3.6.21 · D1 · Physics › Spacecraft Structures & Systems Engineering › Spacecraft bus — structure, power, thermal, ADCS, C&DH, comm
Ek spacecraft basically ek box hai jo cold, dark vacuum mein rehta hai — jise khud ko power deni hai, khud ko warm-but-not-too-warm rakhna hai, launch ki shaking ke against hold karna hai, jahan bola jaye wahan point karna hai, aur ghar phone karna hai — bina kisi air ke, bina kisi repairman ke, aur bina kisi do-over ke. Is chapter ka har equation bas ek balance sheet hai: energy in vs. energy out, force applied vs. strength available, heat absorbed vs. heat radiated.
Parent note mein koi bhi formula padhne se pehle, tumhe woh alphabet chahiye jisme wo formulas likhe gaye hain. Yeh page har letter define karta hai — plain words mein uska matlab, woh kaunsi picture represent karta hai, aur kyun topic uske bina kaam nahi kar sakta. Upar se neeche padho; har idea sirf upar wale ideas use karta hai.
Intuition Space do crutches cheen leta hai jinpe hum rely karte hain
Earth pe, gravity cheezein neeche pakad ke rakhti hai aur air heat carry karke door le jaati hai aur tumhe support karti hai. Orbit mein, gravity abhi bhi pull karti hai (isliye tum circling karte rehte ho) lekin koi air nahi hoti. No air ka matlab:
No convection — tum heat fan karke door nahi bhej sakte; heat dump karne ka ek hi tarika hai ki use invisible light ke roop mein glow karke radiate karo.
Speed pe no air resistance ka dar — lekin jo launch tumhe wahan le gaya tha usne tumhe violently shake kiya.
Yeh ek fact — no air — hi reason hai kyun thermal section sirf radiation ki baat karta hai, aur kyun parent note baar baar "no convection" kehta rehta hai. Ise yaad rakho.
Figure s01 — Woh picture jo Part 0 fix karti hai: warm box heat sirf orange radiation arrows se shed kar sakta hai; crossed-out "no air" yaad dilata hai ki convection aur conduction-to-air simply unavailable hain. Baad ke har thermal equation mein yeh restriction inherit hoti hai.
m
m kisi object mein kitna "stuff" hai woh measure karta hai, kilograms (kg) mein. Ek pile of bricks imagine karo: zyada bricks, bada m .
Topic ko m isliye chahiye kyunki spacecraft jitna heavy hoga, launch utna zyada shake karega (Part 4), aur total utna zyada "useful payload" aur "supporting bus" ke beech split hoga.
A
A kitni flat surface koi cheez cover karti hai, square metres (m²) mein. Ek sheet of paper jo floor pe shadow daalta hai, uske size ko imagine karo — uska size hi area hai.
Do alag areas matter karte hain aur inhe mix nahi karna chahiye:
A proj — woh projected (shadow) area jo Sun ki taraf face karti hai. Ek tilted panel kam sunlight pakadta hai; uski shadow hi count hoti hai.
A — woh total radiating surface jo heat glow karke radiate kar sakti hai.
Common mistake Sari radiating area
A cold space ko equally nahi dekhti
Full surface area A ek upper limit hai ki kitna radiate ho sakta hai. Actually ek face warm Earth ki taraf point kar sakta hai, panels ek doosre ko block kar sakte hain, aur folds sirf khud ko "see" kar sakte hain. Engineers isko view factor kehte hain — ek surface ki glow ka woh fraction jo actually cold space tak pahuncha. Jab parent note ka thermal section baad mein apna heat-rejection formula likhta hai, to woh quietly assume karta hai ki A woh effective area hai jo truly cold sky ki taraf face karti hai, jo geometric total se noticeably kam ho sakti hai. (Us formula ke symbols — ϵ , σ , T — sab Part 6 mein define hain unhe use karne se pehle.)
Figure s02 — Kyun topic do alag areas alag rakhta hai: sunlight power plum projected (shadow) area A proj pe depend karti hai, bade teal panel pe nahi. Panel ko tilt karo aur uski shadow shrink ho jaati hai chahe panel khud unchanged ho — woh shrinking shadow exactly wahi hai jo A proj measure karta hai.
