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Geometrical Optics (Refraction)
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Q. If plane side of a plano convex lens is silvered what is the effective focal lenght . If curved side is sivered then what is effective focal lenght Please tell me the formula and answer in both these cases?
A plano-convex lens when silvered in the plane side behaves like a concave mirror of focal length 30cm. However, when silvered on the convex side it behaves like a concave mirror of focal length 10 cm.
Q. A fixed cylindrical tank of height H=4m and radius R=3m is filled up with a liquid. An observer through a telescope fitted at the top of the wall of the tank and inclined at angle theta= 45 degree with the vertical. When the tank is completely filled with liquid, he notices an insect , which is the center of the bottom of the tank. At t=0 , he opens a cork of radius r=3cm at the bottom of tank. The insect moves in such a way that it is visible for a certain time. Determine (a) the refractive index of the liquid (b) the velocity of insect as a function of time. How did the value of x is determined?
Applying the Bernoulli's equation for the given setup: P 0+ 2 1×2×ρv 2 =P 0+2ρg+ 2 h+ρgh So, velocity of efflux comes out to be v= 2ghNow, for the distance covered in vertical direction: 2 1gt 2 = 2 hSo, t= g hSo, the ranfe of the efflux will be: R=v×t R= 2h
Q. What will be formula for calculations of apparent depth when refractive index of material and real depth is given in question and what will be conditions for it?
Refractive Index = real depth/apparent depth
When a ray of light moves from one medium to another there is a change in velocity and direction of ray due to refraction which results in false appearance of depth of the material. The actual depth that a transparent medium has is known as real depth. Note − Real depth is always greater than apparent depth.
Q. A telescope has objective lens of focal length 15m and eyepiece of focal length 1cm. If it is used to view the moon , what is the diameter of the image of moon formed by objective lens? Diameter of moon is 3.48 ×10^6 and radius of lunar orbit is 3.8 ×10^8?
a) | em / m | = | f₀ / fe |
f₀ = Focal length of objective
fe = Focal length of eyepiece
| m | = 15 × 100 / 1 = 1500
∵ image formed is inverted
∵ Angular magnification = + 1500
(b) Angle subtended by moon at object = angle of image at objective
D/R = d/f₀
3.4 × 10⁶ / 3.8 × 10⁸ = d/15
d = 3.4/3.8 × 10⁻² × 15 m
d = 13.4 cm