3.2.35 · D1 · Physics › Orbital Mechanics & Astrodynamics › Solar radiation pressure
Sunlight ek aisi nadi hai jo choti-choti momentum-carrying bullets — jise photons kehte hain — se bhari hai, aur bhale hi har ek photon unbelievably chhota ho, Sun itni badi tadaad mein fire karta hai ki woh milkar kisi bhi space object ko ek steady, halki si push dene lagte hain. Us push ko predict karne ke liye hume bas yeh karna hai: count karo kitni light-energy har second ek surface par girti hai, us energy ko momentum mein badlo, aur dekho ki light chipki ya uchhal gayi.
Is page par kuch bhi assume nahi kiya gaya . Isse pehle ki tum Solar radiation pressure padho — sorry, isse pehle ki tum parent topic Solar radiation pressure padho — usmein jo bhi letter, ratio, aur Greek symbol aata hai, woh sab yahan neeche se upar tak build kiya gaya hai. Top se bottom padho; har ek brick usse pehle waali par tikhi hai.
Definition Energy — symbol
E , aur joule
Energy woh "capacity" hai jo kisi cheez mein change laaye — use heat kare, hilaye, ya roshan kare. Hum ise letter E se represent karte hain, aur iska unit joule (J ) hai. Ek joule roughly utni energy hai jitni ek chhote seb ko ek metre uthane mein lagti hai. Is topic mein energy light ke roop mein aati hai, aur yahi E woh letter hai jo Section 3 ke photon rule mein dobara aata hai — toh ise abhi hi samjho.
Definition Power, aur watt
Power energy per second hai — yani energy kitni tezi se deliver hoti hai. Iska unit watt (W ) hai, aur 1 W = 1 J/s . Ek 60 W bulb har second 60 joules bahar phenkhta hai.
Hume E aur power dono ki zaroorat kyun hai? Kyunki ek spacecraft ko ek akele photon ki chhoti si energy se farq nahi padta — use steady stream se matlab hai. "Per second" is poore topic mein baka hai. Force khud, jaise hum dekhenge, ek "per second" quantity hai.
Neeche ka figure dekho. Naranga bulb ek fixed power (60 W) emit karta hai. Clock ki har tick par, ek naaya identical 60-joule packet bahar nikalta hai — figure clearly batata hai ki "power = energy delivered every second." Woh per-second ki heartbeat yaad rakho: woh wahi beat hai jo baad mein intercepted light-energy ko ek steady force mein badal deti hai.
Definition Speed of light — symbol
c
c woh speed hai jis par light khali space mein travel karti hai: c ≈ 3 × 1 0 8 m/s (teen sau million metres har second). Letter c (celeritas , Latin mein "swiftness" ke liye) physics mein universal hai. Yeh isliye aata hai kyunki light ka momentum us speed se juda hai jis par woh move karti hai — light ki push ko uski speed se alag nahi kar sakte.
hota hai, ek tasveer mein
Momentum hai "kisi cheez ko rokna kitna mushkil hai jab woh chal rahi ho." Ek chalti bowling ball mein bahut momentum hota hai (rokna mushkil); ek chalte ping-pong ball mein thoda. Jab koi chalti cheez tumse takraati hai aur ruk jaati hai, woh tumhe apna momentum de deti hai — woh handover ek push hai.
Definition Momentum — symbol
p
Ek ordinary object ke liye, momentum p = m v : mass m baar velocity v . Zyada mass ya zyada speed → zyada momentum. Unit: kg⋅m/s .
Neeche ka figure dekho. Is poore topic ke liye key idea bottom row hai: jab ek bullet wall se takraati hai aur chip jaati hai , wall ko bullet ka momentum p milta hai. Jab bullet seedha wapas uchhalti hai , woh − p momentum ke saath jaati hai, toh wall ko p − ( − p ) = 2 p mila — do guna push. Woh "do guna" yaad rakho; yahi mirror-vs-black-paint ka fact hai jis par parent topic tikha hai.
Common mistake "Light mein mass nahi hai, toh
p = m v = 0 — light push nahi kar sakti."
Yeh sahi kyun lagta hai: tumne sirf p = m v formula dekha hai, aur m = 0 use khatam kar deta hai.
Fix yeh hai: p = m v sirf slow-object ka rule hai. Light ek alag rule follow karti hai (agla section) jo use bina mass ke momentum deta hai. Momentum "hamesha mass times velocity" nahi hai — yeh ek conserved book-keeping quantity hai, aur light ke paas kuch hota hai. Dekho Photon momentum and relativity .
