3.2.4 · D1 · Physics › Orbital Mechanics & Astrodynamics › Orbit shape from eccentricity — circle (e=0), ellipse (0 - e
Gravity ke under move karne wala koi bhi body hamesha ek conic section trace karta hai, aur ek akela dimensionless number — eccentricity e — batata hai ki kaun sa (circle, ellipse, parabola, ya hyperbola). Parent page par jo bhi hai woh sirf yeh carefully unpack karta hai ki e kaise do conserved quantities (energy aur angular momentum) se paida hota hai aur e ki har value kaun sa shape draw karti hai.
Yeh page har woh symbol build karta hai jis par parent note rely karta hai, ek smart 12-saal-ke-bacche ke toolkit se shuru karke aur kuch nahi. Upar se neeche padho — har block sirf wahi cheezein use karta hai jo uske upar define ho chuki hain.
M aur m — do masses
==M badi central mass hai (Sun, ya ek planet) jo centre mein still baith ke kheenchti hai. m chota orbiting body hai== (planet, comet, ya spacecraft) jo kheencha jaata hai. Dono kilograms mein measure hote hain.
Picture: ek bhaari bowling ball M jo ek stretched sheet par raki hai, aur ek halka marble m jo us dip ke around roll kar raha hai jo woh banata hai.
r — distance
r simply ==yeh hai ki orbiting body m central mass M se kitni door hai==, ek ruler se mapa gaya. Yeh ek positive length hai. Symbols mein yeh metres (ya kilometres, ya astronomical units) ka ek number hai.
Picture: Sun se ek planet tak kheenchi gayi seedhi line. Iska length r hai.
θ — angle
θ (Greek letter "theta") woh ==angle hai jitna line r ne sweep kiya hai==, ek chosen starting direction se measure kiya gaya. Hum angles degrees (0 ∘ se 36 0 ∘ tak) ya radians mein measure karte hain.
Picture: Sun par khado, wahan point karo jahan planet sabse paas tha, use θ = 0 kaho. Jaise-jaise planet ghoomta hai, pointer muda; jitna woh muda hai woh θ hai.
Saath mein ( r , θ ) polar coordinates hain — ek "kitni door, kis taraf" address. Isliye poora topic r ( θ ) ke roop mein likha gaya hai: mujhe direction do, main distance bata dunga.
x , y kyun nahi?
Gravity centre ki taraf line ke saath kheenchti hai. Woh line exactly woh direction hai jis taraf r point karta hai. Isliye gravity problem describe karne ke liye natural coordinate "centre se distance-aur-angle" hai, na ki x , y boxes ki grid. Maths kaafi saaf nikal ke aata hai.
Focus ek fixed point hai jiske around ek conic curve build hoti hai. Central mass M ek focus par baith'ti hai. Hamare orbit ke liye, focus origin hai — woh jagah jahan r = 0 hai.
Picture: woh pin jo aap zameen mein thokoge; orbit us pin ke relative draw hoti hai, loop ke geometric centre ke relative nahi.
Yeh matter karta hai kyunki — ek baar jab hum baad mein orbit equation build kar lenge — distance r hamesha focus se measure hogi, na ki geometric centre se. Sun focus par hai, ellipse ke ek taraf — kabhi uske middle mein nahi.
Intuition Ek equation se chaar shapes kyun milti hain
Ek hollow ice-cream cone lo aur use flat blade se seedha kaato. Cut ke tilt ke hisaab se tumhe circle, ellipse, parabola, ya hyperbola milega. Yeh chaar Conic Sections hain — literally "cone ke sections (slices)". Gravity ki orbit equation in slices ki algebra hai, isliye exactly yeh chaar shapes (aur koi nahi) appear hoti hain.
e (shape score)
Eccentricity e ek akela dimensionless number hai (e ≥ 0 ) jo record karta hai ki slice kitna "un-circular" hai: cutting blade kitna tilted tha.
e = 0 : blade horizontal → circle
0 < e < 1 : blade thoda tilted → ellipse (ek closed oval)
e = 1 : blade cone ki side ke parallel → parabola (barely open)
e > 1 : blade itna steep ki cone ke dono halves ko kaate → hyperbola (wide open)
Picture: 0 se upar ek dial; jaise-jaise tum use ghumaate ho, loop stretch hota hai, phir snap ho ke khul jaata hai.
Energy aane se pehle, ek ellipse ki shape ko teen lengths chahiye.
a — semi-major axis
==a ellipse ke longest diameter ka aadha hai== — centre se door end tak ki distance.
