3.2.5 · D5 · HinglishOrbital Mechanics & Astrodynamics
Question bank — Kepler's first law — orbits are conic sections
3.2.5 · D5· Physics › Orbital Mechanics & Astrodynamics › Kepler's first law — orbits are conic sections
True or false — justify karo
Sun planet ki elliptical orbit ke geometric center par baithta hai.
False. Ek ellipse ke do foci aur ek alag center hota hai; Sun ek focus par hota hai. Doosra focus aur center dono space mein empty points hain.
Ek nearly circular orbit () ke liye do foci merge hokar ek single point ban jaate hain.
True. Focus–center distance hai, toh focus–focus separation jab ; dono foci aur center coincide karte hain — woh limiting shape circle hai, isliye chote ke liye "Sun-at-center" ka illusion hota hai.
Circular orbit sirf zero eccentricity wala ek ellipse hai.
True. mein set karne se milta hai, jo constant hai — ek circle. Circle conic family ka ek genuine special case hai, koi alag law nahi.
family ka har conic ek possible gravitational orbit hai.
True. Ek hi derivation () inhe sab produce karta hai; kaun sa milega woh initial energy se fix hota hai, jisse milta hai.
wala orbit ek mathematical curiosity hai jo nature mein kabhi nahi hota.
False. Hyperbolic () trajectories real unbound flybys hain; interstellar object ʻOumuamua ka tha. "Bound vs unbound" energy sign se set hota hai, ki kisi cap se nahi.
Ek elliptical orbit par planet ki speed har jagah same hoti hai.
False. Sirf circle () mein constant speed hoti hai. ke liye body perihelion par sabse fast aur aphelion par sabse slow hoti hai — yeh Kepler's second law in action hai.
Semi-latus rectum orbit ki radius ke barabar hai un do points par jahan hai.
True. par, , toh exactly hai. Yahi ka geometric meaning hai: major axis ke perpendicular measure ki gayi focus-to-curve distance.
Angular momentum badhane par (fixed aur fixed negative energy ke saath) orbit rounder ho jaata hai.
True. se, ke saath, term negative hai aur badhne par aur zyada negative hota jaata hai, toh decrease karke ki taraf jaata hai — orbit rounder hota jaata hai (circle given energy ke liye maximum- orbit hai).
Error dhundo
" par denominator sabse bada hota hai, toh sabse bada hai — woh aphelion hai."
Beech mein error hai: denominator ko sabse chota () banata hai, jo ko sabse bada banata hai. Conclusion (aphelion at ) sahi hai, lekin reason ulta hai — chota denominator, bada .
"Kyunki distance measure karta hai, hum ko ellipse ke center se measure karte hain."
Error: focus se measure kiya jaata hai (polar frame ka origin), kyunki wahi origin hai jahan attracting mass baithta hai. Center se measure karne par yeh clean single-focus equation nahi milegi.
"Parabolic orbit () ka matlab hai object bound hai lekin sabse bade possible ellipse par hai."
Error: bound nahi hai. Yeh exact threshold hai — object infinity tak pahunchta hai zero leftover speed ke saath aur kabhi nahi lautta. Bound orbits ke liye strictly chahiye.
"Kyunki gravity closer in zyada strong hai, planet perihelion ke paas zyada time spend karta hoga."
Error, ulta hai: planet perihelion ke paas sabse fast move karta hai (equal areas in equal times), isliye wahan kam time spend karta hai. Woh aphelion ke paas ruka rehta hai jahan woh rengta hai.
"Angular momentum conserved hai kyunki gravity ek weak force hai."
Error: conservation ka strength se koi lena dena nahi. conserved hai kyunki gravity central hai ( ke along point karta hai), focus ke baare mein zero torque deta hai chahe kitna bhi strong ho.
"Substitution sirf inverse-square law ke liye kaam karta hai; yeh gravity ka ek lucky coincidence hai."
