Optics 6 Question 8

9. A planet is observed by an astronomical refracting telescope having an objective of focal length 16m and an eyepiece of focal length 2cm

(1992, 2M)

(a) the distance between the objective and the eyepiece is 16.02m

(b) the angular magnification of the planet is -800

(c) the image of the planet is inverted

(d) the objective is larger than the eyepiece

Fill in the Blank

Show Answer

Solution:

  1. Key Idea In a YDSE, path difference between 2 rays, reaching at some common point P located at angular position ’ θ ’s shown in the figure below is

ΔL=dsinθ

For small value of θ;sinθθ

So, path difference =ΔL=dθ

For a bright fringe at same angular position ’ θ ‘, both of the rays from slits S1 and S2 are in phase.

Hence, path difference is an integral multiple of wavelength of light used.

 i.e., ΔL=nλ or dθ=nλλ=dθn

Here, θ=140rad,d=0.1mm Hence, λ=0.140nmm=0.1×103m40n

=0.1×103×10940nnmλ=2500nnm

So, with light of wavelength λ1 we have

λ1=2500n1(nm)

and with light of wavelength λ2, we have

λ2=2500n2(nm)

Now, choosing different integral values for n1 and n2, (i.e., n1,n2=1,2,3 etc) we find that for

n1=4,λ1=25004=625nm

and for n2=5,

λ2=25005=500nm

These values lie in given interval 500nm to 625nm.



जेईई के लिए मॉक टेस्ट

एनसीईआरटी अध्याय वीडियो समाधान

दोहरा फलक