Picture: ellipse ka lamba "radius".
c — focal distance
==c ellipse ke centre se ek focus tak ki distance hai==. Bada c = focus middle se door = zyada squashed.
Picture: pin kitni off-centre hai.
p — semi-latus rectum
==p woh distance r hai jo focus se long axis ke right angle par measure ki gayi hai==. Ellipse par yeh "focus par half-width" hai.
Picture: focus par khado, long axis ke right angle mein dekho; curve tak ki distance p hai.
p = a ( 1 − e 2 ) kyun hai — ek "kyun", koi leap nahi
p ek width hai aur a ek length hai; unka related hona zaroori hai. Figure s03 dekho: sabse paas ka point (perihelion) focus se a − c distance par hai, aur sabse door (aphelion) a + c par. Ellipse ki ek standard property — "do foci tak distances ka sum constant hai" definition se nikali gayi — yeh hai ki semi-latus rectum barabar hai
p = a a 2 − c 2 .
Kyunki e = c / a ka matlab hai c = e a , numerator hai a 2 − e 2 a 2 = a 2 ( 1 − e 2 ) , isliye
p = a a 2 ( 1 − e 2 ) = a ( 1 − e 2 ) .
Toh p shrink hota hai jaise e badhta hai: orbit jitni zyada stretched, focus par utni narrow. (Ek lookalike se bachna: quantity ( a − c ) ( a + c ) = a 2 − c 2 semi-minor axis ke square b ke barabar hai, yaani b 2 , na ki p 2 — dono ko confuse mat karo.)
Ab hamare paas p purely geometry se hai. Baad mein, jab angular momentum aur gravity ki strength define ho jaayegi (Sections 6 aur 8), wohi p dobara p = h 2 / μ ke roop mein appear hoga — same width ki physics value. p ka yeh double life exactly wahi hai jo orbit ki shape ko body ki motion se jodta hai, lekin hum woh formula honestly tab tak nahi likh sakte jab tak woh symbols exist na karein.
cos θ — cosine
Ek angle θ ke liye, cos θ ek number hai − 1 aur + 1 ke beech jo batata hai ki ==direction θ "reference axis ke along" kitna point karta hai==. Yeh θ = 0 ∘ par + 1 hai, 9 0 ∘ par 0 hai, aur 18 0 ∘ par − 1 hai.
Picture: ek unit-length pointer ka woh shadow jo horizontal axis par padta hai jab woh rotate karta hai.
Ab jab hamare paas p , e , aur cos θ hain, hum finally woh orbit equation padh sakte hain jo parent state karta hai:
r ( θ ) = 1 + e c o s θ p
Isme har symbol ab earn ho chuka hai. (θ = 9 0 ∘ par, cos 9 0 ∘ = 0 , isliye r = p — exactly isliye p "width at the focus" hai jaise humne upar define kiya.)
Intuition Cosine kyun, sine kyun nahi?
Humne θ = 0 ko closest approach (perihelion) ki direction chose kiya. Hum chahte hain ki r wahan sabse chhota ho, matlab denominator 1 + e cos θ wahan sabse bada hona chahiye. Cosine θ = 0 par + 1 hai — perfect, yeh denominator ko exactly perihelion par sabse bada banata hai. Sine θ = 0 par 0 hota aur closest point galat jagah rakhta. Isliye cosine woh tool hai jo "orbit ko apni chosen start ke saath line up karta hai."
Yeh single fact parent ke poore "read off the denominator" argument ko drive karta hai: denominator shrink hota hai jaise θ 18 0 ∘ ki taraf badhta hai (cos − 1 ki taraf fall karta hai), aur r badhta hai.
Common mistake Domain trap: jab
e > 1 , har θ allowed nahi hai
Kyun problem hoti hai: circle ya ellipse ke liye (e < 1 ), 1 + e cos θ hamesha positive hai — θ = 18 0 ∘ par sabse chhota jahan woh 1 − e > 0 equals karta hai — isliye har angle ek valid positive r deta hai aur curve band ho jaati hai.
Edge case: hyperbola ke liye (e > 1 ), denominator zero hit karta hai jab cos θ = − 1/ e , aur us se aage negative ho jaata hai. Negative r unphysical hai. Isliye body sirf un angles par orbit par exist karti hai jahan 1 + e cos θ > 0 hai, yaani cos θ > − 1/ e . Woh forbidden angles incoming/outgoing asymptotes hain — woh directions jis se body aati hai aur jis mein escape karti hai.
Knife-edge (e = 1 , parabola): denominator 1 + cos θ zero reach karta hai sirf θ = 18 0 ∘ par (aur kahi negative nahi jaata), isliye r → ∞ exactly ek direction mein. Domain har angle hai sirf us ek escape direction ko chhor kar.