L aur density ρ
L (metres) bas koi piece kitna tall/long hai woh hai. ρ (Greek letter rho , "row" bolo) density hai — har cubic metre mein kitna mass packed hai, kg/m³ mein. Lead vs. foam imagine karo: same box size, lead ka ρ bahut bada hoga.
m = A ⋅ L ⋅ ρ kyun? Pehle ek straight wall ka volume nikalo: constant cross-section A ki shape ko length L pe stretch karo to volume V = A ⋅ L hoga (end ka area × kitni dur drag kiya). Phir mass = volume × density, m = V ⋅ ρ = A ⋅ L ⋅ ρ . Yeh two-step chain hai jisse "yeh wall kitni strong honi chahiye" (jo A fix karta hai) "kitna heavy hoga" mein convert hoti hai.
a acc
a acc kitni tezi se tumhari speed change ho rahi hai woh hai, metres per second, per second (m/s²) mein. Ek car floor karte imagine karo: tum seat mein press ho rahe ho — woh press hi acceleration hai.
Ek deliberate subscript: is chapter mein baad mein plain italic a Earth ke albedo ke liye use hoga (Part 6), jo bilkul alag quantity hai. Inhe shuru se alag rakhne ke liye, hum acceleration ko a acc likhte hain is foundations page mein throughout.
Letter g ek unit hai jiska matlab hai "Earth ki gravity jitna strong", 1 g = 9.8 m/s 2 . To launch ke waqt "10 g " ka matlab hai rocket spacecraft ko 10 × zyada strongly push kar raha hai jitna gravity tumhe chair mein pakad ke rakhti hai.
σ aur yield strength σ y
σ (Greek sigma ) force spread over area hai: σ = F / A , pascals (Pa = N/m²) mein. Snow pe khade hone ka imagine karo: flat feet (bada area) → tum float karte ho; stiletto heel (tiny area) → tum dhanste ho. Same weight, alag stress .
σ y yield strength hai — woh stress jis par material permanently jhuk jaata hai aur waise hi rehta hai instead of spring back karne ke. σ y se neeche push karo: safe. Upar push karo: barbad.
Letter σ ke baare mein heads-up: Part 6 mein yahi Greek letter phir aayega Stefan–Boltzmann constant ke roop mein, jo bilkul alag cheez hai. Yahan structure world mein, σ ka matlab hamesha stress hai.
Common mistake Stress force NAHI hai
Ek thin wire aur ek fat beam same force F carry kar sakte hain, phir bhi wire high stress pe hai (tootne ke qareeb) jabki beam relaxed hai — kyunki stress area se divide hota hai. Hamesha poochho "kitni area ke upar?"
Hum Greek letter η se pehle milte hain kisi bhi specialised ratio mein use karne se pehle, kyunki Part 4 mein structural "strength-per-weight" ratio usi letter se likha gaya hai.
η
η (Greek eta , "ay-ta" bolo) ek general idea hai ek "goodness ratio" ka: jo tum chahte ho woh kitna milta hai, per unit of jo tumhe cost hota hai . Sabse clean case mein yeh woh fraction hai jo tumhare paas bachi rehti hai, 0 aur 1 ke beech ki number.
Picture: paani ek leaky bucket mein daalo; η woh fraction hai jo leak se bach jaati hai.
Topic η ko kai flavours mein use karta hai — battery charging, battery discharging, aur structural bang-per-kilogram — isliye abhi general meaning seekho, phir har specific wala jab aaye tab milo.
Definition Battery efficiencies
η charge , η discharge
η charge = 0.9 ka matlab hai har 10 joules jo tum battery mein push karte ho, 9 stick hote hain (baaki heat ke roop mein leak ho jaate hain). η discharge = 0.95 ka matlab hai har 10 joules jo tum wapas pull karne ki koshish karte ho, 9.5 milte hain. Dono "fraction kept" numbers hain.
Intuition Strength-per-weight, aur kyun units yahi kehte hain
Agar tum strength chahte ho lekin mass carry karna nahi chahte, to tumhe aisi material chahiye jismein high strength σ y ho lekin low density ρ ho . Unka ratio η struct = σ y / ρ hai "bang per kilogram" — exactly Part 3 ke η sense mein ek goodness ratio (jo tum chahte ho ÷ jo cost hota hai).
Kyun units yeh "strength per weight" banate hain: stress σ y pascals = N / m 2 mein hai, aur force newtons mein kg ⋅ m / s 2 hai, isliye
ρ σ y = kg / m 3 N / m 2 = m 2 ⋅ kg N ⋅ m 3 = kg N ⋅ m .
Yeh hai force-carrying-capacity times length, divided by mass — literally kitna load-times-reach tum buy karte ho per kilogram jo tumhe orbit mein lift karna hai. Aluminium aur carbon-fibre yahan high score karte hain, aur yahi poora reason hai ki spacecraft inse banaye jaate hain.
