3.2.34 · D1 · Physics › Orbital Mechanics & Astrodynamics › Atmospheric drag — exponential atmosphere model, orbit decay
Ek satellite atmosphere ki bilkul upar se guzarta hai, aur har halki si air puff uski thodi si energy chura leti hai. Kyunki neeche ki orbit matlab tezi wali orbit hoti hai, yeh energy loss craft ko aur tezi se andar ki taraf spiral karwata hai jab tak woh jal na jaye — toh poora topic bas energy loss + girne ki geometry hai.
Is page mein assume kiya gaya hai ki aap kuch nahin jaante. Atmospheric drag pe parent note padhne se pehle, usmein use hone wale har letter aur symbol ka matlab aapko samajh aana chahiye aur usse koi picture connect honi chahiye. Aao har ek ko earn karein.
v
Ek vector woh quantity hai jisme dono size (kitna) aur direction (kidhar) hoti hai. Hum isse ek arrow ki tarah draw karte hain: length size hai, arrowhead direction hai. Hum letter ke upar ek chhota arrow lagate hain, v , yaad dilane ke liye "yeh cheez kisi taraf point karti hai."
Satellite ki velocity v aisa hi ek arrow hai: yeh travel ki direction mein point karta hai, aur uski length batati hai ki craft kitni tez chal rahi hai.
v aur unit vector v ^
Magnitude v (koi arrow nahin) bas arrow ki length hai — ek plain number jaise "7670 metres per second". Unit vector v ^ (ek "hat", arrow nahin) wohi arrow hai jo length 1 tak shrink kiya gaya ho: yeh sirf direction rakhta hai. Toh koi bhi vector aisa split hota hai v = v v ^ : "size times pure-direction".
Topic ko yeh kyun chahiye: drag ek force hai jo travel se bilkul opposite direction mein point karti hai. "Opposite" ko precisely kehne ke liye, hum direction chahiye, aur yahi − v ^ (hat, flipped) deta hai. Parent note drag ko − 2 1 B ρ v v likhta hai — v ka ek factor size badhna hai, aur v direction carry karta hai. Ab aap jaante hain yeh sirf "v 2 " kyun nahin hai.
d t
d t ka matlab hai "time ka ek bahut chhota tukda " — itna chhota ki hum treat karte hain ki us dauran sab kuch unchanging hai. Usi tarah d h height ka ek tiny sliver hai aur d ρ density mein ek tiny change hai. Kisi bhi quantity ke aage d letter bas dhyaan se kehta hai "is cheez ka thoda sa."
Intuition Hum slivers mein kyun kaatein
Real motion smooth aur continuous hoti hai. Usse arithmetic karne ke liye hum ek heartbeat-thin moment d t freeze karte hain, figure out karte hain ki us frozen instant mein kya hota hai, phir saare instants ko add kar dete hain. Woh "saare slivers ko add karo" wala step integration kehlata hai — isi se exponential atmosphere aur decay rate dono build hote hain.
Time ke ek sliver mein, speed v se chalti cheez ek tiny distance v d t cover karti hai (speed × time). Yeh akela fact drag force ka seed hai, jaise hum dekhenge.
ρ (Greek "rho")
Density ρ measure karta hai ki space ke har cubic metre mein kitna mass packed hai . Sea-level ki moti air mein high ρ hoti hai; 400 km par near-vacuum mein astonishingly tiny ρ hoti hai (lagbhag 5 × 1 0 − 12 kg per cubic metre — ek matchbox mein kuch molecules). Units: kilograms per cubic metre, kg/m 3 .
Topic ko yeh kyun chahiye: satellite molecules se takrata hai, aur ρ count karta hai ki wahan hit karne ke liye kitne hain. Zyada ρ → zyada collisions → zyada drag. Kyunki ρ height ke saath change hoti hai, yeh Section 7 mein "exponential atmosphere" idea ka star hai.