Light ek smooth continuous stream nahi hai — yeh chhote indivisible packets mein aati hai jise photons kehte hain. Ek machine gun ki tarah socho jo har second millions light-bullets fire karti hai. Har photon ek specific amount energy E carry karta hai — wahi E (joules mein measured) jo humne Section 1 mein dekha tha.
Intuition Yeh ek formula sab kuch kyun unlock karta hai
Agar tum jaante ho ki har second kisi surface par kitni light-energy girti hai, toh tum use 1/ c se multiply karo aur turant jaano ki har second kitna momentum gir raha hai — aur momentum-per-second ek force hai. Poora topic yahi hai: energy count karo, c se divide karo, kaam khatam.
Definition Force — symbol
F
Force ek push ya pull hai. Newton ki insight: force woh momentum hai jo har second deliver hota hai . Agar koi stream har second momentum p hand over karti hai, toh woh p per second ki ek force hai . Unit: newton (N ), aur 1 N = 1 kg⋅m/s 2 .
Definition Pressure — symbol
P
Pressure force ko area par spread karna hai: P = F / A . Wahi push ek chhote patch par = high pressure; ek bade sail par = low pressure. Unit: pascal (Pa ), 1 Pa = 1 N/m 2 .
Topic pehle pressure ki baat kyun karta hai aur force ki baad mein? Kyunki sunlight per square metre aati hai — yeh naturally ek pressure hai. Apne actual spacecraft par force paane ke liye tum pressure ko uske area se multiply karte ho. Yahi logical order hai jo parent note follow karta hai.
Definition Acceleration aur mass — symbols
a aur m
Mass m hai ki kitni "cheez" push hone se resist karti hai (unit kg ). Acceleration a hai ki velocity kitni tezi se change hoti hai. Newton ka law dono ko jodhta hai: F = ma , toh a = F / m . Ek diya hua push halki cheez ko zyada hilata hai. Isliye topic force par nahi, acceleration par khatam hota hai — orbits a par react karte hain, aur ek feather-light sail ek tiny force se bhi bahut tezi se accelerate karta hai.
Definition Luminosity — symbol
L ⊙
L ⊙ woh total power hai jo Sun har direction mein radiate karta hai: L ⊙ ≈ 3.83 × 1 0 26 W . Chhota circle-with-a-dot ⊙ astronomy mein "the Sun" ka standard symbol hai.
Definition Distance — symbol
r , aur AU
r Sun ke centre se tumhari doori hai. Astronomers ise astronomical units (AU ) mein measure karte hain: 1 AU = Sun se Earth ki average doori ≈ 1.5 × 1 0 11 m .
Intuition Wahi light door jaane par kamzor kyun padti hai — sphere picture
Sun ki power sab directions mein equally stream hoti hai. Doori r par, woh sab ek imaginary sphere ki surface par phail jaati hai jiska radius r hai. Us sphere ka area 4 π r 2 hai. Doori double karo → sphere ka area chaar guna ho jaata hai → light chaar guna patli ho jaati hai. Yeh "4 π r 2 par phailna" hi famous 1/ r 2 falloff ki poori wajah hai.
Ab chain ek saath jud jaati hai: S energy-per-second-per-area hai → c se divide karo (photon rule) → momentum-per-second-per-area = pressure :
P rad = c S .
Definition Surface normal, aur angle
θ
Normal ek surface se seedha bahar nikla hua arrow hota hai, uske perpendicular — jaise ek pencil tabletop par balanced ho. Angle θ (Greek "theta") us normal arrow aur Sun ki taraf ki direction ke beech measure kiya jaata hai. Agar surface Sun ki taraf seedha face kar rahi hai, θ = 0 . Agar Sun ke saath edge-on hai, θ = 9 0 ∘ aur woh almost koi light nahi pakadti.
Definition Reflectivity — symbol
η
η (Greek "eta") 0 se 1 tak ka ek number hai jo batata hai ki ek surface light ko kitna achha wapas uchhalti hai. η = 0 matlab "perfectly black — har photon ko niga leta hai" (absorb). η = 1 matlab "perfect mirror — har photon ko wapas uchhalti hai" (reflect). Yeh factor ( 1 + η ) ke andar hota hai: black deta hai × 1 , mirror deta hai × 2 — wahi Section 2 ka recoil-doubling ek dial mein convert ho gaya.
Common mistake "Edge-on se zyada tilt hua surface phir bhi sunlight pakad leti hai."
Yeh sahi kyun lagta hai: tum koi bhi θ cos θ mein daalo aur ek number milta rehta hai.