E vs. Power P
Energy E "kaam karne ki ability" ki ek total amount hai, joules (J) mein. Power P woh rate hai jis par tum ise spend ya banate ho, watts (W) mein, jahan 1 W = 1 J/s .
Picture: bank mein paisa energy hai; tumhari salary-per-second power hai.
Link ek stretch of time hai, jise hum T likhte hain — ek duration seconds mein measure hoti hai. Steady power P par time T ke baad, deliver ki gayi energy hai
E = P ⋅ T ( power × kitna der ) .
Common mistake Watts aur joules ko confuse karna
"Array 80 W banata hai" tumhe ek rate batata hai, koi stockpile nahi. Kitni energy deliver hoti hai yeh jaanne ke liye kitna der se multiply karo: E = P ⋅ T . Batteries energy store karti hain (joules / watt-hours); solar arrays power supply karti hain (watts).
Yeh sirf upar wale duration T ki specific values hain, tagged ki orbit ke kis part ko cover karti hain. Jaise spacecraft Earth ke loops lagata hai, woh har lap ka kuch part sunlight mein spend karta hai aur kuch part Earth ki shadow mein chhupa rehta hai.
T orbit — ek full lap ka time.
T sun — sunlit part (arrays working).
T eclipse — shadow part (arrays dead, battery load carry karti hai).
Yeh satisfy karte hain T orbit = T sun + T eclipse .
Figure s03 — Orbit-timing symbols kahan rehte hain: spacecraft dotted loop pe ride karta hai, arc T sun pe orange sunlight mein nahaya hua aur T eclipse ke liye plum shadow cone mein swallowed. Poora lap T orbit hai. Yeh woh physical stage hai jis par neeche ka power-balance derivation play out hota hai.
Definition Temperature in kelvin
Temperature measure karta hai koi cheez kitni hot hai. Spacecraft engineers kelvin (K) use karte hain: Celsius jaisi hi size ke steps, lekin absolute zero se shuru hoti hai, isliye K = ° C + 273 . Room temperature 20° C = 293 K .
Letter ke baare mein note: parent note temperature ko plain T likhta hai, lekin is page pe T ka matlab pehle se ek time duration hai (Part 5). Isliye is Part mein hum temperature ko T temp tag karte hain dono ko alag rakhne ke liye; jab tum parent ka thermal formula padho, uska T yahi temperature hai.
Kelvin kyun, Celsius nahi? Kyunki neeche ka radiation law T temp 4 se multiply karta hai, aur yeh sirf tab kaam karta hai jab temperature true zero se shuru ho — ek 0° C object abhi bhi bahut glow karta hai, isliye tumhe ise "no glow" mean nahi karne de sakte.
Definition Jo heat free mein aati hai
S — solar constant , 1361 W/m 2 : woh power jo sunlight Earth ke paas har square metre ko deliver karti hai. Ek fixed brightness ki heat-lamp ke neeche khade hone ka imagine karo.
a — Earth ka albedo ≈ 0.3 : sunlight ka woh fraction jo Earth upar tum par bounce karta hai . Yeh italic a (albedo) acceleration se alag quantity hai, exactly isliye humne acceleration ko a acc tag kiya Part 2 mein.
E Earth ≈ 237 W/m 2 — woh infrared glow jo warm Earth khud tumhare upar radiate karta hai.
Mnemonic Kaunsa knob kis climate ke liye
Hot orbit → cool rehna chahte ho → low α / ϵ (kam soak karo, zyada glow karo).
Cold orbit → flip karo: high α / ϵ . "Alpha In, Epsilon Out."
Q ke liye sign convention
Har Q ek heat flow in watts hai. Hum sab kuch jo spacecraft ko warm karta hai use positive input count karte hain aur Q in mein lump karte hain; heat jaane ka ek hi tarika hai Q out . Chaar inputs hain:
Sunlight: Q solar = α A proj S — projected area beam pakadta hai.
Albedo (bounced sunlight): Q albedo = α A a S — fraction a sunlight ka jo Earth reflect karta hai upar.
Earth ki apni glow: Q Earth = ϵ A E Earth .
Electronics waste heat: Q dissip — power jo spacecraft ke apne circuits heat mein turn karte hain.
Inका sum total input hai:
Q in = Q solar + Q albedo + Q Earth + Q dissip .
