Yeh page assume karta hai ke tum parent note ke symbols ke baare mein kuch nahi jaante. Hum har ek cheez ground up se build karenge, ek aisi order mein jahan har idea sirf pehle waale ideas par depend karta hai. Ant tak tum sentence "M=n(t−tp) and M=E−esinE" padh paoge aur feel karoge ke har letter apni jagah earn kar chuka hai.
Kisi bhi angle se pehle, hume us shape ki zaroorat hai jis par planet travel karta hai.
Hume iska kyun zaroorat hai: poora topic hai "planet on an ellipse", isliye a (uska size) aur b (uski squashedness) har formula mein appear karte hain.
Ek ellipse ka ek centreO hota hai (beech mein, jahan dono axes cross karte hain). Lekin iske do khaas inner points bhi hote hain jinhein foci (singular: focus) kehte hain. Planet ke liye, Sun ek focus par baitha hai, jise hum S kehte hain — centre par nahi.
e ke baare mein do facts jo parent note baar baar use karta hai:
Hume iska kyun zaroorat hai: ae wahi exact offset hai jo baad mein esinE correction term produce karta hai, aur b2=a2(1−e2) woh algebra key hai jo radius formula ko simplify karne ke liye use hoti hai.
Recall
b2=a2(1−e2) kahan se aata hai?
Yeh ellipse geometry ka defining relation hai (dono foci se distances se bana). Hum ise yahan ek diya hua tool maante hain; poori construction ke liye Eccentricity and ellipse geometry (a, b, ae, b²=a²(1−e²)) dekho.
Ek angle measure karta hai "kitna turn". Tum degrees jaante ho (ek poora circle =360°). Physics yahan radians use karta hai.
Radians kyun, degrees kyun nahi? Is topic ke har formula circles ki areas aur arcs se aaya, jahan "arc = radius × angle" rule sirf radians mein hold karta hai. Angle θ ka circular sector area 21R2θ hota hai — phir se sirf radians mein. M=E−esinE mein degrees daalo aur nonsense milega.
Radius R ke circle par ek point, rightward axis se angle θ par measured, ke coordinates hain
x=Rcosθ,y=Rsinθ.
Woh identity jis par hum lean karte hain: cos2θ+sin2θ=1 (us right triangle par Pythagoras). Yahi hai jo Derivation 2 mein messy radius algebra ko collapse karke r=a(1−ecosE) tak le aata hai.
Ab squash apply karo. Auxiliary circle (radius a) par helper point (acosE,asinE) hai. Vertically b/a se squash karo aur ellipse par planet yahan baithta hai:
x=acosE,y=bsinE.
Yahi woh jagah hai jahan eccentric anomaly E enter hone wala hai — un cosines aur sines ko feed karne wale angle ke roop mein.
Yeh sabse simple symbols hain, lekin inke bina topic ka koi matlab nahi.
Perihelion khud ek jagah hai: orbit ka Sun ke sabse nazdik point (distance a(1−e)). Iska opposite, sabse door wala point, aphelion hai (distance a(1+e)). Hum perihelion direction ko axis X label karte hain jis se saare angles count hote hain.
Hume inka kyun zaroorat hai: yeh ek time question ko agle hi step mein ek angle question mein turn kar dete hain.
Yahan hai core idea wali "steady imaginary clock".
Hume iska kyun zaroorat hai: yeh woh input hai jo hum hamesha jaante hain (hum time jaante hain), aur Kepler's equation ka poora kaam hai is honest clock reading M ko real geometry mein convert karna.
Yeh topic ka star hai, aur woh aakhri symbol jo hum build karte hain.
Hume iska kyun zaroorat hai: E bridge symbol hai. Time se M milta hai; geometry se position cosE,sinE ke zariye milti hai; Kepler's equation M=E−esinE dono ko weld karta hai.
Completeness ke liye (parent ise ek baar use karta hai): true anomalyν (Greek "nu") planet ka actual angle hai jaise Sun se focus S par dekha gaya, perihelion se measured. Yahi woh hai jis direction mein tum literally telescope point karoge. Iska E se relation hai
tan2ν=1−e1+etan2E.
Apni kahani ke liye True anomaly ν and the orbit equation r = a(1−e²)/(1+e cos ν) dekho. Abhi ke liye: M (clock) → E (centre helper) → ν (real angle) poori chain hai.
M=E−esinE mein Ebahar bhi hai (E) aur andar bhi ek sin ke. Tum ise "E= (formula in M)" mein rearrange nahi kar sakte. Is tarah ke equations ko transcendental kehte hain; inhe repeated guessing se solve karte hain jo answer par home in karta hai (dekho Numerical root-finding — Newton–Raphson).