Gravitation

# Class 10th Science And Technology Part 1 MHB Solution

### Exercise

1. Study the entries in the following table and rewrite them putting the connected items in a…

2. What is the difference between mass and weight of an object. Will the mass and weight of…

3. What are (i) free fall, (ii) acceleration due to gravity (iii) escape velocity (iv)…

4. Write the three laws given by Kepler. How did they help Newton to arrive at the inverse…

5. A stone thrown vertically upwards with initial velocity u reaches a height ‘h’ before…

6. If the value of g suddenly becomes twice its value, it will become two times more…

7. Explain why the value of g is zero at the centre of the earth.

8. Let the period of revolution of a planet at a distance R from a star be T. Prove that if…

9. An object takes 5 s to reach the ground from a height of 5 m on a planet. What is the…

10. Solve the following example. The radius of planet A is half the radius of planet B. If the…

11. The mass and weight of an object on earth are 5 kg and 49 N respectively. What will be…

12. An object thrown vertically upwards reaches a height of 500 m. What was its initial…

13. A ball falls off a table and reaches the ground in 1 s. Assuming g = 10 m/s^2 , calculate…

14. The masses of the earth and moon are 6 x 10^24 kg and 7.4x10^22 kg, respectively. The…

15. The mass of the earth is 6 x 10^24 kg. The distance between the earth and the Sun is 1.5x…

###### Exercise

# Question 1.Study the entries in the following table and rewrite them putting the connected items in a single row.

Answer:

Question 2.Answer the following question.

What is the difference between mass and weight of an object. Will the mass and weight of an object on the earth be same as their values on Mars? Why?

Answer:Following are the difference between the weight and mass of an object.

i. Since mass is the amount of the matter present in the body, and amount of matter (ex: bones, blood, skin etc) is same everywhere. Therefore the mass of the object on earth will be the same as that on the mars.

ii. whereas the weight of an object on Earth and Mars will be different as the value of accelearation due to gravity(g) is different for Earth and Mars and we know that Weight= Mass × g. Therefore, the weight of the object will be different on Mars as that on the surface of Earth

Question 3.Answer the following question.

What are (i) free fall, (ii) acceleration due to gravity (iii) escape velocity (iv) centripetal force?

Answer:(i) __Free Fall__: Whenever an object moves under the influence of the force of gravity alone, it is said to be in Free Fall. During __free fall initial velocity of an object is zero__ and force of air also acts on an object. Thus real free fall is possible only in a vacuum because there is no air.

For Example:

a) When an object is dropped from the top of the table it falls down only due to gravitational force hence it is under free fall.

b) An apple falling from the tree.

But when we are standing on the ground, flying in a flight we are not in free fall because other forces except gravitational force are also acting.

(ii) __Acceleration due to gravity__: The acceleration which is gained by an object because of the gravitational force is called acceleration due to gravity. Its S.I unit is m/s2. It is denoted by ‘g’ and its value at the surface of the earth is 9.8m/s2.

It is a vector quantity (have both magnitude and direction) and it is directed towards the centre of the earth. The value of acceleration due to gravity is not fixed it changes from place to place Like at moon ‘g’ value is one-sixth of value on earth.

(iii) __Escape velocity__: The minimum value of the initial velocity at which an object to escape from the gravitational pull of the earth and never comes back to the earth is called the escape velocity.

__The escape velocity from earth is about 11.186 km/s,__ means if an object travels 11.186 km in 1 sec it will escape from earth’s gravitational pull. All the satellites and rockets are launched with a velocity equal to escape velocity in order to escape from the earth’s gravity.

(iv) __Centripetal force__: The force that acts on an object to keep it moving along the circular path with constant speed is called the centripetal force.

It is given by Fc =

It is directed towards the centre of the circle (of radius ‘r’) in which the object is moving ( with velocity ‘v’).

Example: The stone tied to a piece of string whirl in a circle due to centripetal force only.

The diagram below illustrates the centripetal force acting on an object towards the centre.

Question 4.Answer the following question.

Write the three laws given by Kepler. How did they help Newton to arrive at the inverse square law of gravity?

Answer:Johannes Kepler studied about the planets motion and their positions and. He noticed that motion of the planets follows a certain law. He gave three laws describing the planetary motion. These are known as Kepler’s laws which are as follows:

__Kepler’s First law__: The orbit of planet is an ellipse with sun at one of the foci. The figure below illustrates the elliptical orbit of earth with sun at its focus.

