2.5.7 · D1 · Physics › Optics › Power of a lens, combination of lenses
Ek lens light rays ko modta hai , aur poora topic ek single number tak reduce ho jaata hai — power — jo batata hai ki yeh kitni zor se modta hai. Jab ek baar aap woh ek number padhna seekh lo, lenses ko stack karna seedhi addition ban jaati hai, scary fraction arithmetic nahi.
Is page par assume kiya gaya hai ki aapne parent note ki notation mein se kuch bhi nahi dekha. Hum har letter, har ratio, har sign ek picture se build karte hain, ek aisi order mein jahan har idea sirf pichle waale par lean karta hai. Jab aap finish karo, Power of a lens, combination of lenses dobara padho aur woh obvious lagni chahiye.
Kisi bhi symbol se pehle, woh scene dekho jisme sab kuch rehta hai.
Definition Principal axis
Principal axis woh seedhi horizontal line hai jo lens ke exact centre se hoke guzarti hai, uske perpendicular. Yeh hamari "ground line" hai — har distance aur height isi se measure hoti hai.
Picture: upar lens ke beech mein se left-to-right jaati dashed gray line.
Isko kyun chahiye: bina ek reference line ke hum yeh nahi keh sakte ki ek ray "kitni uchi" hai ya ek point "kitni door" hai. Yeh hamare poore coordinate world ka origin hai.
Ek ray ek patli seedhi arrow hai jo light ke travel karne ka path dikhati hai. Light left se aati hai, lens se takrati hai, aur jaise hi pass hoti hai bend ho jaati hai (direction change karti hai).
Picture: left se enter karti blue arrow, axis ki taraf bend hoti orange arrow.
Isko kyun chahiye: "rays ko modnaa" literally ek lens ka kaam hai, isliye ray woh cheez hai jise hum track karte hain.
h — ray height
h yeh hai ki ek ray lens se principal axis ke kitna upar takraati hai, seedha upar measure kiya gaya.
Picture: neeche diye figure mein green vertical segment, axis se le kar jahan ray lens se milti hai wahan tak.
Isko kyun chahiye: ek lens ray ko zyada modta hai jitni door woh hit karti hai. Toh bending h par depend karegi, aur hume woh height name karni hogi.
Definition Focus aur focal length
f
Ek ray axis ke parallel bhejon. Lens ke usse modne ke baad, woh axis ko ek special point par cross karti hai jise focus F kehte hain (woh point). Lens se us point tak ki distance focal length f hai (ek length).
Picture: upar waale figure mein, orange bent ray red dot F par axis se milti hai; f label wala red horizontal bracket uski distance hai.
Isko kyun chahiye: f woh single number hai jo batata hai ki ek lens kaise focus karta hai. Chota f matlab ray quickly axis ki taraf khinch jaati hai (strong lens); lamba f matlab woh dheere dheere neeche drift karti hai (weak lens).
f chota vs lamba
f ko sochो "light ko ek point par gather hone ke liye kitna door travel karna hai." Impatient lens = chota f = strong. Aaram-pasand lens = lamba f = weak. Yeh feeling pakad ke rakho; Section 6 mein yeh power ban jaata hai.
δ — deviation angle
δ (Greek letter delta ) woh angle hai jitna lens ray ko turn karta hai — incoming direction aur outgoing direction ke beech ka angle.
Picture: neeche waale figure mein, flat blue "seedha jaata" line aur orange "actually-bent" line ke beech shaded wedge.
Isko kyun chahiye: "lens kitni zor se modta hai" exactly yahi angle hai. Yeh woh physical quantity hai jise power measure karegi.
Parent note likhta hai tan δ ≈ δ = h / f . Uska har piece yahan earn kiya gaya hai.
Figure s03 dekho. Bent ray, axis, aur vertical height h ek right triangle banate hain:
opposite side (angle δ ke opposite) height h hai,
adjacent side (δ ke paas, axis ke saath) length f hai,
right angle wahan baithta hai jahan h axis se milti hai.
tan — "opposite over adjacent"
Kisi bhi right triangle ke liye, tan ( angle ) = adjacent side opposite side .
Picture: s03 mein, tan δ = f h — green height ko red base se divide kiya.
YEH tool kyun, koi aur kyun nahi? Hum ek angle (δ ) ko do lengths (h aur f ) se connect karna chahte hain. Saare trig ratios mein, tan exactly woh hai jo opposite over adjacent se bana hai — aur wahi do sides hain jo haara triangle hamare haath deta hai. Sine ya cosine ko slanted hypotenuse chahiye hoga, jis ki hume parwah nahi.
Recall Small-angle ka matlab
tan δ ≈ δ kyun hota hai?
Ek tiny wedge ke liye, seedha opposite side aur curved arc almost coincide karte hain, isliye opposite/adjacent (=tan ) aur arc/adjacent (=radian angle) almost equal hote hain. ::: Woh small angles ke liye first order tak agree karte hain.
Parent mein lensmaker's relation R 1 aur R 2 use karta hai. Yeh hain woh actually .
R — radius of curvature
Ek lens surface ek sphere ka ek slice hai. Uska radius of curvature R us sphere ka radius hai. Flatter surface ⇒ bada R ; zyada sharply curved ⇒ chota R .
Picture: imagine karo ki lens face ke peeche ek balloon phula rahe ho; R yeh hai ki woh balloon kitna bada hai.
R 1 un pehli surface ke liye hai jise light milti hai, R 2 doosri ke liye. Subscripts 1 , 2 sirf "pehla" aur "doosra" mean karte hain.
