugal matter karta hai. Iska magnitude position-only hai:
F cf = m ω 2 r ⊥ .
Yeh step kyun? Coriolis ko v rot = 0 chahiye; tum frame mein rest par ho, toh yeh bilkul drop ho jaata hai (Ex 4 dekho). Sirf centrifugal bachta hai.
Step 2 — plug in karo.
F cf = 60 × ( 1.5 ) 2 × 2 = 60 × 2.25 × 2 = 270 N .
Yeh step kyun? Direct substitution; units kg ⋅ ( rad/s ) 2 ⋅ m = kg⋅m/s 2 = N (radians dimensionless hote hain).
Step 3 — real force interpret karo. Inertial frame mein koi outward force nahi hai. Seat tumhe 270 N se andar ki taraf push karti hai — yahi centripetal force m ω 2 r ⊥ hai jo tumhe circle mein rakhti hai. "Centrifugal" force bas yahi hai ki wahi situation andar se kaisi lagti hai .
Verify: 60 ⋅ 2.25 = 135 ; 135 ⋅ 2 = 270 N . ✓ Ek person jo ek brisk carousel par ~270 N (~27 kg-weight) sideways feel karta hai, yeh realistic hai.
Worked example Baahir ki taraf throw karna
Usi carousel par (ω = 1.5 z ^ ) tum ek ball seedha baahir (r ^ ) ki taraf v = 5 m/s par throw karte ho, ball mass m = 0.2 kg . Coriolis force (size aur direction) nikalo.
Forecast: ball kis taraf curve karti dikhegi — spin ke saath ya uske against?
Step 1 — velocity ko frame directions mein likho. v rot = 5 r ^ .
Yeh step kyun? Coriolis sirf object ki velocity se matlab rakhta hai jaise rotating frame ke andar measure ki gayi hai , aur radial-out exactly r ^ hai.
Step 2 — cross product banao.
F Cor = − 2 m ω × v rot = − 2 ( 0.2 ) ( 1.5 ) ( z ^ × 5 r ^ ) .
z ^ × r ^ = θ ^ use karke:
F Cor = − 2 ( 0.2 ) ( 1.5 ) ( 5 ) θ ^ = − 3.0 θ ^ N .
Yeh step kyun? Cross product velocity direction ko 90° rotate karta hai, "outward" ko "sideways" mein badal deta hai. Minus sign phir ise − θ ^ par flip kar deta hai: spin direction ke opposite .
Step 3 — picture karo. Rider ki seat se ball spin ke against peeche ki taraf mur jaati hai. Baahir se, ball seedha udti hai; rider (aur turntable) uske neeche rotate karta hai.
Verify: 2 ⋅ 0.2 ⋅ 1.5 ⋅ 5 = 3.0 N . ✓ Direction − θ ^ r ^ ke perpendicular hai, toh F Cor ⋅ v rot = 0 — koi work nahi, jaisa hona chahiye.
Worked example Spin ke saath sideways move karna
Wahi carousel. Ab ek mouse tangentially, spin direction mein (+ θ ^ ) v = 4 m/s par daudta hai, mass m = 0.1 kg . Coriolis force?
Forecast: pichhli baar radial motion ne sideways push kiya. Tangential motion… kahan push karegi?
Step 1 — frame mein velocity. v rot = 4 θ ^ .
Yeh step kyun? Spin ke along daudna matlab velocity θ ^ ki taraf point karti hai.
Step 2 — doosri handedness ke saath cross product. z ^ × θ ^ = − r ^ use karo:
F Cor = − 2 ( 0.1 ) ( 1.5 ) ( z ^ × 4 θ ^ ) = − 2 ( 0.1 ) ( 1.5 ) ( 4 ) ( − r ^ ) = + 1.2 r ^ N .
Yeh step kyun? Yeh matrix mein doosra sign case hai. Tangential motion ek radial Coriolis push produce karta hai — yahan outward (+ r ^ ) kyunki mouse spin ke saath move kar raha hai, effectively apni circling speed up kar raha hai aur frame jo provide karta hai usse zyada inward force ki zaroorat hai.
Step 3 — direction reverse karo, sign flip karo (C3 ki sanity). Agar mouse spin ke against daudta (− θ ^ ) toh answer − 1.2 r ^ ho jaata hai — inward. Coriolis hamesha v ke saath sign flip karta hai.
Verify: 2 ⋅ 0.1 ⋅ 1.5 ⋅ 4 = 1.2 N , direction r ^ . ✓ θ ^ ke perpendicular → koi work nahi.
