NCERT Exemplar solutions for Physics [English] Class 11 chapter 8 - Gravitation [Latest edition]

The earth is an approximate sphere. If the interior contained matter which is not of the same density everywhere, then on the surface of the earth, the acceleration due to gravity ______.

As observed from earth, the sun appears to move in an approximate circular orbit. For the motion of another planet like mercury as observed from earth, this would ______.

Different points in earth are at slightly different distances from the sun and hence experience different forces due to gravitation. For a rigid body, we know that if various forces act at various points in it, the resultant motion is as if a net force acts on the c.m. (centre of mass) causing translation and a net torque at the c.m. causing rotation around an axis through the c.m. For the earth-sun system (approximating the earth as a uniform density sphere).

Satellites orbiting the earth have finite life and sometimes debris of satellites fall to the earth. This is because ______.

Both earth and moon are subject to the gravitational force of the sun. As observed from the sun, the orbit of the moon ______.

In our solar system, the inter-planetary region has chunks of matter (much smaller in size compared to planets) called asteroids. They ______.

Choose the wrong option.

Particles of masses 2M, m and M are respectively at points A, B and C with AB = ½ (BC). m is much-much smaller than M and at time t = 0, they are all at rest (Figure). At subsequent times before any collision takes place ______.

Which of the following options are correct?

1. Acceleration due to gravity decreases with increasing altitude.
2. Acceleration due to gravity increases with increasing depth (assume the earth to be a sphere of uniform density).
3. Acceleration due to gravity increases with increasing latitude.
4. Acceleration due to gravity is independent of the mass of the earth.

If the law of gravitation, instead of being inverse-square law, becomes an inverse-cube law- ______.

1. planets will not have elliptic orbits.
2. circular orbits of planets is not possible.
3. projectile motion of a stone thrown by hand on the surface of the earth will be approximately parabolic.
4. there will be no gravitational force inside a spherical shell of uniform density.

If the mass of sun were ten times smaller and gravitational constant G were ten times larger in magnitudes ______.

1. walking on ground would became more difficult.
2. the acceleration due to gravity on earth will not change.
3. raindrops will fall much faster.
4. airplanes will have to travel much faster.

If the sun and the planets carried huge amounts of opposite charges ______.

1. all three of Kepler’s laws would still be valid.
2. only the third law will be valid.
3. the second law will not change.
4. the first law will still be valid.

There have been suggestions that the value of the gravitational constant G becomes smaller when considered over very large time period (in billions of years) in the future. If that happens, for our earth ______.

1. nothing will change.
2. we will become hotter after billions of years.
3. we will be going around but not strictly in closed orbits.
4. after sufficiently long time we will leave the solar system.

Supposing Newton’s law of gravitation for gravitation forces F₁ and F₂ between two masses m₁ and m₂ at positions r₁ and r₂ read F₁ = – F₂ = `- r_12/r_12^3 GM_0^2 ((m_1m_2)/M_0^2)^n` where M₀ is a constant of dimension of mass r₁₂ = r₁ – r₂ and n is a number. in such a case.

1. the acceleration due to gravity on earth will be different for different objects.
2. none of the three laws of Kepler will be valid.
3. only the third law will become invalid.
4. for n negative, an object lighter than water will sink in water.

Which of the following are true?

1. A polar satellite goes around the earth’s pole in north- south direction.
2. A geostationary satellite goes around the earth in east-west direction.
3. A geostationary satellite goes around the earth in west-east direction.
4. A polar satellite goes around the earth in east-west direction.

The centre of mass of an extended body on the surface of the earth and its centre of gravity ______.

1. are always at the same point for any size of the body.
2. are always at the same point only for spherical bodies.
3. can never be at the same point.
4. is close to each other for objects, say of sizes less than 100 m.
5. both can change if the object is taken deep inside the earth.

Molecules in air in the atmosphere are attracted by gravitational force of the earth. Explain why all of them do not fall into the earth just like an apple falling from a tree.

Give one example each of central force and non-central force.

Draw areal velocity versus time graph for mars.

What is the direction of areal velocity of the earth around the sun?

How is the gravitational force between two point masses affected when they are dipped in water keeping the separation between them the same?

Is it possibe for a body to have inertia but no weight?

We can shield a charge from electric fields by putting it inside a hollow conductor. Can we shield a body from the gravitational influence of nearby matter by putting it inside a hollow sphere or by some other means?

An astronaut inside a small spaceship orbiting around the earth cannot detect gravity. If the space station orbiting around the earth has a large size, can he hope to detect gravity?

The gravitational force between a hollow spherical shell (of radius R and uniform density) and a point mass is F. Show the nature of F vs r graph where r is the distance of the point from the centre of the hollow spherical shell of uniform density.

Out of aphelion and perihelion, where is the speed of the earth more and why?

What is the angle between the equatorial plane and the orbital plane of polar satellite?

What is the angle between the equatorial plane and the orbital plane of geostationary satellite?

Mean solar day is the time interval between two successive noon when sun passes through zenith point (meridian). Sidereal day is the time interval between two successive transit of a distant star through the zenith point (meridian). By drawing appropriate diagram showing earth’s spin and orbital motion, show that mean solar day is four minutes longer than the sidereal day. In other words, distant stars would rise 4 minutes early every successive day.

Two identical heavy spheres are separated by a distance 10 times their radius. Will an object placed at the mid point of the line joining their centres be in stable equilibrium or unstable equilibrium? Give reason for your answer.

Show the nature of the following graph for a satellite orbiting the earth. 

1. KE vs orbital radius R
2. PE vs orbital radius R
3. TE vs orbital radius R.

Shown are several curves (Figure). Explain with reason, which ones amongst them can be possible trajectories traced by a projectile (neglect air friction).

An object of mass m is raised from the surface of the earth to a height equal to the radius of the earth, that is, taken from a distance R to 2R from the centre of the earth. What is the gain in its potential energy?

A mass m is placed at P a distance h along the normal through the centre O of a thin circular ring of mass M and radius r (Figure).

If the mass is removed further away such that OP becomes 2h, by what factor the force of gravitation will decrease, if h=r?

A star like the sun has several bodies moving around it at different distances. Consider that all of them are moving in circular orbits. Let r be the distance of the body from the centre of the star and let its linear velocity be v, angular velocity ω, kinetic energy K, gravitational potential energy U, total energy E and angular momentum l. As the radius r of the orbit increases, determine which of the above quantities increase and which ones decrease.

Six point masses of mass m each are at the vertices of a regular hexagon of side l. Calculate the force on any of the masses.

A satellite is to be placed in equatorial geostationary orbit around earth for communication.

1. Calculate height of such a satellite.
2. Find out the minimum number of satellites that are needed to cover entire earth so that at least one satellites is visible from any point on the equator.

[M = 6 × 10²⁴ kg, R = 6400 km, T = 24 h, G = 6.67 × 10^–11 SI units]

Earth’s orbit is an ellipse with eccentricity 0.0167. Thus, earth’s distance from the sun and speed as it moves around the sun varies from day to day. This means that the length of the solar day is not constant through the year. Assume that earth’s spin axis is normal to its orbital plane and find out the length of the shortest and the longest day. A day should be taken from noon to noon. Does this explain variation of length of the day during the year?

A satellite is in an elliptic orbit around the earth with aphelion of 6R and perihelion of 2 R where R= 6400 km is the radius of the earth. Find eccentricity of the orbit. Find the velocity of the satellite at apogee and perigee. What should be done if this satellite has to be transferred to a circular orbit of radius 6R ?

[G = 6.67 × 10^–11 SI units and M = 6 × 10²⁴ kg]