__Kepler’s Second law__: The line joining the planet and the Sun sweeps equal areas in equal intervals of time.

In the above figure A1 = A2 according to law.

__Kepler’s Third law__: The Square of its period of revolution around the Sun is directly proportional to the cube of the mean distance of a planet from the Sun.

If ‘r’ is the average distance of the planet from the sun and ‘T’ is the period of revolution then according to third law;

__Inverse Square law of gravity__: We know that centripetal force F is given by ;

F =

Where v = velocity of the planet =

Distance travelled in one revolution=2πr

Where r = radius of the orbit.

V =

F =

According to Kepler’s third law;

Hence

F = (Multiplying and dividing by r2)

F =

F = (By Kepler’s third law).

But is constant

Therefore

And this is __the newton’s inverse square law which states that the centripetal force acting on planet is inversely proportional to the square of the distance (‘r’) between the sun and the planet__

Question 5.Answer the following question.

A stone thrown vertically upwards with initial velocity u reaches a height ‘h’ before coming down. Show that the time taken to go up is same as the time taken to come down.

Answer:Given;

Initial velocity = u;

Distance travelled(s) = h;

Diagram below shows the situation given in the question;

__Time to go up (t__1): By Newton’s first equation of the motion

v = u + at

Where v = final velocity;

u= initial velocity

a = acceleration;

t = time taken;

According to our question;

v = 0 (because object has reach a maximum height ‘h’ before coming down and velocity at maximum height is zero);

u= u;

a = -g (because when object will be going up the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is opposite therefore a is negative);

T = t1;

Putting the values in the equation of motion we get;

.

__Time of descent (t2)__: By Newton’s second equation of motion

Where;

s = Distance travelled;

u = initial velocity;

a = acceleration;

t = time taken;

According to our question;

s = h;

u = 0 (When the object is at maximum height its velocity is zero);

a = g (because when object will be down the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is same therefore a is positive);

T = t2;

Putting the values in the equation we get;

From newton’s third equation of the motion;

Where symbols have usual meanings as above;

When the object is descending down

u = 0 (When the object is at maximum height its velocity is zero);

v = u (Final velocity will be the same as initial velocity);

a = g (because when object will be down the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is same therefore a is positive);

s = ;

Putting values in the equation of motion ;

Hence

Since t1 = t2 =

__Hence the time of ascent and time of descent are equal__;

Question 6.Answer the following question.

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:For lifting any body of mass ‘m’ the force(F1) required is equal to ‘mg’ where

g = acceleration due to gravity;

(Since Force= Mass × Accleration

Therefore F1 =

Now if the value of ‘g’ suddenly becomes twice its value than force(F2) required will be

F2 = .

We can see that

Therefore it becomes difficult to pull a heavy object if value of ‘g’ becomes twice its value as double the force is required to overcome the acceleration produced by the force of attraction of earth acting in downward direction

Question 7.Explain why the value of g is zero at the centre of the earth.

Answer:The value of ‘g’ changes as we go inside the earth. According to formula of . As we go deep inside the earth the Value of ’R’ decreases therefore according to formula the value of ‘g’ should increase. But it is not so because as we go inside the earth towards its center the part of the earth(M) responsible for the gravitational force also decreases that is the value of the ‘M’ also decreases.

And due to the combined result of decrease of ‘R’ and ‘M’ the value of ‘g’ decreases as we go inside the earth and is zero at the center of the earth.

Question 8.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 √8 T.

Answer:By Kepler’s Third law of planetary motion;

Where ‘r’ is the distance of planet from the star; ‘T’ is the period of revolution.

Let T1 be the time period when planet was at a distance of ‘2R’ from the star.

By Kepler’s third law;

Since K is constant and its value is same therefore;

⇒

⇒

__Hence Period of revolution will be____times the period of revolution when planet was at distance ‘R’ from the star.__

Question 9.Solve the following example.

An object takes 5 s to reach the ground from a height of 5 m on a planet. What is the value of g on the planet?

Answer:Given;

Time for object to reach ground (t) = 5 s;

Height of object from the ground(s) = 5m;

Acceleration due to gravity (g) =? ;

Since when Object is released from the height of 5m it will be in free fall hence its initial velocity (u) = 0;

Now, By Newton’s second equation of motion

Here u = 0, a = g, t = 5s, s = 5m;

Putting these values in the above equation we get;

⇒ .

⇒ .

⇒ .

__Hence acceleration due to gravity on the planet is 0.4m/s2.__

Question 10.Solve the following example.