Worked example Khade rehna
Ek 70 kg banda carousel par r ⊥ = 3 m par khada rehta hai , ω = 1.5 rad/s . Dono fictitious forces do.
Forecast: kya koi Coriolis hota hai jab tum move nahi karte?
Step 1 — Coriolis. v rot = 0 , toh
F Cor = − 2 m ω × 0 = 0.
Yeh step kyun? Coriolis velocity frame ke andar ke proportional hai. Zero velocity ⇒ zero Coriolis. Yeh sabse common student error hai jo bachni chahiye.
Step 2 — Centrifugal abhi bhi act karta hai.
F cf = m ω 2 r ⊥ = 70 × ( 1.5 ) 2 × 3 = 70 × 2.25 × 3 = 472.5 N , outward .
Yeh step kyun? Centrifugal sirf position par depend karta hai, velocity par nahi — jab tak tum spinning platform par baithe ho tab tak yeh kabhi off nahi hota.
Verify: 70 ⋅ 2.25 = 157.5 ; 157.5 ⋅ 3 = 472.5 N . ✓ Coriolis = 0 , centrifugal = 0 — exactly degenerate cell.
Worked example Kaun dominate karta hai?
Ek 0.5 kg puck radially outward v = 6 m/s par slide karta hai jab woh r ⊥ = 1 m par hai, ek turntable par jahan ω = 2 rad/s hai. Dono forces aur unka vector sum nikalo.
Forecast: 1 m aur 2 rad/s par, kya centrifugal ya Coriolis yahan bada hai?
Step 1 — centrifugal (radial, outward, + r ^ ).
F cf = m ω 2 r ⊥ = 0.5 × ( 2 ) 2 × 1 = 2.0 N ( + r ^ ) .
Yeh step kyun? Position-based, hamesha r ^ ke along outward.
Step 2 — Coriolis (radial-out velocity → tangential force). v rot = 6 r ^ aur z ^ × r ^ = θ ^ ke saath:
F Cor = − 2 ( 0.5 ) ( 2 ) ( 6 ) θ ^ = − 12 θ ^ N .
Yeh step kyun? Ex 2 jaisi C2 machinery; yahan number bahut bada hai kyunki ω aur v large hain.
Step 3 — perpendicular vectors ki tarah add karo. + 2.0 r ^ aur − 12 θ ^ right angles par hain, toh
∣ F total ∣ = 2. 0 2 + 1 2 2 = 4 + 144 = 148 ≈ 12.17 N .
Yeh step kyun? r ^ ⊥ θ ^ , toh Pythagoras inhe combine karta hai. Coriolis dominate karta hai kyunki motion yahan fast hai.
Verify: 2 ⋅ 0.5 ⋅ 2 ⋅ 6 = 12 ; 4 + 144 = 148 ≈ 12.166 . ✓ Units sab N.
Worked example Formula ki edges
Ek bug ek turntable par ω = 3 rad/s ke saath radially outward v = 1 m/s par crawl karta hai, mass m = 0.01 kg . Forces evaluate karo (i) exactly axis par r ⊥ = 0 aur (ii) r ⊥ = 10 m par bahut door.
Forecast: centre par kaun si force disappear hoti hai, aur kaun si dono jagah same rehti hai?
Step 1 — centrifugal at r ⊥ = 0 .
F cf = m ω 2 ⋅ 0 = 0.
Yeh step kyun? Centrifugal ∝ r ⊥ hai: bilkul axis par koi outward direction nahi hai, toh yeh vanish ho jaata hai. Yeh "on the axis" limiting cell hai.
Step 2 — centrifugal at r ⊥ = 10 m .
F cf = 0.01 × 9 × 10 = 0.9 N .
Yeh step kyun? Centrifugal distance ke saath linearly grow karta hai — bahut door par yeh chhote mass ke liye bhi bada ho sakta hai.
Step 3 — dono jagah Coriolis.
F Cor = 2 mω v = 2 ( 0.01 ) ( 3 ) ( 1 ) = 0.06 N ( same at r ⊥ = 0 aur 10 m ) .
Yeh step kyun? Coriolis mein koi r ⊥ nahi hai — yeh velocity par depend karta hai, position par nahi. Toh jab bug baahir move karta hai tab bhi yeh unchanged rehta hai. Yahi contrast (centrifugal grow karta hai, Coriolis constant) is cell ka poora point hai.