Isko kyun chahiye: parent ka formula P = ( n − 1 ) ( R 1 1 − R 2 1 ) kehta hai curvature power banata hai. Teekhay curves (R chota) ⇒ bada R 1 ⇒ strong bending.
n — refractive index
n ek number hai jo batata hai ki glass light ko air ke comparison mein kitna slow aur bend karta hai . Ordinary glass ka n ≈ 1.5 hota hai.
( n − 1 ) kyun? Agar glass air ke identical hota (n = 1 ), toh woh light ko bilkul nahi modta — power zero hoti. ( n − 1 ) "air se kitna alag hai" measure karta hai, isliye yeh curvature se zaroor multiply hona chahiye.
Ab upar sab kuch ek number mein collapse ho jaata hai.
P — lens ki power
Power unit height per bending strength hai, aur yeh focal length ke reciprocal ke barabar hai:
P = f 1 ( f metres mein )
Section 4 se: unit height per bending = h δ = f 1 . Woh ratio hi P hai.
Reciprocal kyun? Chota f (strong lens) bada P dena chahiye. f se divide karne par scale exactly sahi tarah flip ho jaata hai.
Unit: dioptre (D ), jahan 1 D = 1 m − 1 . Isliye f metres mein hona chahiye — unit defined hai per metre.
f ko centimetres mein padhna
f = 20 cm ka matlab P = 1/20 nahi hai. Pehle convert karo: 20 cm = 0.2 m , toh P = 1/0.2 = 5 D .
Behaviour ka har quadrant cover hona chahiye — yahan "cases" do lens shapes aur unke signs hain.
Definition Lenses ke liye sign convention
Lens
Shape
Parallel rays ke saath kya karta hai
f
P
Convex (converging)
fat middle
unhe saath ek real focus par kheenchta hai
f > 0
P > 0
Concave (diverging)
thin middle
unhe alag failata hai (woh ek focus se peeche se aate lagte hain)
f < 0
P < 0
Picture: convex = ")(" ulta, arrow-heads milte hue; concave = "()", arrows bahar fan karti huin.
Minus kyun matter karta hai: ek negative power ek positive ko cancel kar sakti hai. Jab hum combination ki powers add karte hain, sign woh cheez hai jo ek concave lens ko convex lens ka part undo karne deti hai. Sign drop karo aur physics toot jaati hai.
Parent mein combination derivation u , v , v 1 , aur F use karta hai. Sab ko name karo.
u , v , aur thin-lens equation
u = lens se object tak distance (woh cheez jo aap dekh rahe ho).
v = lens se image tak distance (jahan lens light ko ek point par bheajta hai).
Yeh thin-lens equation v 1 − u 1 = f 1 maante hain, jo Thin Lens Equation mein poori tarah banai gayi hai.
Isko kyun chahiye: "powers add hoti hain" ka proof ek object ko u par leta hai, image ko v 1 par lenses ke beech track karta hai, phir final image ko v par. Woh teen naam bookkeeping hain.
v 1 aur capital F
v 1 = sirf lens 1 dwara banaya gaya image; yeh lens 2 ke liye object ban jaata hai. Subscript 1 = "lens 1 ka hai."
Capital F = poore stack ki combined focal length (focus point F ya ek lens ke f se confuse mat karo). Iska power P = 1/ F hai.
Principal axis - reference line
tan delta approx delta equals h over f
P equals 1 over f - the core number
Lensmaker P equals n minus 1 times curvature
Convex positive - Concave negative
Combination 1 over F equals sum
Power and Combination of Lenses
Parent note mein jaane se pehle har ek ka jawab do; agar koi atka le, woh section dobara padho.
Principal axis kya hai, aur isko kyun chahiye? Lens ke through centre line; yeh woh reference hai jisse saari heights aur distances measure hoti hain.
h kya represent karta hai?Axis ke upar woh height jahan ek ray lens se takraati hai.
f kya hai, aur physically chota f ka kya matlab hai?Lens-to-focus distance; chota f = rays quickly gather hoti hain = strong lens.
Deviation angle δ kya hai? Woh angle jitna lens ek ray ko uski original direction se turn karta hai.
tan kyun aata hai, sine ya cosine kyun nahi?Haara triangle opposite side (h ) aur adjacent side (f ) deta hai; tan exactly opposite/adjacent hai.
tan δ ≈ δ kyun allowed hai?Chote (paraxial) angles ke liye tangent aur radian angle almost coincide karte hain.
R 1 aur R 2 kya hain?Pehli aur doosri lens surfaces ki radii of curvature; chota R = teekhaa curve.
Lensmaker relation mein factor ( n − 1 ) kyun? Agar glass air se match karta (n = 1 ) toh koi bending nahi hoti; ( n − 1 ) measure karta hai ki glass air se kitna alag hai.
Power P aur uska unit define karo. P = 1/ f jahan f metres mein; unit dioptre hai, 1 D = 1 m − 1 .
Convex aur concave lenses ke liye P ke signs? Convex P > 0 (converging), concave P < 0 (diverging).
Lowercase f aur capital F mein kya fark hai? f = ek lens; F = poore stack ki combined focal length.
Power of a lens, combination of lenses — woh parent jiske liye yeh page taiyaar karta hai.
Thin Lens Equation — jahan u , v , aur 1/ v − 1/ u = 1/ f aate hain.
Lensmaker's Equation — yahan built n , R 1 , R 2 use karta hai.
Magnification of Lenses — distances ke baad agla quantity.
Defects of Vision — dioptres mein spectacle powers.