1
IIT-JEE 2010 Paper 1 Offline
Numerical
+3
-0
A 0.1 kg mass is suspended from a wire of negligible mass. The length of the wire is 1 m and its crosssectional area is 4.9 $$ \times $$ 10-7 m2. If the mass is pulled a little in the vertically downward direction and released, it performs simple harmonic motion of angular frequency 140 rad s−1. If the Young’s modulus of the material of the wire is n $$ \times $$ 109 Nm-2, the value of n is
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2
IIT-JEE 2010 Paper 1 Offline
MCQ (Single Correct Answer)
+3
-0.75

A block of mass m is on an inclined plane of angle θ. The coefficient of friction between the block and the plane is μ and tan θ > μ. The block is held stationary by applying a force P parallel to the plane. The direction of force pointing up the plane is taken to be positive. As P is varied from P1 = mg(sinθ − μ cosθ) to P2 = mg(sinθ + μ cosθ), the frictional force f versus P graph will look like

IIT-JEE 2010 Paper 1 Offline Physics - Laws of Motion Question 24 English
A
IIT-JEE 2010 Paper 1 Offline Physics - Laws of Motion Question 24 English Option 1
B
IIT-JEE 2010 Paper 1 Offline Physics - Laws of Motion Question 24 English Option 2
C
IIT-JEE 2010 Paper 1 Offline Physics - Laws of Motion Question 24 English Option 3
D
IIT-JEE 2010 Paper 1 Offline Physics - Laws of Motion Question 24 English Option 4
3
IIT-JEE 2010 Paper 1 Offline
MCQ (More than One Correct Answer)
+3
-0.75
A point mass of 1 kg collides elastically with a stationary point mass of 5 kg. After their collision, the 1 kg mass reverses its direction and moves with a speed of 2 ms−1. Which of the following statement(s) is (are) correct for the system of these two masses?
A
Total momentum of the system is 3 kg ms−1
B
Momentum of 5 kg mass after collision is 4 kg ms−1
C
Kinetic energy of the centre of mass is 0.75 J
D
Total kinetic energy of the system is 4 J
4
IIT-JEE 2010 Paper 1 Offline
Numerical
+3
-0
A binary star consists of two stars A (mass 2.2Ms) and B (mass 11Ms), where Ms is the mass of the sun. They are separated by distance d and are rotating about their centre of mass, which is stationary. The ratio of the total angular momentum of the binary star to the angular momentum of star B about the centre of mass is
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