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IIT-JEE 2010 - Career Point

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2. Show that the temperature of a planet varies inversely<br />

as the square root of its distance from the Sun.<br />

Sol. Let R s be the radius of the Sun. Consider the Sun as a<br />

black body.<br />

Energy emitted per sec by it equals 4 π R σ T<br />

4<br />

This energy falls uniformly on the inner surface of<br />

spheres centred on the Sun. If d is the distance of the<br />

planet from the Sun, then energy falling on unit area<br />

of the sphere of radius d is :<br />

2 4<br />

sσTs<br />

2<br />

4πR<br />

σR sTs<br />

=<br />

2<br />

4πd<br />

d<br />

This energy received by the planet is given by<br />

2<br />

4<br />

2<br />

Q = πr 2 σR sTs<br />

= where r is the radius of planet.<br />

2<br />

d<br />

If T is the temperature of the planet, then energy lost<br />

by it per sec is 4 π r 2 σ T 4<br />

In the steady state the rate of reception of energy is<br />

equal to the loss of energy<br />

Hence, 4 π r 2 σ T 4 πr σR<br />

=<br />

2<br />

d<br />

1<br />

Thus, T ∝<br />

d<br />

4<br />

2<br />

2 4<br />

s Ts<br />

3. A sphere of specific gravity s just fits into a vertical<br />

cylinder with lower end closed. The sphere is allowed<br />

to drop slowly until it is held in equilibrium by the<br />

thrust of the compressed air. There is no leakage of<br />

air. If the diameter of the sphere is d, the length of<br />

the cylinder is L and the height of the water<br />

barometer is h, then what will be the position of<br />

sphere ?<br />

Sol. Initially, the cylinder contained air at atmospheric<br />

pressure. When the sphere comes down into the<br />

cylinder by the action of its own weight, it presses the<br />

air downwards. Suppose the sphere comes to position<br />

C which is at height x above the closed end. Let the<br />

sphere remain in equilibrium in this position.<br />

Volume of sphere = (4/3)πr 3<br />

Weight of the sphere = (4/3)πr 3 sg<br />

Volume of cylinder = πr 2 L<br />

Volume of air inside the cylinder when the sphere is<br />

in position A = πr 2 L – (2/3)πr 3<br />

2<br />

s<br />

s<br />

Volume of compressed air when the sphere is in<br />

position C = [πr 2 x – (2/3)πr 3 ]<br />

Atmospheric pressure = h cm of water<br />

Let the pressure of compressed air be p cm of water.<br />

L<br />

d<br />

According to Boyle's Law (assuming no change in<br />

the temperature of compressed air)<br />

p[πr 2 x – (2/3)πr 3 ] = h[πr 2 L – (2/3)πr 3 ]<br />

or p[x – (2r/3) = h[L – (2r/3)] ...(1)<br />

In the equilibrium position C, the weight of the<br />

sphere is balanced by the difference of vertical thrust<br />

on either side due to atmospheric and compressed air.<br />

Hence, πr 2 (p – h)g = mg = (4/3)πr 3 sg<br />

or p – h = (4/3)rs ...(2)<br />

From equation (1) and (2), we get<br />

h(3L<br />

− 2r)<br />

x =<br />

+<br />

3p<br />

h(3L − 2r)<br />

or x =<br />

+<br />

3h + 4rs<br />

or x =<br />

2<br />

9hL + 2d s<br />

9h + 6ds<br />

2r<br />

3<br />

A<br />

C<br />

x<br />

2 r 9hL + 8r s<br />

=<br />

3 3(3h + 4rs)<br />

4. Given the position of the object O and the image I as<br />

shown in the figure. Find (a) the position of the<br />

convex lens (b) its focal length and the magnification<br />

of the image. Verify graphically.<br />

2<br />

1<br />

0<br />

–1<br />

–2<br />

Y<br />

O<br />

1 2 3 4 5 6 7 8 9 10 11 12 13 14<br />

Sol. A ray of light from the object passes undeviated<br />

through the optic centre of the lens (C) and also the<br />

image I. So join OI.<br />

So it cuts the principal axis XY and C. So AB is the<br />

position of the lens. A ray parallel to the principal<br />

axis from the object after refraction meets the<br />

principal axis at F. F is the focus.<br />

2<br />

I<br />

X<br />

XtraEdge for <strong>IIT</strong>-<strong>JEE</strong> 23 DECEMBER 2009

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