The radius of planet A is half the radius of planet B. If the mass of A is MA, what must be the mass of B so that the value of g on B is half that of its value on A?

Answer:We know that acceleration due to gravity (g) is given by

Where G = universal gravitational constant;

M = mass of the planet;

R = radius of the planet;

Mass of Planet A = MA;

Radius of Planet A = RA;

Value of ‘g’ on A = gA;

Mass of Planet B = MB;

Radius of Planet B = RB;

Value of ‘g’ on B = gB;

Also it is given that;

Therefore;

(from question )

⇒

__Therefore the mass of planet B should be two times the mass of planet A i.e MB = 2MA__ .

Question 11.Solve the following example.

The mass and weight of an object on earth are 5 kg and 49 N respectively. What will be their values on the moon? Assume that the acceleration due to gravity on the moon is 1/6th of that on the earth.

Answer:__Mass value:__ Since mass is the amount of matter present in our body and it remains same irrespective of the change in position. Therefore the value of mass will be 5 Kg on moon as well.

__Weight value:__ Weight is the force with which an object is attracted by a planet and it is equal to;

Where m = mass of the object;

g = acceleration due to gravity;

On earth weight(W1) = mg = 49N;

On moon weight(W2) = (acceleration due to gravity is one-sixth of earth).

Hence weight on moon =

__Therefore Mass on moon is 5kg and weight on moon is 8.17N.__

Question 12.Solve the following example.

An object thrown vertically upwards reaches a height of 500 m. What was its initial velocity? How long will the object take to come back to the earth? Assume g = 10 m/s2

Answer:From newton’s third equation of the motion;

Where;

V = Final velocity;

U = initial velocity;

T = time taken;

S = distance travelled;

A = acceleration;

According to our question;

The figure below illustrates the situation given in the question

V = 0 (Velocity at maximum height is zero);

S = 500m;

A = -10m/s2 (because when object will be going up the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is opposite therefore a is negative);

Putting the above values we get

⇒u= √1000=100

__Therefore initial velocity is 100m/s__.

From the Newton’s first law of motion;

Where symbols have there usual meanings as above;

v = 0 (velocity at maximum height is zero);

u = initial velocity = 100m/s;

a = - 10m/s2 (because when object will be going up the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is opposite therefore a is negative);

Putting the values we get;

Now we know that time required by an object to go up is same as time required to come down.

Therefore;

Total time = time of ascent + time of descent = 10 + 10 = 20 s

__Hence total time to come back to earth is 20 seconds.__

Question 13.Solve the following example.

A ball falls off a table and reaches the ground in 1 s. Assuming g = 10 m/s2, calculate its speed on reaching the ground and the height of the table.

Answer:From the Newton’s first law of motion;

V = Final velocity;

U = initial velocity;

T = time taken;

A = acceleration;

According to our question;

u = 0 (ball is at table and is falling from it (free fall) hence its initial velocity is zero);

A = 10m/s2 (because when object will be down the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is same therefore a is positive);

T = 1 sec ( given);

The figure below describes the ball falling from the table on ground with final velocity v.

Putting the values we get;

__Hence final velocity on reaching the ground is 10m/s.__

__Height of table__ Now, By Newton’s second equation of motion

According to our question;

s = Table height;

u = 0 (ball is at table (maximum height) and is falling from it hence its initial velocity is zero);

a = 10m/s2.

t = 1s.

Putting the above values we get

__Hence height of the table is 5m__

Question 14.Solve the following example.

The masses of the earth and moon are 6 x 1024 kg and 7.4x1022 kg, respectively. The distance between them is 3.84 x 105 km. Calculate the gravitational force of attraction between the two?

Use G = 6.7 x 10-11 N m2 kg-2

Answer:Gravitational force of attraction between two bodies of masses m1 and m2separated by a distance of R is given by;

G = Gravitational constant;

Figure below illustrates the question well;

Putting values of m1 =;

m2 = ;

R = = m (since 1km = 1000m);

__Therefore the gravitational force of attraction between the earth and the moon is____.__

Question 15.Solve the following example.

The mass of the earth is 6 x 1024 kg. The distance between the earth and the Sun is 1.5x 1011 m. If the gravitational force between the two is 3.5 x 1022 N, what is the mass of the Sun?

Use G = 6.7 x 10-11 N m2 kg-2

Answer:Gravitational force of attraction between two bodies of masses m1 and m2separated by a distance of R is given by;

G = Gravitational constant

Putting values of m1 = ;

;

.

⇒

Since

Since

.

