2.1.21 · D3 · HinglishAnalytical Mechanics

Worked examplesRigid body dynamics — Euler angles, Euler's equations of motion

2,308 words10 min read↑ Read in English

2.1.21 · D3 · Physics › Analytical Mechanics › Rigid body dynamics — Euler angles, Euler's equations of mot

Shuru karne se pehle, ek line ka reminder us tool ka jo hum poore time use karenge.


The scenario matrix

Is topic ki har problem inhi cells mein se ek hoti hai. Last column batata hai ki kaun sa worked example usse solve karta hai.

# Case class Kya badalta hai Example
A Symmetric top, torque-free (, ) body-frame precession, ka sign Ex 1, Ex 2
B Fully asymmetric, torque-free () har axis ki stability, sign flips Ex 3
C Degenerate: sphere () saari coupling khatam Ex 4
D Zero input: exactly principal axis par spin , koi wander nahi Ex 4
E Torque driven, single axis () pure angular acceleration Ex 5
F Gyroscopic / steady precession (real-world word problem) torque vs ka balance Ex 6
G Euler-angle rates → (projection trap) non-orthogonal axes, Ex 7
H Exam twist: prolate vs oblate sign ( vs ) precession ki direction ulat jaati hai Ex 8
I Limiting value (fast-spin limit) kaun sa term dominate karta hai Ex 2 (part b)

Ex 1 — Cell A: torque-free symmetric top, basic precession rate

Step 1. Equation 3 ko aur ke saath likhte hain: Yeh step kyun? Agar spin-axis rate constant nahi hoti, toh "uske baare mein precession" fixed-rate motion nahi hoti — pehle confirm karna zaroori hai ki frozen hai.

Step 2. Constant ko equations 1 aur 2 mein substitute karo. ke saath yeh ban jaate hain: Yeh step kyun? Yeh pair ek point ke equation hai jo angular rate par circle mein ghoom raha hai — yahi wobble hai.

Step 3. Numbers daalo:

Figure — Rigid body dynamics — Euler angles, Euler's equations of motion

Figure dekho: transverse angular-velocity vector (pale-yellow arrow) ki tip body-3 axis ke baare mein blue circle trace karti hai rate par, jabki constant (pink) seedha upar point karta hai.

Recall Forecast answer

ke same sign mein (kyunki , isliye ), aur yahan yeh ke barabar hota hai kyunki exactly hai. Thin disk ke liye yeh "" relation disguise mein hai.

Verify: Units: . ✓ Sign: , ek oblate body, precession spin ke same sense mein. ✓


Ex 2 — Cell A + Cell I: Earth ki Chandler-type wobble aur fast-spin limit

Step 1 (a). Ex 1 se, . Yeh step kyun? Same symmetric-top formula; sirf number badla.

Step 2 (a). Period . Yeh step kyun? Period hota hai divided by rate; cancel ho jaate hain, spin-periods = 305 days bachta hai.

Step 3 (b). Equation 1 with : . Jab , right side ( mein linear) kisi bhi aisi term ko dwarf karta hai jo se multiply nahi hui. Yeh step kyun? Dominant term identify karne se pata chalta hai ki wobble frequency linearly spin ke saath scale karti hai — faster spin karo, faster wobble hoga.

Recall Real Chandler wobble par reality check

Observed wobble ~433 days hai, 305 nahi — kyunki Earth perfectly rigid nahi hai; yeh deform hoti hai. Dekho Chandler wobble. Rigid-body prediction bilkul humara 305-day answer hai, aur yeh discrepancy apne aap mein informative hai.

Verify: days from . Units: in rad/day in days. ✓ Limit: right-hand side , baaki sab se independent. ✓


Ex 3 — Cell B: fully asymmetric body, intermediate-axis (tennis-racket) test

Step 1. Axis 1 ke baare mein nearly spin: const large, tiny. Equations 2 aur 3 ko linearize karo (do chhoti quantities ka product drop karo): Yeh step kyun? Small-perturbation analysis: sirf chhote components mein linear terms rakho yeh dekhne ke liye ki woh badhte hain ya oscillate karte hain.

Step 2. Pehle wale ko differentiate karo, doosre ko substitute karo: Yeh step kyun? Do first-order equations ko ek second-order equation mein reduce karne se ka sign milta hai: oscillation (stable), exponential growth (unstable).

Step 3. Har axis ke liye coefficient evaluate karo (bahar factor hota hai, isliye sirf is product ka sign matter karta hai). Maano , toh stable :

  • Axis 1 (smallest): stable.
  • Axis 2 (middle): unstable.
  • Axis 3 (largest): stable.
Figure — Rigid body dynamics — Euler angles, Euler's equations of motion
Recall Forecast answer

Axis 2, intermediate axis. Yahi [tennis-racket / Dzhanibekov effect] hai — apna phone middle axis ke baare mein spin karake flip karo aur yeh palta jaata hai. Dekho bhi Angular momentum in rotating frames.