Fix yeh hai: θ > 9 0 ∘ ke liye surface Sun se doori face kar rahi hai — uska lit side shadow mein hai, toh koi sunlight nahi girti aur force zero hai, negative nahi. Mathematically cos θ wahan negative ho jaata hai, jo push ko nonsensically flip kar deta. Toh hamesha clamp karo: max ( cos θ , 0 ) use karo. Sirf 0 ≤ θ ≤ 9 0 ∘ light receive karta hai.
Ab har symbol defined hai. Dekho yeh sab ek expression mein kaise click karte hain, ek factor ek time.
Definition Area-to-mass ratio — symbol
A / m
A sunlit cross-section area hai (woh kitna bada shadow daalta hai), m uski mass hai. Ratio A / m kehta hai "har kilogram mein kitna sail hai." Bada A / m (ek balloon, ek sail) → strong SRP effect; chhota A / m (ek dense metal probe) → barely feel karta hai — dekho Solar sails versus ek heavy orbiter, aur Orbital perturbations mein ek perturbation ke roop mein uska role.
Har node ek symbol aur uska plain meaning batata hai, toh tum diagram ko seedha upar diye definitions se map kar sako.
Power = E per second, watts
Radiation pressure Prad = S over c
Intensity S = power per area
Sphere area 4 pi r squared
Force F = Prad times A times one plus eta times cos theta
Acceleration a = F over m
Area to mass ratio A over m
Ise ek nadi ki tarah padho: energy E aur speed of light c milkar photon momentum rule banate hain; luminosity L ⊙ ek sphere 4 π r 2 par phailkar intensity S banati hai; intensity ko c se divide karo toh pressure P rad milta hai; pressure times area, bounce factor aur cos θ milkar force F banate hain; force ko mass se divide karo toh woh acceleration milta hai jo ek orbit ko mod deta hai.
Right side cover karo aur khud ko test karo. Agar koi bhi jawab surprising lage, toh parent note kholne se pehle woh section dobara padho.
Power kya hai, ek phrase mein, aur uska unit? Energy delivered per second; the watt (W = J/s ).
Energy ko kaun sa letter denote karta hai, aur uska unit? E , joules mein measured (J ).
c ki value aur meaning kya hai?The speed of light, ≈ 3 × 1 0 8 m/s .
Ordinary momentum formula aur uska unit? p = m v , in kg⋅m/s .
Light-momentum rule aur kyun yeh p = m v nahi hai? p = E / c ; p = m v sirf massive slow objects ke liye kaam karta hai, light massless hai.
Ek mirror ko black paint se do guna zyada push kyun milti hai? Ek bounced photon momentum reverse kar deta hai (p → − p ), toh change p ki jagah 2 p hota hai.
Force ko "per second" idea se kaise state karein? Force = momentum delivered per second; unit newton (N ).
Pressure ki definition aur uska unit? Force per area, P = F / A ; the pascal (Pa = N/m 2 ).
Newton ka force, mass, acceleration ke beech link? F = ma , toh a = F / m .
L ⊙ ka kya matlab hai?Woh total power jo Sun sab directions mein radiate karta hai, ≈ 3.83 × 1 0 26 W .
Light 1/ r 2 ki tarah kamzor kyun hoti hai? Fixed power 4 π r 2 area wale ek sphere par phailta hai, jo r 2 ke saath badhta hai.
Intensity S ki definition aur uski 1 AU value? Power per area, S = L ⊙ / ( 4 π r 2 ) ; 1 AU par ≈ 1361 W/m 2 .
Angle θ kis cheez ke beech measure kiya jaata hai? Surface normal aur Sun ki direction ke beech.
θ > 9 0 ∘ ke liye force ka kya hota hai?Surface doori face karti hai, koi light nahi girti — cos θ ko 0 par clamp karo, force zero hai.
η kya encode karta hai, aur η = 0 vs η = 1 ka matlab?Reflectivity; 0 = perfect absorber, 1 = perfect mirror.
Ek plate par poora simple force formula? F = ( S / c ) A ( 1 + η ) cos θ for 0 ≤ θ ≤ 9 0 ∘ .
Orbits A / m ki parwah kyun karte hain? SRP acceleration area-to-mass ke saath scale karta hai, toh light high-area craft ise strongly feel karte hain.
Solar radiation pressure — woh parent topic jise yeh foundations unlock karte hain.
Photon momentum and relativity — p = E / c kahan se aata hai.
Inverse-square law — sphere area ke zariye intensity 1/ r 2 ki tarah kyun girta hai.
Solar sails — extreme high-A / m application.
Orbital perturbations — jahan resulting acceleration matter karta hai.