3.2.36 · D1 · HinglishOrbital Mechanics & Astrodynamics

FoundationsThird-body perturbations

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3.2.36 · D1 · Physics › Orbital Mechanics & Astrodynamics › Third-body perturbations

Yeh page parent note ke har ek symbol aur idea ko build karta hai, ek samajhdar 12-saal ke bachche se shuru karte hue jisne kabhi koi arrow hat-wala nahi dekha. Upar se neeche padhein; har block agla earn karta hai.


1. Ek vector, aur uske upar chhoti arrow

Pehla figure dekho. Neela arrow ek point se shuru hokar doosre point par khatam hota hai. Woh poora arrow hi hai. Number sirf yeh hai ki arrow kitna lamba hai — ruler se measure karo.

Figure — Third-body perturbations
Position
ek arrow kisi chosen origin se kisi cheez ke location tak
Bare symbol (bina arrow)
ki length, ek akela number

2. Ek origin se position, aur "relative" positions

Har arrow ko kahin se shuru hona padta hai. Woh starting point origin kehlata hai.

Doosra figure dekho: teen lambe arrows door origin se nikalte hain, aur chhota green arrow woh hai jo Earth se satellite tak chalke milta hai — yeh literally minus hai.

Figure — Third-body perturbations
is topic mein
satellite ki position Earth ke relative,
third body ki position Earth ke relative,
Hum kyun ghataate hain
kyunki hum Earth se observe karte hain, inertial origin se nahi

3. Gravity kaise kheenchti hai: piece by piece

Ab pull khud. Hum famous law ko bite-sized symbols mein todenge.

Teesra figure dekho yeh dekhne ke liye ki aur ek hi cheez hain: ek extra se divide karne par poora arrow (length ) unit arrow (length 1) ban jaata hai, aur woh denominator mein chala jaata hai.

Figure — Third-body perturbations
bundle , kheenchne wali body ka gravitational parameter
unit vector — ki direction, length exactly 1
mein minus sign
gravity inward kheenchti hai, mass ki taraf
mein kyun aata hai
yeh ko rewrite kiya hai; ek ko mein convert karta hai

4. Acceleration aur double-dot

velocity — position har second kaise change hoti hai
acceleration — velocity har second kaise change hoti hai

5. Dot product aur "along vs perpendicular"

Tidal formula use karta hai. Yeh ek symbol jawaab deta hai "third body ki direction mein kitna point karta hai?"

Chautha figure dekho: green arrow ki seedhi shadow orange line par daalo. Us shadow ki length exactly hai. Agar seedha ki taraf point kare, toh shadow poori length ki hai; agar perpendicular hai, toh shadow zero hai.

Figure — Third-body perturbations
ka direction par shadow (projection) (uska "along-the-Moon" part)
Perpendicular arrows ka dot product
zero
Tidal formula ise kyun use karta hai
stretch direction ko squeeze direction se alag karne ke liye

6. "Do pulls ka difference" — tides kahaan se aate hain

Ab har piece haath mein hai, toh hum central object ko naam de sakte hain.

satellite-se-third-body arrow,
Raw pull perturbation kyun nahi hai
Earth lagbhag utna hi kheencha jaata hai; common part cancel ho jaata hai, sirf difference bachta hai
Bachne wala difference kehlata hai
tidal / differential acceleration

7. aur small-quantity approximation

Earth–satellite distance, Earth–third-body distance se bahut chhoti hai
kyun drop karte hain
yeh rakhe gaye first-order term ke comparison mein negligibly small hai

Prerequisite map

Vector arrow r-hat and length r

Positions from an origin

Relative position r equals r_s minus r_E

G and mass give mu equals GM

Newton pull minus mu r over r cubed

Double dot r means acceleration

Difference of two pulls

Dot product d-hat dot r

Split along versus perpendicular

Tidal approximation with r much less than d

Third-body perturbation


Equipment checklist

Khud test karo — tum parent note ke liye ready ho tabhi jab har reveal obvious lage.

Main bata sakta hoon arrow aur hat ka matlab
ek poora arrow hai (direction + length ); sirf direction hai, length 1
Main ko aur se bana sakta hoon
, Earth se satellite tak ka arrow
Mujhe pata hai kya bundle karta hai
, gravitational parameter; third body ke liye
Main Newton ka pull padh sakta hoon
, inward point karta hai, ki tarah kamzor hota hai
Mujhe pata hai ka matlab
acceleration, position ka second time-derivative
Main interpret kar sakta hoon
ka third body ki direction mein shadow (projection)
Main samajhta hoon perturbation difference kyun hai
Earth bhi free-fall karta hai; common pull cancel hota hai, sirf tidal gradient bachta hai
Mujhe pata hai mein expand kyun karte hain
se tiny ho jaata hai, toh first order clean tidal form deta hai