Definition Dot — rate of change
Kisi symbol ke upar dot ka matlab hai woh per second kitni tezi se change ho raha hai . Toh θ ˙ ("theta-dot") angle kitni tezi se ghoom raha hai — angular speed.
Picture: ghadi ki second hand; θ ˙ uski turning rate hai.
Intuition Rate ki zaroorat kyun hai
Ek shape akele nahi bata sakti ki body wapas aayegi ya nahi . Yeh motion se decide hota hai — speeds aur kaise woh trade off karte hain. Rates of change motion ki language hain, isliye unhe enter karna hoga.
h — specific angular momentum
==h = r 2 θ ˙ orbit ka spin-content hai, orbiting body m ke per kilogram measure kiya gaya.== "Specific" ka hamesha matlab "per unit mass" hota hai. Kyunki gravity kuch bhi sideways torque nahi karti, h orbit ke dauran kabhi nahi badalti — yeh conserved hai.
Picture: ek figure-skater; arms in (chhota r ) → tezi se spins (bada θ ˙ ); arms out (bada r ) → dheere spins. Product r 2 θ ˙ fixed rehta hai.
L — total angular momentum
L = m h = m r 2 θ ˙ poore body ka spin-content hai, jahan m Section 1 se orbiting mass hai. h se sirf yahi fark hai ki mass factor m hai.
L ::: poore body ke liye (= mh ); h ::: per kilogram. Parent dono use karta hai — mass m ke through dono ko straight rakhna.
Connection dekho Angular Momentum in Orbits : h woh width p = h 2 / μ fix karta hai (isme μ Section 8 mein define hai).
E — total energy
E body ki kinetic energy (move karne se) plus gravitational potential energy (well mein hone se) , saath mein add kiya gaya. Yeh conserved hai.
Picture: ek bowl mein marble. Total energy = (kitni tezi se roll kar raha hai) + (wall par kitna upar hai), aur yeh total bina friction ke kabhi nahi badalti.
U — gravitational potential energy
==U body ki "well mein height" energy hai==: mass ke paas trapped hone ke liye woh kitni energy "owes" karti hai. Is usual choice ke saath ki U → 0 infinitely door, yeh hai
U = − r GM m ,
jahan G aur M gravity ka constant aur central mass hain (Section 8 G finish karta hai; M Section 1 se hai). Yeh negative hai kyunki body door rim se neeche hai. Toh total energy honestly E = 2 1 m v 2 + U = 2 1 m v 2 − r GM m hai, jahan v body ki speed hai.
Picture: bowl mein jitna deep (chhota r ), U utna zyada negative — bahar niklna utna mushkil.
ε — specific energy
ε = E / m total energy per kilogram hai (orbiting mass m se divide karke). Same idea, mass divided out.
ε ::: energy per unit mass E / m .
Intuition Energy ka SIGN poori kahani kyun hai
Potential energy U ko infinitely door zero set karo (jaise upar). Tab:
ε < 0 : body well ke rim ke neeche fasi hai — kabhi bahar nahi nikal sakti → bound → closed orbit (circle/ellipse).
ε = 0 : uske paas exactly itna hai ki rim tak pahunche, zero speed ke saath pahunche → marginal escape → parabola.
ε > 0 : woh energy bachao ke saath bahar nikalti hai, infinity par bhi move karti rahti hai → unbound → hyperbola.
Isliye parent ki table har shape ko ε ke sign ke saath pair karti hai.
Figure s04 exactly yahi draw karta hai. Curved chalk line potential well U = − GM m / r hai: centre ke paas steep aur deep, door "rim" (energy = 0 ) ki taraf flat hoti jaati hai. Body ki total energy ek horizontal level line hai — kyunki energy conserved hai, body move hone par flat rehti hai. Figure aise padho: blue level rim ke neeche baith'ti hai (ε < 0 ) isliye body kabhi right edge tak nahi pahunch sakti → woh trapped hai → ellipse. Pink dashed level exactly rim par hai (ε = 0 ) → yeh barely infinity tak pahunchti hai → parabola. Yellow level rim ke upar hai (ε > 0 ) → yeh height bachao ke saath infinity tak pahunchti hai → hyperbola.
Dekho Specific Orbital Energy aur Escape Velocity (ε = 0 boundary), aur Vis-viva Equation (jo ε ko kisi bhi r par speed mein convert karta hai).
G — gravitational constant
==G nature ka ek fixed number hai== (G ≈ 6.674 × 1 0 − 11 SI units mein) jo batata hai ki gravity poore universe mein kitni strong hai. Yeh ek pebble aur ek galaxy ke liye same hai.
