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FoundationsKepler's first law — orbits are conic sections

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3.2.5 · D1 · Physics › Orbital Mechanics & Astrodynamics › Kepler's first law — orbits are conic sections

Parent note Kepler's first law padhne se pehle, tumhe genuinely har symbol ka malik banna hoga jo woh use karta hai. Yeh page har ek ko zero se banata hai — simple words mein, phir ek picture, phir kyun yeh topic uske bina nahi chal sakta.


1. Position: planet kahan hai? ( aur )

Imagine karo tum Sun par khade ho, ek planet ko apne around swing karte dekh rahe ho. Exactly yeh batane ke liye ki woh kahan hai, tumhe do numbers chahiye:

  • Woh kitna door hai — isse kaho, Sun se planet tak ki doori.
  • Woh kis direction mein hai — isse kaho, woh angle jitna tumhe uski taraf point karne ke liye turn karna hoga.
Figure — Kepler's first law — orbits are conic sections

Yeh topic ko kyun chahiye. Kepler's first law ka poora goal orbit ki shape ke liye ek formula hai. Shape ek rule hai jo kehta hai "har direction ke liye, planet is doori par baithta hai." Exactly yahi ka matlab hai — padho isse " ka function ," yaani mujhe ek angle do, main tumhe doori dunga. Ordinary left–right / up–down coordinates bhi kaam karte, lekin kyunki gravity seedha Sun ki line par kheenchti hai, distance-and-angle use karne se mathematics dramatically cleaner ho jati hai.


2. Dots: rates of change (, , )

Planet move karta hai, isliye aur frozen nahi hain — woh time ke saath change hote hain. Physicists ek symbol ke upar ek chhota dot likhte hain matlab "yeh per second kitni tezi se change ho raha hai."

ko imagine karo jaise Sun se planet tak ki spoke par ek bead slide karne ki speed; ko us spoke ki speed jaise woh clock hand ki tarah sweep kare.


3. Do masses aur

Inhe mein bundle kyun karein? Har orbit equation mein combination ek single lump ki tarah appear karta hai — chhote planet ki mass cancel ho jati hai (ek pankh aur ek cannonball same tarah girte hain). Isliye hum lump ko ek naam dete hain, , algebra tidy rakhne ke liye. Two-body problem and reduced mass dekho fine print ke liye jab ko ignore kiya ja sakta hai.


4. Inverse-square pull aur yeh kaise acceleration banta hai

Yeh poori kahaani ka engine hai. Gravity ki strength constant nahi hai — yoh doori ke saath fade hoti hai, aur specifically yeh doori-squared ke reciprocal ke roop mein fade hoti hai.

Figure — Kepler's first law — orbits are conic sections

Topic ko exactly yahi law kyun chahiye. Jaise parent note stress karta hai, sirf shape clean, closed, non-repeating orbits produce karta hai (dekho Inverse-square law and Bertrand's theorem). Thoda alag power — maano — orbits ko spiral ya precess karayega instead of ek fixed ellipse trace karne ke. Kepler's first law ka magic is specific power law ka gift hai.


5. Chhoti hat: direction ()

Toh "" padho: strength ki ek pull, ke opposite aim ki gayi — yaani inward, wapas Sun ki taraf. Minus sign "outward" ko "inward" mein flip karta hai.

Topic ko yeh kyun chahiye. Force ek vector hai — iska ek size aur ek direction hota hai. woh tarika hai jisse hum size par direction bolt karte hain. Iske bina hum sirf kitna hard bol sakte, kaun si taraf nahi.


6. Central force aur angular momentum ()

Kyunki gravity hamesha exactly ke along point karti hai — seedha Sun ki taraf — ise central force kehte hain. Yeh single fact humein ek khazana deta hai: ek quantity jo kabhi change nahi hoti.

Figure — Kepler's first law — orbits are conic sections

Topic ko yeh kyun chahiye. ka constant rehna woh lever hai jo derivation use karta hai time erase karne aur pure geometry paane ke liye. Yeh secretly Kepler's second law bhi hai, Kepler's second law — equal areas in equal times: constant matlab spoke equal areas sweep karta hai equal times mein.


