True anomaly from eccentric anomaly ki child note. Yahan hum poori conversion ko zero se redraw karte hain. Har step ko ek tasveer milti hai. Kuch bhi assume nahi kiya gaya — agar koi symbol use kiya, toh aapne usse bante hue dekha hoga.
Kisi bhi formula se pehle, har word ko samajhte hain.
Tasveer dekho. Teal dot center O hai. Uske dayi taraf orange dot focus F hai — notice karo ki yeh center se perihelion ki taraf exactly c=ae push kiya gaya hai.
Hum woh angle chahte hain jo orange focus se dekha jaaye — woh true anomaly ν hai. Lekin jo angle compute karna aasaan hai (Kepler's Equation se, Kepler's Equation) woh teal center se measure hota hai — woh eccentric anomaly E hai. Poora page yeh hai: E diya, ν nikalo.
Yahan exactly E kaise define hota hai. Planet P ko ellipse par lo. Seedha upar (ya neeche) jaao jab tak auxiliary circle par point P′ na aa jaaye. Center O se, perihelion se P′ tak measure kiya gaya angle ==eccentric anomaly E== hai.
Focus perihelion ki taraf c=ae distance par hai — wahi e jo Orbit geometry — semi-major axis and eccentricity mein hai. Bada e = focus center se aur door.
Figure mein orange arrow planet ka position vector hai focus se. Uska horizontal part purana xO minus offset c=ae hai:
1±cosν build karo common denominator par:
1+cosν=1+1−ecosEcosE−e=1−ecosE(1−ecosE)+(cosE−e)=1−ecosE(1−e)(1+cosE)1−cosν=1−ecosE(1−ecosE)−(cosE−e)=1−ecosE(1+e)(1−cosE)
Divide karo — ugly denominator 1−ecosE cancel ho jaata hai:
1+cosν1−cosν=(1−e)(1+cosE)(1+e)(1−cosE)Dono sides par half-angle identity apply karo:
tan22ν=1−e1+etan22E
Figure ν vs E plot karta hai kai e values ke liye, upar ke atan2 recipe se compute kiya. Har baar ek single smooth increasing curve hai — woh monotonicity (ek baar branch correctly choose ho jaaye) hi woh poora reason hai hum yeh form prefer karte hain.
Ek frame poori chain carry karta hai: circle → ellipse par squash → origin ko focus par slide karo (c=ae se) → angle read karo. Teal machinery center world hai (jahan E rehta hai); orange machinery focus world hai (jahan ν rehta hai). Baaki sab Pythagoras aur ek half-angle identity hai.
Recall Feynman retelling — walkthrough plain words mein
Humne oval orbit ke aas-paas ek perfect circle draw kiya aur ek helper angle Emiddle se mark kiya. Circle se seedha neeche slide karne par oval par land karte hain — isi tarah helper angle real planet ko point karta hai. Lekin Sun beech mein nahi baitha; woh ek taraf baitha hai, focus par, c=ae door. Toh humne apna poora coordinate system uthaya aur Sun par slide kar diya. Wahan se humne ek right triangle measure kiya: across, up, aur planet tak slanted distance r. "Across over slant" ne cosν diya; "up over slant" ne sinν diya. Dono milke real angle ν pin kar dete hain bina kisi guessing ke. Ise ek neat recipe banane ke liye, humne ek half-angle trick use ki aur nikla tan2ν=1−e1+etan2E. Square-root factor "Sun-is-off-center" stretch hai: Sun ke paas ek chota helper step ek bada real angle swing karta hai. Ek warning: us ratio ko blindly arctan mat karo — aphelion par yeh blow up karta hai, isliye top aur bottom ko atan2 de do aur woh smooth rehta hai. Round orbit? Koi offset nahi, koi stretch nahi, teenon angles same hain.
Recall
r ko E ke terms mein do. ::: r=a(1−ecosE)r ke liye positive square root kyun lete hain? ::: r ek distance hai isliye r≥0; aur a(1−ecosE)>0 ek valid ellipse ke liye, isliye negative root physically meaningless hai.
Origin ko focus par shift kyun karna chahiye, aur kitna? ::: νfocus par measure hota hai; center se aapko E milta. Focal distance c=ae se shift karo.
Half-angle tan formula prefer kyun karte hain, aur invert karne mein kya catch hai? ::: tan(θ/2) ek poore orbit mein monotone hai — koi quadrant ambiguity nahi, unlike arccos. Catch: tan(E/2) ka E=π par pole hai, isliye alag numerator/denominator par atan2 se invert karo, raw arctan se nahi.
Stretch factor kya hai aur uski e=0 value kya hai? ::: (1+e)/(1−e); e=0 par 1 ke barabar hota hai isliye ν=E.
Square root ka + branch kyun? ::: Stretch factor positive hai, isliye tan(ν/2) aur tan(E/2) same sign share karte hain — ν aur E orbit ke same half mein hain.
Dekho bhi: Position and velocity in the perifocal frame · Orbital radius equation · Kepler's Equation.