Definition Cross-sectional area
A
A woh area hai jo satellite travel direction mein shadow daalta hai — woh "hole" ka size jo yeh air mein punch karta hai. Aage ki taraf facing flat panel mein bada A hota hai; usi panel ka edge-on mein tiny A hota hai. Units: square metres, m 2 .
m
m simply kitna matter satellite mein hai — push hone ki resistance. Units: kilograms, kg.
Definition Drag coefficient
C D
Ek messy real object apna saara forward momentum air ko nahin deta; sirf ek fraction stick karta hai. C D ek dimensionless fudge-number hai (satellite ke liye lagbhag 2) jo capture karta hai ki shape kitna "grippy" hai. Koi units nahin — bas ek multiplier.
Definition Ballistic coefficient
B
Inhein bundle karo: B = m C D A . Words mein, drag-area per unit mass . Ek halka craft jisme bade panels hain (bada A , chhota m ) mein bada B hota hai aur air se zyada dhakka lagta hai → tezi se decay hota hai. Ek dense compact craft mein chhota B hota hai aur zyada survive karta hai. Units: m 2 / kg .
Bundle kyun karein? Warna har drag formula mein C D , A , aur m alag se aate. Nature hamesha sirf unka combination use karta hai, toh hum ek baar naam dete hain aur aage badhte hain. Yeh ballistic coefficient hai jo decide karta hai ki reentry mein kaun survive karta hai.
F aur acceleration a
Ek force ek push ya pull hai. Jab koi force mass m par act karta hai, toh woh acceleration a produce karta hai — velocity change hone ki rate (tez hona, slow hona, ya turn karna). Inhein Newton's law F = m a se tie kiya gaya hai. Force bhi velocity ki tarah apna size aur direction split karta hai, toh a bhi ek arrow hai.
Common mistake "Acceleration" ko "tez jaana" samajhna
Yeh sahi kyun lagta hai: roz ki boli mein "accelerate" matlab "tez jaana" hai.
Fix: acceleration velocity mein koi bhi change hai — slow hona aur turn karna bhi. Drag ka acceleration backward point karta hai (− v ^ ), toh yeh path ke saath ek deceleration hai, phir bhi orbit tez ho jaati hai. "Acceleration = change of velocity" ko dimag mein pakke se rakho.
Topic ko yeh kyun chahiye: parent ka central boxed result ek drag acceleration hai a d r a g = − 2 1 B ρ v v . Ab ise padhein: minus sign = backward, 2 1 B ρ v = kitna strong, v = path ke along (toh poori cheez backward point karti hai strength ke saath jo v 2 ki tarah badhti hai).
Definition Orbit ka semi-major axis
a
Ek orbit (generally) ek oval hoti hai, ek ellipse . Uski lambi taraf mein aadhi length semi-major axis a hoti hai. Near-circular orbit ke liye, a bas circle ka radius hota hai — satellite ki Earth ke centre se doori. Bada a = zyada upar, wider orbit.
Definition Gravitational parameter
μ
μ = G M ⊕ Newton's gravity constant G ko Earth ki mass M ⊕ ke saath ek single number mein package karta hai (SI units mein 3.986 × 1 0 14 ). Yeh kehta hai yeh particular planet kitna strongly pull karta hai . Hum ise B ki tarah bundle karte hain: gravity hamesha sirf yeh product use karta hai.
Definition Specific mechanical energy
ε
Specific energy ε satellite ki total energy (motion + height) per kilogram of the satellite hai. "Per kilogram" (word specific ) convenient hai kyunki isse answer craft ke weight par depend nahin karta. Ek bound orbit ke liye yeh negative hoti hai, aur parent key result ε = − 2 a μ use karta hai.