7. Radial equation of motion (force actually kya drive karti hai)

Jab ek baar tumhare paas inward acceleration aur constant hain, Newton's second law in–out (radial) direction mein ek single equation ban jata hai:

Yeh exist kyun karta hai. Polar coordinates mein true radial acceleration sirf nahi hoti; around swing karna ek outward term add karta hai (wahi effect jo tumhe merry-go-round par outward throw karta hai). Net radial acceleration ko inward pull ke equal set karne se upar wala equation milta hai. Yeh woh single relation hai jo parent note solve karta hai — constant use karke time erase karte hue — orbit shape par pahunchne ke liye. Tumhe ise yahan solve karne ki zaroorat nahi; tum bas ise pehchano jab neeche ka flowchart ise point kare.


8. Conic family (, , aur )

Conic section koi bhi curve hai jo tum ek cone ko ek flat plane se slice karke paate ho: plane ko alag-alag taraf jhukao aur circles, ellipses, parabolas, hyperbolas milte hain. Full geometry Conic sections — geometry of ellipse, parabola, hyperbola mein hai.

Figure — Kepler's first law — orbits are conic sections

Formula padhna, sab cases ( perihelion par):

  • (perihelion, closest): , denominator biggest, smallest .
  • : , exactly.
  • (aphelion, farthest): , denominator smallest, largest (sirf finite agar ).
  • Agar , toh kisi angle par , jisse — curve infinity tak chala jata hai aur kabhi return nahi karta. Yeh precisely ek escape trajectory hai.

Topic ko yeh kyun chahiye. Yeh target hai: prove karna ki orbits is formula ko follow karti hain yahi hai Kepler's first law.


9. Energy per unit mass () aur speed ()

Parent note ise ke saath tie karta hai: dekho square root ko se neeche shrink karta hai (ellipse), exactly deta hai (parabola), se upar push karta hai (hyperbola). Energy ka sign → conic ka type. Perfect harmony.


Sab kuch kaise fit hota hai

Polar coords r and theta

Rates r-dot theta-dot

Masses M m and G bundled as mu

Inverse-square pull

Acceleration per mass a = mu over r squared

Direction hat r

Central force zero torque

Angular momentum h constant

Radial equation of motion

Orbit shape r of theta

Conic family p and e

Energy E and speed v

Which conic ellipse parabola hyperbola

Keplers first law

Ise top-down padho: coordinates aur masses force feed karte hain; force ko planet ki mass se divide karne par acceleration milta hai; force central hone se freeze hota hai; acceleration aur milke radial equation of motion dete hain; use solve karne par shape milti hai, jo ek conic se match karti hai; energy tab batati hai ki kaun si conic hai.


Equipment checklist

Apne aap test karo — right side cover karo aur reveal karne se pehle jawab do.

Do polar coordinates aur kya measure karte hain?
= Sun se planet tak ki doori; = ek fixed reference se us direction ka angle.
Ek symbol ke upar dot (jaise ) ka kya matlab hai?
Time-derivative — woh quantity per second kitni tezi se change hoti hai.
Hum ko ek single symbol mein kyun bundle karte hain?
Kyunki hamesha saath appear karta hai aur planet ki apni mass cancel ho jati hai, isliye ek symbol algebra clean rakhta hai.
kya hai aur inverse-square law iske baare mein kya kehta hai?
gravitational force hai ; yeh doori-squared ke reciprocal ke roop mein fall off karta hai.
se kaise milta hai?
Force ko planet ki mass se divide karo (Newton's second law); 's cancel ho jaate hain, bachta hai.
kya hai aur uski length kya hai?
Ek unit vector (exactly length) Sun se outward planet ki taraf point karta hua — pure direction.
Angular momentum gravity ke liye constant kyun hai?
Gravity ek central force hai jo seedha Sun ki taraf point karti hai, isliye woh Sun ke baare mein zero torque exert karti hai.
Radial equation of motion kya hai?
— net radial acceleration inward gravitational pull ke equal hai.
mein, aur kya control karte hain, aur kahan point karna chahiye?
size set karta hai, shape; perihelion (closest approach) ki taraf point karna chahiye.
Orbit bound hai ya unbound, yeh kya decide karta hai?
Total energy ka sign: negative → bound ellipse, zero → parabola, positive → unbound hyperbola.
Recall Ready check

Agar tum upar ke sab das questions bina dekhke answer kar sakte ho, toh tum parent note mein poori derivation padhne ke liye equipped ho.