Verify: Products: axis1 , axis2 , axis3 . Exactly ek positive → exactly ek unstable axis. ✓


Ex 4 — Cells C & D: sphere, aur exactly principal axis par spin

Step 1 (C). Har coupling factor hai, isliye teeno equations padhti hain . Yeh step kyun? Sphere ultimate degenerate case hai — koi bhi principal axis special nahi, isliye koi wobble direction select nahi ho sakti.

Step 2 (C). const forever. Koi bhi axis stable spin axis hai.

Step 3 (D). ke saath: equation 1 mein hai, equation 2 mein hai, equation 3 mein hai. Isliye . Yeh step kyun? Yeh zero-input cell hai: pure principal-axis spin mein koi gyroscopic coupling nahi hoti kyunki baaki do components jo multiply hote woh zero hain. Yeh motion equations ka ek fixed point hai.

Verify: (C) saare isliye RHS . ✓ (D) har RHS product mein mein se kam se kam ek hai, dono zero hain, isliye RHS . ✓


Ex 5 — Cell E: single-axis torque, pure angular acceleration

Step 1. Kyunki hai, equation 3 apna coupling term kho deti hai: Yeh step kyun? Hume coupling vanish hona check karna chahiye assume karne ki jagah — yahan use khata hai, isliye hum ek clean -style law se bache hain.

Step 2. Integrate karo: ; zero start ke saath, . Yeh step kyun? Constant angular acceleration ek straight-line spin-up mein integrate hoti hai.

Step 3. par: .

Recall Forecast answer

Koi coupling nahi — yeh woh ek case hai jahan naive sahi hai, precisely isliye kyunki hum principal axis par koi transverse rate ke bina spin kar rahe hain.

Verify: . Units: . ✓


Ex 6 — Cell F: real-world gyroscope, steady precession

Step 1. Pivot ke baare mein gravity torque: , horizontal, spin axis ke perpendicular. Yeh step kyun? Yahi torque hai jise steady precession mein machinery ko balance karna hota hai.

Step 2. Steady precession ke liye spin angular momentum rate par turn karta hai, isliye . set karo: Yeh step kyun? Yeh Euler ka balance disguise mein hai — torque wheel ko speed up nahi karta, yeh uski axis ko swing karta hai. Dekho Gyroscope precession.

Step 3. Numbers:

Figure — Rigid body dynamics — Euler angles, Euler's equations of motion
Recall Forecast answer

Slower. : ek fast top lazily precess karta hai, ek dying top wildly — bilkul wahi jo aap real top slowdown hote waqt dekhte ho.

Verify: . Units: . ✓


Ex 7 — Cell G: Euler-angle rates → (projection trap)

Step 1. Parent note ke 3-1-3 projection formulas use karo: Yeh step kyun? Teen Euler axes (, line of nodes, body-) perpendicular nahi hain, isliye hum sirf components read off nahi kar sakte — hume project karna padega, yahi kaam yeh factors karte hain.

Step 2. daalo (, ), (), :

Step 3. Toh .

Recall Forecast answer

Nahi hai, 5 nahi. Precession body-3 axis mein term ke through leak karta hai. Rates ko components ki tarah treat karna parent note ka [!mistake]-2 hai.

Verify: ; . ✓ Kinetic energy mein yeh kahan feed hote hain, uske liye dekho Lagrangian of the symmetric top.


Ex 8 — Cell H: exam twist, prolate vs oblate precession ka sense flip karta hai

Step 1 (oblate). . Yeh step kyun? factor ko positive banata hai — precession spin ke same sense mein (frisbee ki tarah).

Step 2 (prolate). . Yeh step kyun? factor ko negative banata hai — precession spin ke opposite sense mein (spinning pencil / cigar ki tarah). ka sign hi poori kahani hai.

Step 3. Summary: oblate , prolate .

Recall Forecast answer

Prolate (cigar-shaped) top: uska transverse body-3 axis ke around apne khud ke spin ke ulte direction mein circle karta hai.

Verify: oblate , prolate ; signs hain aur . ✓


Jaate jaate ek full-throttle question:

ke liye kaun sa axis unstable hai?
Intermediate axis (axis 2).
Torque-free symmetric top ke liye, spin ke terms mein kya hai?
.
Kya gyroscope faster spin karne par faster ya slower precess karta hai?
Slower, kyunki .