Intuition Energy picture padho
Upar ke curve ko dekho. Jaise a (rightward) badhta hai, ε neeche se zero ki taraf climb karta hai — ek badi dur wali orbit mein zyada energy hoti hai (escape ke karib). Jaise a shrink hoti hai, ε zyada negative ho jaati hai: satellite mein kam energy hoti hai. Drag hum ko is curve ke along leftward drive karta hai, aur energy-versus-size relationship hi "energy gayi" ko "orbit shrink hui" mein convert karti hai.
Yeh do facts — Two-Body Problem aur Vis-Viva Equation se — woh bridge hain jis par poori decay story khadi hai:
ε = − 2 a μ , v = a μ ( circular orbit ) .
Intuition Ek nazar mein paradox
v = μ / a : square-root ke neeche chhota a bada v deta hai. Toh jis moment drag energy churaata hai aur a shrink karta hai, orbital speed badh jaati hai. Energy kho jaane se aap tez ho jaate hain — kyunki aap Earth ke karib gir gaye, jahan orbit mein rehne ke liye tez chalana padta hai.
Definition Exponential function
e − x
e ek fixed number hai, lagbhag 2.718 . Function e − x kisi bhi cheez ko describe karta hai jo har equal step par same fraction se shrink hoti hai : ek step jaao, yeh e 1 ≈ 37% ho jaata hai; ek aur step, uska 37% ; aur aisa chalte rehta hai — kabhi zero nahin pahunchta. Yeh "jitna zyada ho, utni tezi se khoye" ka natural fingerprint hai.
H
Scale height H woh vertical distance hai jitni upar jaane par air ek factor e se thin ho jaati hai (37% tak aa jaati hai). Ground ke paas H ≈ 8 km hai; thermosphere mein H ≈ 60 km. Density law hai ρ ( h ) = ρ 0 e − ( h − h 0 ) / H : har H metres upar jaane par ρ ko e se divide kar do.
Topic ko yeh kyun chahiye: density linearly nahin fade hoti — yeh exponentially collapse hoti hai. Isliye low perigee par drag itna fierce hota hai aur thoda upar jaate hi negligible ho jaata hai, aur isliye decay itni violently nonlinear hai. Exponential seedha pressure ko gravity se balance karne se aata hai, isliye H = k B T / ( m m o l g ) — hot, halki air puff up hoti hai (bada H ); strong gravity ke neeche bhaari air squash ho jaati hai (chhota H ).
Tiny slice dt and integration
Specific energy and semi-major axis a
Circular speed from mu over a
Upar se neeche padho: geometry aur density drag acceleration build karte hain; drag times velocity power lost hai; energy loss plus energy-size relation decay rate deta hai — parent ka finale d t d a = − B ρ μ a .
Apne aap ko test karo — right side cover karo aur dekho ki parent note kholne se pehle kya ring of truth hai.
v par arrow aapko kya batata hai jo plain v nahin batata?Motion ki direction; plain v sirf length (speed) hai.
Unit vector v ^ kya hai? Wohi arrow length 1 tak scale kiya gaya — pure direction, koi size nahin.
d t ka matlab?Time ka ek vanishingly small slice jiske dauran kuch bhi appreciably change nahin hota.
Density ρ kya count karta hai? Har cubic metre mein packed air ka mass — kitne molecules hit karne ke liye hain.
Ballistic coefficient B define karo aur large B kya imply karta hai. B = C D A / m , drag-area per mass; bada B (halka, bada area) tezi se decay karta hai.
Force aur acceleration mein kya fark hai? Force push hai; acceleration velocity mein resulting change hai,
F = m a .
Near-circular orbit ke liye semi-major axis a kya hai? Orbit ka radius — Earth ke centre se doori.
μ kya bundle karta hai?μ = G M ⊕ , Earth ke gravitational pull ki strength.
a ke terms mein circular speed aur specific energy batao.e − x kaisi shape describe karta hai?Kuch aisa jo har equal step par same fraction se shrink hota hai — kabhi zero nahin pahunchta.
Scale height H kya hai? Woh altitude gain jiske baad density ek factor e se drop ho jaati hai (lagbhag 37% tak).