3.2.26 · HinglishOrbital Mechanics & Astrodynamics

Patched conic method — interplanetary trajectory design

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3.2.26 · Physics › Orbital Mechanics & Astrodynamics


KYA patch ho raha hai?

Hum poori trip ko teen conic patches mein divide karte hain:

  1. Departure hyperbola — Earth ke SOI ke andar, Earth central body hai. Spacecraft ek hyperbola pe nikal jaati hai.
  2. Heliocentric transfer ellipse — SOIs ke beech mein, Sun central body hai. Zyaadatar ek Hohmann-type ellipse hoti hai.
  3. Arrival hyperbola — target ke SOI ke andar, target planet central body hai.
Figure — Patched conic method — interplanetary trajectory design

SOI radius mein woh power KYU hai? (Derivation)

YEH kyun sahi lagta hai: planet ke paas ( chota) (planet clearly jeet ta hai); door jaane pe (Sun clearly jeetta hai). Yahi crossover SOI hai.


Transfer design KAISE karte hain: heliocentric leg


Departure/arrival hyperbola KAISE design karte hain


Worked Example 1 — Earth→Mars Hohmann heliocentric speeds

Use , m, m.

  • m. Kyun? Ellipse dono orbits ko touch karti hai.
  • m/s. Kyun? Earth ki circular speed baseline set karti hai.
  • m/s. Kyun? Transfer ke perihelion pe vis-viva.
  • m/s ≈ 2.94 km/s. Kyun? Woh speed jo departure hyperbola ko deliver karni hai.

Worked Example 2 — 200 km LEO se Departure

m³/s², m, km/s.

  • km/s. Kyun? Parking-orbit speed.
  • m/s ≈ 11.40 km/s. Kyun? Hyperbolic perigee speed.
  • km/s. Kyun? Injection burn.

Worked Example 3 — Transfer time

Ellipse ki period ka aadha: . Kyun? Hohmann aadha orbit hota hai. s ≈ 259 days.



Recall Feynman: 12-saal ke bachhe ko explain karo

Socho ek fast-ghoomte merry-go-round (Earth) se ek aur merry-go-round (Mars) pe ball phenko jo ek lamppost (Sun) ke around ghoom raha hai. Lamppost, apna merry-go-round, aur doosra — teeno ek saath sochna bahut mushkil hai. Isliye hum trip ko chapters mein kaatte hain: Chapter 1 — sirf tumhara merry-go-round matter karta hai, tum dodte ho aur choddte ho (ek curved escape path). Chapter 2 — ab sirf lamppost matter karta hai, ball Mars ki taraf ek lambe looping arc pe swing karti hai. Chapter 3 — pakad te waqt sirf Mars ka merry-go-round matter karta hai. Har chapter ek easy shape hai jo hum pehle se draw karna jaante hain. Phir hum chapters ko aise jod te hain ki ball kabhi jump na kare. Yahi jodhna "patch" hai.


Connections

  • Vis-viva equation — yahan har speed ka engine.
  • Hohmann transfer orbit — sabse sasta heliocentric ellipse.
  • Hyperbolic escape trajectories — departure/arrival legs.
  • Oberth effect — deep burns efficient kyun hote hain.
  • Sphere of influence — woh boundary jo har patch define karti hai.
  • Kepler's laws — guarantee karti hain ki har patch ek conic hai.
  • Launch windows & synodic period — jab Mars sahi jagah ho.
Patched conic method ki core assumption
Kisi bhi instant pe sirf ek body ki gravity dominate karti hai, isliye motion ek two-body conic hai.
Sphere-of-influence radius ka formula
.
2/5 power kyun hai?
Planet-frame aur Sun-frame perturbation ratios ko equal set karne pe milta hai.
Vis-viva equation
, energy se.
Hohmann semi-major axis
.
Hyperbolic excess speed ka matlab
SOI boundary pe planet ke relative speed (planet frame mein jaane pe).
Departure hyperbola pe perigee speed
.
Departure injection
.
kyun hai?
Oberth effect: energy conservation ka matlab hai ki well ke deep mein burn karne se sasta pad ta hai.
Earth→Mars ke liye heliocentric departure excess
km/s.
Hohmann transfer time
(ellipse period ka aadha), Earth→Mars ke liye ~259 days.
Kya SOI ek real physical wall hai?
Nahi — yeh ek approximation hai; asli gravity field continuous hai.

Concept Map

simplified by

assumes

defines

radius from equal perturbations

stitches three patches

stitches three patches

stitches three patches

inside Earth SOI

inside target SOI

usually a

solved by

solved by

solved by

Many-body problem unsolvable

Patched conic method

One dominant body assumption

Sphere of influence

r_SOI = a_p times mass ratio ^2/5

Departure hyperbola near Earth

Heliocentric transfer ellipse

Arrival hyperbola near target

Hohmann transfer ellipse

Kepler two-body solutions