3.2.26 · D1 · Physics › Orbital Mechanics & Astrodynamics › Patched conic method — interplanetary trajectory design
Spacecraft ko Earth se Mars bhejना actually har cheez har cheez ko kheench rahi hai ka ek ulajha hua jumla hai, jise koi bhi clean formula se solve nahi kar sakta. Toh hum cheat karte hain: har moment pe pretend karte hain ki sirf sabse paas wala bhaari body matter karta hai , us easy one-body problem ko solve karte hain, aur easy pieces ko glue karte hain — planet ke paas hyperbola, Sun ke around ellipse.
Is parent note ko padhne se pehle patched conic method par, tumhe har woh symbol jo woh tum par fenkta hai pehle se obvious lagna chahiye. Yeh page har ek ko kuch nahi se build karta hai, ek aisi order mein jahan har idea usse pehle wale par tikaa hota hai.
Central body woh single bhaari object hai jise hum pretend karte hain ki kisi given moment mein saari khichaav wahi kar raha hai. Socho ek lamppost jiske around ek string par ek ball ghoom rahi hai — lamppost central body hai, ball hamara spacecraft hai.
Definition Conic (conic section)
Conic woh koi bhi curve hai jo ek flat plane se cone ko kaatne par milti hai: circle, ellipse, parabola, hyperbola. Gravity mein, ek single central body ke around ek object hamesha inhi mein se ek trace karta hai. Isliye hi is method ko "patched conic " kehte hain: har easy piece inhi curves mein se ek hoti hai.
Figure dekho: wahi cone, chaar slices, chaar curves. Ek closed slice (ellipse) matlab object bound hai aur wapas aata rahega. Ek open slice (hyperbola) matlab woh hamesha ke liye ud jaata hai. Poori trip mein ek ellipse (Sun-bound cruise) use hoti hai jo do hyperbolas (har planet ke paas fly-away/fly-in) se glued hoti hai. Yeh mental image rakhna — neeche har symbol inhi curves mein se ek ko decorate karta hai.
r = central body se distance
r simply itna hai ki spacecraft kitna door hai us body ke centre se jo kheench rahi hai , metres mein measure kiya hua. Ek picture mein yeh central body se spacecraft tak seedhi arrow ki length hai.
Intuition Isko kyun chahiye
Gravity distance ke saath weak hoti jaati hai. Har gravity formula pehle "kitna door?" poochta hai — isliye r almost har cheez ka input hai. Dhyan rakho ki wahi letter cruise chapter mein Sun se distance ka matlab hai lekin fly-by chapter mein planet se distance ka. Jab bhi r dekho, pehle poochho: kisse distance?
a = semi-major axis
Ek ellipse ek stretched circle hai. Iska sabse lamba line, corner se corner centre ke through, major axis hai. Uska aadha semi-major axis a hai. Yeh woh single number hai jo kehta hai "yeh orbit kitni badi hai."
Definition Perihelion & aphelion (perigee & apogee)
Transfer ellipse par Sun ke sabse paas wala point perihelion hai (note mein radius r 1 ) aur sabse door wala aphelion hai (radius r 2 ). "Peri-" = paas, "apo-" = door, "-helion" = Sun, "-gee" = Earth.
Kyunki do extreme points major axis ke opposite ends par baithte hain,
a t = 2 r 1 + r 2 .
Yeh kya kehta hai: trip ellipse ka semi-major axis sirf near aur far distances ka average hai. Figure dekho — r 1 aur r 2 do ends hain, unka midpoint centre hai, aur a t centre se end tak pahunchta hai.
Subscripts jo milenge: a p = ek p lanet ke orbit ka size (Sun se uski distance), a t = t ransfer ellipse ka size.
m p = ek p lanet ka mass, m ⊙ = Sun ka mass (chota circle-with-dot ⊙ Sun ka purana symbol hai), m E = E arth ka mass. Mass hai "kitna stuff," aur zyada stuff matlab zyada strong pull.
G — gravitational constant
G nature ka fixed conversion factor hai jo "mass aur distance" ko "pull" mein convert karta hai. Yeh kabhi nahi badlta: G = 6.674 × 1 0 − 11 SI units mein.
v = speed
v kitna fast spacecraft move karta hai, metres per second mein. Ek picture mein yeh motion ki direction mein ek arrow hai; uski length speed hai.
Parent note kai speeds name karta hai — yeh sab sirf v hai jo kisi khaas jagah ya kisi khaas body ke relative measure kiya gaya:
Symbol
Seedha matlab
v c
kisi radius par c ircular orbit hold karne ki speed
v esc
esc ape speed — bas itna kaafi ki hamesha ke liye nikal jao
v p
p erigee par speed (closest approach)
v ∞
bahar nikalne ke baad infinitely door jaane par jo speed bachi, woh
v t
t ransfer ellipse par speed
v ∞
v ∞ ko "vee-infinity" padho — woh speed jo spacecraft ke paas tab bhi bachi hoti hai jab woh kisi planet ke gravity well se poori tarah bahar nikal jaata hai, us planet ke relative measure ki gayi. Socho ek ball seedha upar phenk rahe ho: escape speed use top tak pahunchati hai kuch bacha nahi; extra speed matlab woh top par abhi bhi move kar raha hai — woh bachi hui speed v ∞ hai. Yeh ek symbol woh "handshake" hai jo fly-away hyperbola ko Sun-cruise ellipse se glue karta hai.