Definition Stefan–Boltzmann constant
σ
σ yahan Stefan–Boltzmann constant hai = 5.67 × 1 0 − 8 W/(m 2 K 4 ) — nature ka ek fixed number jo set karta hai kitni brightly ek warm surface glow karti hai . Warning: yeh wahi Greek letter σ hai jo Parts 2–4 mein stress ka matlab rakhta tha, lekin yahan yeh radiation constant hai. Dono unrelated hain; sirf neighbourhood batata hai kaun sa meant hai. (Structure section → stress; thermal section → yeh constant.)
Figure s04 — Woh cheez jo T 4 law add karta hai jo words nahi kar sakte: rejected heat ki orange curve tezi se aur tezi se upar uthti hai, isliye "heat jo mujhe dump karni hai" ki horizontal line (teal) exactly ek temperature pe cross karti hai (plum dot). Woh crossing HI spacecraft ki settling temperature hai — heat load thoda upar karo aur crossing barely move karti hai, isliye vehicle self-stabilise karta hai.
Intuition Kyun "balance" temperature solve karta hai
Spacecraft ki temperature tab tak drift karti rehti hai jab tak Q in = Q out na ho. Ise write karte hain,
Q in = ϵ σ A T temp 4 ,
aur T temp ke liye solve karna batata hai exactly kitna hot woh rehega — yahi poora thermal calculation hai.
battery eta_charge eta_discharge
power P and energy E over time T
load power P_load and array power P_SA
orbit times T_sun T_eclipse
solar constant S albedo a
Stefan-Boltzmann sigma and T to the 4
Parent Spacecraft Bus topic dekho in letters ko full subsystem story mein assemble hote dekhne ke liye.
Right side cover karo aur khud test karo — tab ready ho jab har jawab instantly aaye.
Launch par F = m a acc se tum kya compute kar sakte ho? Woh axial force jo structure ko carry karni padegi: mass times launch acceleration.
Acceleration ko is page par a acc tag kyun kiya? Ise plain italic a se alag rakhne ke liye jo Earth ke albedo ke liye use hota hai.
Stress σ aur force F mein kya difference hai? Stress force divided by area hai; same force thin part par high stress deta hai, fat part par low stress.
σ y kya mark karta hai?Yield strength — woh stress jiske upar material permanently jhuk jaata hai.
Efficiency η kya hai, ek phrase mein? Ek goodness ratio — jo tum chahte ho divided by jo cost hota hai (often kept-fraction, 0 to 1).
σ y / ρ ke units "strength per weight" kyun mean karte hain?Yeh newton·metre per kilogram tak reduce hote hain — load-times-reach jo per kilogram lifted khareeda jaata hai.
Ek wall ka mass m = A L ρ kyun hai? Volume = cross-section area × length, phir mass = volume × density.
P load aur P SA ka matlab kya hai?P load woh rate hai jis par sab equipment power khaate hain; P SA (SA = Solar Array) woh rate hai jis par panels power generate karti hain.
Power P aur energy E ko confuse kyun nahi karna chahiye? P ek rate hai (watts); E ek total hai (joules); E = P T jahan T ek time duration hai.
Array oversizing factor 1 + T eclipse / ( T sun η charge η discharge ) kahan se aata hai? Daylight mein banked energy ko eclipse mein spent energy ke equal set karne se, dono battery leaks ke liye corrected.
Heat options se convection ko kya remove karta hai spacecraft ke liye? Space ka vacuum — koi air nahi, isliye bahar jaane ka ek hi tarika radiation hai.
Radiation law ke liye temperature kelvin mein kyun likhi jaati hai? Kyunki Q out ∝ T 4 ko ek aise scale ki zarurat hai jo absolute zero se shuru ho.
α aur ϵ har ek kya control karta hai?α = sunlight ka absorbed fraction; ϵ = surface kitna well heat glow karta hai.
Heat flows ko kaunsa sign convention ek saath jodta hai? Sab warming flows positive inputs hain Q in mein summed; ek hi exit Q out hai, aur balance set karta hai Q in = Q out .
Effective radiating area geometric A se kam kyun ho sakti hai? View factors — surface ka har part cold space nahi dekhta; kuch warm Earth ki taraf face karta hai ya block hota hai.
T 4 law ek stable operating temperature kyun deta hai?Thodi si temperature rise rejected heat ko sharply multiply karti hai, balance wapas push karti hai.
Kaun si do unrelated quantities dono σ symbol use karti hain? Mechanical stress (pascals) aur Stefan–Boltzmann constant (5.67 × 1 0 − 8 ).