(i) What is a continuous emission spectrum? Name one source of light which produces such a spectrum.
(ii) Explain in brief why dark lines are observed in the solar spectrum.
For the convex lens L1, we have
F = + 15 cm ; u = - 20 cm ; v = ?
Using the lens formula, we have.
1/v - 1/u = 1/f
1/v = 1/f + 1/u
= 1/15 + 1/-20
= 1/15 - 1/20
= 1/60
V = + 60 cm
This means that L1 I’ = 60 cm.
The image I’ formed by the convex lens L1, will serve as an object for the concave lens L2
Referring to Fig above we find that after refraction at L2 rays become parallel to principal axis. Therefore I’ is the focus of lens L2.
Focal length of L2 = L2 I’
= L1 I’ — L1L2
= 60 - 35
= 25 cm.
(i) What are coherent sources?
(ii) In young’s double slit experiment, what is the path differences between the two light waves forming 5th bright band (fringe) on the screen?
(i) In case of polarized light, what is means by the plane of polarization?
(ii) Find refractive index of glass if its polarising angle is 60°.
(i)Explain the statement: “Angular magnification of a compound microscope in normal use is 30”.
(ii) State how the resolving power of an astronomical telescope can be increased.
In Millikan’s oil drop experiment, the two plates are 2 cm apart. When a potential differences of 2355 V is applied between them, an oil drop of radius 1μm is found to remain suspended. Calculate the number of excess electrons on the drop,
[Density of oil = 900 kg/m 3 = Density of air may be ignored]