Definition Specific energy
ε
"Specific" matlab per kilogram , isliye hum spacecraft ka mass saath nahi lete. Ek orbit ki energy ke do parts hain:
ε = motion (kinetic) 2 v 2 − well mein gehraai (potential) r μ .
Intuition Gravity well ka picture
Socho ek smooth funnel: central body ke paas deep, door flat. − μ / r term kitna deep ho (negative = funnel mein neeche). v 2 /2 term tumhari speed hai. Unka sum constant rehta hai jab tum coast karte ho — depth ko speed se trade karo aur wapas, jaise ek skateboarder bowl mein.
ε < 0 : funnel mein trapped → ellipse (wapas aata hai).
ε = 0 : exactly escape karta hai → parabola .
ε > 0 : spare speed ke saath escape karta hai → hyperbola , aur woh spare speed exactly v ∞ hai, kyunki door (r → ∞ ) depth term gayab ho jaata hai aur ε = 2 1 v ∞ 2 .
Yeh single conserved quantity isliye vis-viva formula (agle mein) exist karta hai, aur isliye well mein deep burn karna sasta hota hai.
Do useful special cases seedhe nikalte hain:
Circle (r = a ): v c = μ / r .
Escape (a → ∞ , isliye 1/ a → 0 ): v esc = 2 μ / r — 2 isliye hai ki escape speed circular speed ka 2 × hoti hai.
Definition Exponents jo tumhe fluently padhne chahiye
r 2 matlab r × r ; r 3 matlab r × r × r .
Square root x poochta hai "kaunsa number times itself x deta hai?" — yeh squaring ko undo karta hai, isliye v 2 = … ko v ke liye solve karne ke liye root chahiye.
Fractional power x 2/5 matlab "fifth root lo, phir square karo" (ya square karo phir fifth-root — same thing). Yeh SOI radius mein aata hai kyunki ek r 5 = … equation ko 1/5 power se undo kiya jaata hai.
2/5 se kyun darna nahi chahiye
Parent ki derivation r 5 = a p 5 ( m p / m ⊙ ) 2 par khatam hoti hai. r ko free karne ke liye, dono sides ka fifth root lo: left par 5 cancel ho jaata hai, aur ( m p / m ⊙ ) 2 ban jaata hai ( m p / m ⊙ ) 2/5 . Mysterious 2/5 bas itna hi hai — ek squared ratio ka fifth root.
π aur half-orbit time
π ≈ 3.14159 circle ke edge ka diameter se ratio hai. Orbital periods isko carry karte hain kyunki "poora chakkar lagana" ek full turn hai. Parent ka transfer time
t = π a t 3 / μ ⊙
ek full elliptical period T = 2 π a 3 / μ ka aadha hai — 2 ek bare π mein drop ho gaya kyunki Hohmann transfer exactly aadha lap hai. Woh period formula disguise mein Kepler's third law hai.
Δ v ("delta-vee")
Greek Δ (capital delta) matlab mein badlaav . Toh Δ v woh speed mein badlaav hai jo engine burn produce karta hai. Yeh ek manoeuvre ka asli "cost" hai — zyada Δ v matlab zyada fuel.
Δ v = v after − v before .
Departure burn ki cost Δ v = v p − v c i r c hai: apni circular speed ko hyperbola ki perigee speed tak utha lo.
gravitational parameter mu
heliocentric transfer ellipse
sphere of influence radius
Har foundation box ek symbol hai jo tumne abhi seekha; arrows dikhate hain ki woh parent-note ka kaunsa result power karta hai.
Jab yeh symbols automatic feel hone lagein, parent directly inhi par lean karta hai: Sphere of influence , Hohmann transfer orbit , Hyperbolic escape trajectories , Oberth effect , aur timing ke liye Launch windows & synodic period .
Answers cover karo; tum ready ho jab har ek instant ho.
μ matlab... ::: G times central body ka mass — "pulling strength," isliye use karte hain taaki G aur M alag alag na carry karne paden.
r hamesha pehle ek question demand karta hai, yani... ::: "kis body se distance?" (cruise mein Sun, fly-by mein planet).
Hohmann transfer ka semi-major axis hai... ::: a t = ( r 1 + r 2 ) /2 , near aur far distances ka average.
Specific orbital energy ke do parts hain... ::: kinetic v 2 /2 minus potential μ / r ; unka sum coast ke dauran constant hai.
ε < 0 , = 0 , > 0 kaunse curves dete hain... ::: ellipse, parabola, hyperbola respectively.
v ∞ woh speed hai... ::: planet se infinitely door jaane par jo bachi, us planet ke relative measure ki gayi.
Vis-viva equation hai... ::: v = μ ( 2/ r − 1/ a ) .
Escape speed circular speed se ek factor se related hai... ::: 2 (escape = 2 μ / r , circular = μ / r ).
x 2/5 matlab... ::: fifth root lo aur square karo (ek r 5 equation ko undo karta hai).
Δ v matlab... ::: ek burn se speed mein badlaav — ek manoeuvre ka fuel "cost."
Ek elliptical period ka aadha hai... ::: t = π a 3 / μ (full period ka 2 ka factor drop ho jaata hai).