Picture: universal "exchange rate" jo masses-aur-distances ko ek pulling force mein convert karta hai.
μ — standard gravitational parameter
==μ = GM == gravitational constant G ko central mass M (Section 1 se) ke saath ek number mein bundle karta hai. Yeh is particular Sun/planet ka pull ka strength set karta hai.
Picture: ek single knob jisme "yeh central body cheezein kitni tezi se pakad'ti hai."
G aur M ko bundle kyun karein? Kyunki yeh orbit maths mein hamesha saath appear hote hain, isliye ek symbol μ carry karna cleaner hai. Yeh p = h 2 / μ mein appear karta hai (ab isme har symbol — p , h , μ — define hai) aur e = 1 + 2 ε h 2 / μ 2 mein.
ε ka sign seedha padho:
ε < 0 ⇒ square-root ke andar 1 se kam → e < 1 ⇒ ellipse/circle .
ε = 0 ⇒ e = 1 = 1 ⇒ parabola .
ε > 0 ⇒ e > 1 ⇒ hyperbola .
Woh single formula poora parent topic compressed hai. Baaki sab decoration hai.
Neeche diya diagram is page ka dependency order dikhata hai: geometry symbols (left) orbit equation build karte hain, motion symbols (right) eccentricity–energy relation build karte hain, aur dono streams us four-shape classification mein merge hoti hain jo parent topic hai . Arrow ko "pehle chahiye" padho. Yeh reading order visible ho gaya — koi bhi downstream symbol koi aisa symbol use nahi karta jo uske upstream na ho.
Polar coordinates r and theta
Orbit equation r of theta
Focus at the central mass
Cosine lines up perihelion
Conic sections from cone slices
Eccentricity e equals c over a
Specific angular momentum h
e from energy and momentum
Potential energy U equals minus GMm over r
Gravity strength mu equals GM
Orbit shape from eccentricity
Saari streams parent topic ko feed karti hain.
Khud test karo — right side cover karo aur reveal karne se pehle har ek ka jawab do.
Do masses M aur m kya hain? M bada central body hai jo kheenchta hai; m chota orbiting body hai jo kheencha jaata hai.
Do numbers ( r , θ ) kya batate hain? Body kitni door hai aur kis direction mein, central mass se measure kiya gaya.
Orbit par central mass kahan baith'ti hai? Ek focus par (origin, r = 0 ), kabhi ellipse ke centre mein nahi.
Chaar orbit shapes geometrically kahan se aati hain? Yeh cone ko flat plane se slice karne ke chaar tarike hain — conic sections.
Kya eccentricity ek length hai ya ratio, aur yeh kya hai? Ek dimensionless ratio, e = c / a (focal distance over semi-major axis).
Semi-latus rectum p kya hai, aur p = a ( 1 − e 2 ) kyun? Focus par width r (θ = 9 0 ∘ ); p = ( a 2 − c 2 ) / a = a ( 1 − e 2 ) kyunki c = e a .
( a − c ) ( a + c ) kya equals karta hai, aur yeh p 2 kyun NAHI hai?Yeh a 2 − c 2 = b 2 equals karta hai, semi-minor axis ka square — p 2 nahi.
r ( θ ) mein cos θ (na ki sin θ ) kyun appear karta hai?Kyunki cos 0 ∘ = 1 r ko θ = 0 par sabse chhota banata hai, hamara chosen closest point (perihelion).
e > 1 ke liye, kaun se angles allowed hain aur kyun?Sirf cos θ > − 1/ e , taaki 1 + e cos θ > 0 r ko positive rakhe; us se aage r negative hoga (unphysical).
Kisi symbol ke upar dot ka kya matlab hai, e.g. θ ˙ ? Per second rate of change; θ ˙ angular speed hai.
Specific angular momentum h kya hai, aur conserved kyun hai? h = r 2 θ ˙ , spin per unit mass; conserved kyunki gravity koi sideways torque exert nahi karti.
h aur L mein kya fark hai?L = mh ; L total hai, h per unit mass m hai.
Gravitational potential energy U kya hai? U = − GM m / r , negative aur infinity par zero — "well mein height" energy.
Specific energy ε kya hai aur uska sign kyun matter karta hai? ε = E / m ; uska sign decide karta hai bound (< 0 ), marginal (= 0 ), ya unbound (> 0 ).
G aur μ kya hain?G universal gravitational constant hai; μ = GM use central mass ke saath bundle karta hai us body ki pull strength dene ke liye.
Eccentricity–energy relation batao.