Verify: 0.01 ⋅ 9 ⋅ 10 = 0.9 N ; 2 ⋅ 0.01 ⋅ 3 ⋅ 1 = 0.06 N ; axis par centrifugal = 0 . ✓
Worked example Northern Hemisphere ke storms counter-clockwise kyun spin karte hain
Hawa ek low-pressure centre ki taraf v = 10 m/s par flow karti hai. Earth ki spin rate ω ⊕ = 7.3 × 1 0 − 5 rad/s hai. ω ka local vertical component lo taaki effective ω Northern Hemisphere mein zameen se upar point kare. Coriolis acceleration nikalo aur rotation ka sense explain karo. (Dekho Coriolis Effect in Weather .)
Forecast: aata hua air apni left mein mudta hai ya right mein?
Step 1 — Coriolis acceleration magnitude.
a Cor = 2 ω ⊕ v = 2 ( 7.3 × 1 0 − 5 ) ( 10 ) = 1.46 × 1 0 − 3 m/s 2 .
Yeh step kyun? Hum per-mass effect (acceleration) chahte hain, toh force formula ko m se divide karo: a Cor = 2 ω v . Yeh per second bahut chhota hai.
Step 2 — direction. ω up aur inflow velocity horizontal ke saath, − 2 ω × v air ko uski right ki taraf deflect karta hai. Right-deflected inflow incoming streams ko centre ke around ek counter-clockwise swirl mein curl kar deta hai.
Yeh step kyun? z ^ × v (up × horizontal) par right-hand rule ek leftward vector deta hai; extra minus ise motion ki right side par flip kar deta hai.
Step 3 — "tiny" kyun phir bhi win karta hai. L = 100 km = 1 0 5 m distance par hawa t = L / v = 1 0 5 /10 = 1 0 4 s (~2.8 hours) travel karti hai. Sideways speed jo build hoti hai:
Δ v = a Cor t = 1.46 × 1 0 − 3 × 1 0 4 = 14.6 m/s ,
jo inflow ke comparable hai. Yeh step kyun? Coriolis locally weak hai lekin large distances aur long times par accumulate hota hai — yahi Coriolis Effect in Weather aur Foucault Pendulum ke peeche ka 80/20 idea hai.
Verify: 2 ⋅ 7.3 × 1 0 − 5 ⋅ 10 = 1.46 × 1 0 − 3 ; 1.46 × 1 0 − 3 ⋅ 1 0 4 = 14.6 m/s . ✓
Worked example Trap question
Ek rocket seedha rotation axis ke along upar move karta hai, v rot = v z ^ jahan v = 200 m/s , ek platform par jahan ω = 0.8 z ^ , mass m = 50 kg , abhi r ⊥ = 0 par. Coriolis force?
Forecast: yeh fast move kar raha hai — surely Coriolis bahut bada hai?
Step 1 — parallel vectors ka cross product.
F Cor = − 2 m ω × v rot = − 2 ( 50 ) ( 0.8 ) ( z ^ × 200 z ^ ) .
Kyunki z ^ × z ^ = 0 :
F Cor = 0.
Yeh step kyun? Cross product magnitude mein sin ( angle ) hota hai. Velocity parallel to ω matlab angle = 0 , sin 0 = 0 → koi Coriolis nahi , chahe kitni bhi fast speed ho. Sirf v ka woh component jo axis ke perpendicular hai Coriolis produce karta hai.
Step 2 — yahan centrifugal. Axis par r ⊥ = 0 , toh F cf = m ω 2 r ⊥ = 0 bhi.
Yeh step kyun? Is configuration mein dono fictitious forces vanish ho jaate hain — "gotcha" yeh hai ki badi velocity number tumhe bada answer dene ki taraf attract karti hai.
Verify: z ^ × z ^ = 0 ⇒ F Cor = 0 ; r ⊥ = 0 ⇒ F cf = 0 . ✓
Recall Matrix ke across quick self-test
Coriolis zero hota hai jab object frame mein rest par ho ::: True (Ex 4) — v rot = 0
Coriolis zero hota hai jab object ω ke parallel move kare ::: True (Ex 8) — sin 0 = 0
Centrifugal rotation axis par zero hota hai ::: True (Ex 6, Ex 8) — r ⊥ = 0
Coriolis magnitude r ⊥ par depend karta hai ::: False — yeh v par depend karta hai, position par nahi (Ex 6)
Radial-outward velocity ek tangential Coriolis force deta hai ::: True (Ex 2, Ex 5)
Tangential velocity ek radial Coriolis force deta hai ::: True (Ex 3)