EASY
JEE Main/Advance
IMPORTANT
Earn 100

The compressional force required to prevent a metallic rod of cross-sectional area A from expanding, when it is heated to increase its temperature by t°C, is (modulus of elasticity is E and coefficient of linear expansion is α)

100% studentsanswered this correctly

Important Questions on Thermal Properties of Matter

EASY
JEE Main/Advance
IMPORTANT

Two metallic rods of equal length and cross-section but thermal conductivities K1 and K2 are welded as shown

Question Image

The equivalent thermal conductivity of this resulting rod will be

MEDIUM
JEE Main/Advance
IMPORTANT
In a steady state, the temperatures at the end A and B of 20 cm long rod AB are 100 °C and 0 °C. The temperature of a point 9 cm from A is,
MEDIUM
JEE Main/Advance
IMPORTANT
A uniform metal ring with centre C has two points A and B maintained at two different constant temperatures. The angle ACB is θ. If it is known that for θ=180°, rate of heat flow from A to B is 1.2 W, the rate of heat flow for θ=90° will be
HARD
JEE Main/Advance
IMPORTANT
A metallic sphere having inner radius a and outer radius b has thermal conductivity k=k0r2 (arb). The thermal resistance between inner and outer surface for radial heat flow is
MEDIUM
JEE Main/Advance
IMPORTANT
A hot body cools from 85°C to 75°C T in time T1, from 75°C to 65°C in time T2 and from 65°C to 55°C in time T3, then (temperature of surrounding =30°C)
MEDIUM
JEE Main/Advance
IMPORTANT
The temperature and the surface area of a body are 227°C and 0.15 m2 respectively. If its transmitting power is negligible and reflecting power is 0.5, the thermal power of the body is
EASY
JEE Main/Advance
IMPORTANT
A body cools by Newton's law of cooling. The surrounding temperature is 25°C. The temperature of the body falls from 60°C to 50°C in 10 min. The temperature at the end of next 10 min is
MEDIUM
JEE Main/Advance
IMPORTANT

Assuming the sun to be a spherical body of radius R at a temperature of T K, evaluate the total radiant power, incident on the earth, at a distance r from the sun:

(radius of earth is r0)