Gravitation Exercise Class 10
Q.1. Study the entries in the following table and rewrite them putting the connected items in a single row.I | II | III |
---|---|---|
Mass | m/s2 | Zero at the center of the earth |
Weight | kg | Measure of inertia |
Acceleration due to gravity |
N.m2/kg2 | Same in the entire universe |
Gravitational constant |
N | Depends on height |
I | II | III |
---|---|---|
Mass | kg | Measure of inertia |
Weight | N | Depends on height |
Acceleration due to gravity |
m/s2 | Zero at the center of the earth |
Gravitational constant |
N.m2/kg2 | Same in the entire universe |
Answer:
We have, v = u + at …..(1)
and s = ut +
∴ s = (v – at) t +
= vt – at2 +
∴ s = vt –
As the stone moves upward from A → B,
s = AB = h, t = t1,
a = -g (retardation),
u = u and v = 0
∴ From Eq. (3), h = 0 –
∴ h =
As the stone moves downward from B → A,
t = t2, u = 0, s = h and a = g
∴ from Eq. (2), h =
From Eqs. (4) and (5), t12 = t22
∴ t1 = t2 (∵ t1 and t2 are positive)
(e) If the value of g suddenly becomes twice its value, it will become two times more difficult to pull a heavy object along the floor. Why?
Answer:
To pull an object along the floor, it is necessary to do work against the force of friction between the object and the surface of the floor. This force of friction is proportional to the weight, mg, of the object. If the value of g becomes twice its value, the weight of the object and hence the force of friction will become double. Therefore, it will become two times more difficult to pull a heavy object along the floor.
Q.3. Explain why the value of G is zero at the center of the Earth.
The value of g changes while going deep inside the earth. It goes on decreasing as we go from the earth’s surface towards the earth’s center.
We shall treat the earth as a sphere of uniform density. If we consider a particle of mass m at point P at a distance (R – d) from the earth’s center, where R is the radius of the earth and d is the depth below the earth’s surface, the gravitational force on the particle due to the earth is
F = where ‘M’ is the mass of the sphere of radius (R – d).
because the outer spherical shell is not effective (Fig. 1.10). In this case, the acceleration due to gravity is
where M is the mass of the earth. Thus, g decreases as d increases. It is less than that at the earth’s surface (
∴ g = 0.
[Note: The formulae given in the answer are not given in the textbook. The formula density
=
Q.4. Let the period of revolution of a planet at a distance R from a star be T. Prove that if it was at a distance of 2R from the star, its period of revolution will be.
Answer:
T=?, where T = period of revolution of a planet around the Sun, M = mass of the Sun, G = gravitational constant, r = radius of the orbit assumed to be circular = distance of the planet from the Sun.
For r = R, T =T1.
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