Error: ek general polar-coordinate change of variables hai (jahan ka matlab hai); yeh kisi bhi central-force radial equation ko mein ek form mein convert karta hai. Yeh ke liye especially clean hai (linear driven SHM deta hai), lekin yeh ek tool hai, gravity ka coincidence nahi.
"Agar hai toh object bahut stretched ellipse par hai."
Error: se milta hai, ek hyperbola — ek open, unbound curve. Koi bhi positive-energy orbit kisi bhi ellipse mein close nahi hoti, chahe kitna bhi stretched ho.
Why questions
Sun ek focus par kyun baithta hai, center par kyun nahi?
Kyunki derivation ise force karta hai: solve karne par milta hai, yaani — ek aisi form jiska polar origin (jahan se measure hota hai) attracting mass hai. Woh origin ek focus hai, center nahi, aur woh perihelion () side par off-center baithta hai kyunki term wahan ko sabse chota banata hai. Asymmetry equation mein built-in hai, sirf ek picture nahi.
Linearized orbit ODE ek conic guarantee kyun karta hai, koi aur curve kyun nahi?
Iska general solution hai (jahan ), aur invert karne par exactly milta hai — conic ka polar form. Driven simple harmonic motion se koi aur function type nahi aa sakta.
Closed orbits produce karne ke liye inverse-square power special kyun hai?
Sirf (aur linear spring ) aisi orbits deta hai jo precession ke bina ek revolution ke baad close hoti hain — yeh Bertrand's theorem hai; doosre powers rosette paths dete hain jo kabhi exactly repeat nahi hote. (Inverse-square law and Bertrand's theorem)
Eccentricity ko seedha dekh kar trajectory classify kyun kar sakte hain, energy compute kiye bina?
Kyunki aur same information carry karte hain via : (bound), , . jaanna already energy ka sign fix kar deta hai.
Derivation mein hum time se angle par variables kyun change karte hain?
Hum shape chahte hain, timetable nahi. Angular momentum time ko cleanly eliminate karne deta hai, orbit ki geometry seedhi deliver karta hai. (Conservation of angular momentum in central forces)
Negative total energy bound (returning) orbit ke liye condition kyun hai?
Negative energy ka matlab hai body gravitational potential well mein trapped hai — uske paas infinity tak pahunchne ki energy nahi hai, toh uski distance finite rehti hai aur orbit close hoti hai. (Escape velocity and orbital energy)
Edge cases
Exactly hone par orbit kya hoti hai?
radius ka ek circle; perihelion aur aphelion coincide karte hain aur speed har jagah constant hoti hai. Yeh degenerate ellipse hai jisme dono foci center par hain.
kya hota hai jab us value ke paas jaata hai jahan hota hai (sirf tab possible jab )?
: body ek asymptote ke along infinity ki taraf bhaag jaati hai. ke liye do aisi angles hain (hyperbola ki asymptotic directions); ke liye ek hai, par.
Ek bound ellipse () ke liye, kya denominator kabhi zero reach kar sakta hai?
Nahi. Kyunki hai, denominator kam se kam hota hai ( par), toh finite aur bounded rehta hai — orbit kabhi escape nahi karta.
Parabola () ke liye aphelion kya hai?
Koi aphelion nahi hai. Jaise hota hai denominator aur ; object hamesha ke liye door jaata hai, exactly zero speed ke saath infinity reach karta hai.
Agar angular momentum ho toh orbit equation kya deta hai?
Formula degenerate ho jaata hai: , toh "orbit" ek radial plunge seedhe center mein collapse ho jaati hai. Koi sideways motion nahi hai toh koi conic nahi hai — sirf ek line ke along free-fall.
Eccentricity boundary par, trajectory bound hai ya unbound?
Marginally unbound. Yeh exact dividing line hai (): body escape karti hai lekin infinity par zero remaining speed ke saath pahunchti hai — sabse slow possible escape.
Agar do orbits same share karte hain lekin alag ke saath, kya unka size same hai?
Nahi. Ve same latus-rectum width share karte hain ( par ), lekin alag bahut alag perihelion aur aphelion deta hai — isliye alag overall extent aur shape.