__Therefore mass of the sun is__

Study the entries in the following table and rewrite them putting the connected items in a single row.

Answer:

Question 2.

Answer the following question.

What is the difference between mass and weight of an object. Will the mass and weight of an object on the earth be same as their values on Mars? Why?

Answer:

Following are the difference between the weight and mass of an object.

i. Since mass is the amount of the matter present in the body, and amount of matter (ex: bones, blood, skin etc) is same everywhere. Therefore the mass of the object on earth will be the same as that on the mars.

ii. whereas the weight of an object on Earth and Mars will be different as the value of accelearation due to gravity(g) is different for Earth and Mars and we know that Weight= Mass × g. Therefore, the weight of the object will be different on Mars as that on the surface of Earth

Question 3.

Answer the following question.

What are (i) free fall, (ii) acceleration due to gravity (iii) escape velocity (iv) centripetal force?

Answer:

(i) __Free Fall__: Whenever an object moves under the influence of the force of gravity alone, it is said to be in Free Fall. During __free fall initial velocity of an object is zero__ and force of air also acts on an object. Thus real free fall is possible only in a vacuum because there is no air.

For Example:

a) When an object is dropped from the top of the table it falls down only due to gravitational force hence it is under free fall.

b) An apple falling from the tree.

But when we are standing on the ground, flying in a flight we are not in free fall because other forces except gravitational force are also acting.

(ii) __Acceleration due to gravity__: The acceleration which is gained by an object because of the gravitational force is called acceleration due to gravity. Its S.I unit is m/s2. It is denoted by ‘g’ and its value at the surface of the earth is 9.8m/s2.

It is a vector quantity (have both magnitude and direction) and it is directed towards the centre of the earth. The value of acceleration due to gravity is not fixed it changes from place to place Like at moon ‘g’ value is one-sixth of value on earth.

(iii) __Escape velocity__: The minimum value of the initial velocity at which an object to escape from the gravitational pull of the earth and never comes back to the earth is called the escape velocity.

__The escape velocity from earth is about 11.186 km/s,__ means if an object travels 11.186 km in 1 sec it will escape from earth’s gravitational pull. All the satellites and rockets are launched with a velocity equal to escape velocity in order to escape from the earth’s gravity.

(iv) __Centripetal force__: The force that acts on an object to keep it moving along the circular path with constant speed is called the centripetal force.

It is given by Fc =

It is directed towards the centre of the circle (of radius ‘r’) in which the object is moving ( with velocity ‘v’).

Example: The stone tied to a piece of string whirl in a circle due to centripetal force only.

The diagram below illustrates the centripetal force acting on an object towards the centre.

Question 4.

Answer the following question.

Write the three laws given by Kepler. How did they help Newton to arrive at the inverse square law of gravity?

Answer:

Johannes Kepler studied about the planets motion and their positions and. He noticed that motion of the planets follows a certain law. He gave three laws describing the planetary motion. These are known as Kepler’s laws which are as follows:

__Kepler’s First law__: The orbit of planet is an ellipse with sun at one of the foci. The figure below illustrates the elliptical orbit of earth with sun at its focus.

__Kepler’s Second law__: The line joining the planet and the Sun sweeps equal areas in equal intervals of time.

In the above figure A1 = A2 according to law.

__Kepler’s Third law__: The Square of its period of revolution around the Sun is directly proportional to the cube of the mean distance of a planet from the Sun.

If ‘r’ is the average distance of the planet from the sun and ‘T’ is the period of revolution then according to third law;

__Inverse Square law of gravity__: We know that centripetal force F is given by ;

F =

Where v = velocity of the planet =

Distance travelled in one revolution=2πr

Where r = radius of the orbit.

V =

F =

According to Kepler’s third law;

Hence

F = (Multiplying and dividing by r2)

F =

F = (By Kepler’s third law).

But is constant

Therefore

And this is __the newton’s inverse square law which states that the centripetal force acting on planet is inversely proportional to the square of the distance (‘r’) between the sun and the planet__

Question 5.

Answer the following question.

A stone thrown vertically upwards with initial velocity u reaches a height ‘h’ before coming down. Show that the time taken to go up is same as the time taken to come down.

Answer:

Given;

Initial velocity = u;

Distance travelled(s) = h;

Diagram below shows the situation given in the question;

__Time to go up (t__1): By Newton’s first equation of the motion

v = u + at

Where v = final velocity;

u= initial velocity

a = acceleration;

t = time taken;

According to our question;

v = 0 (because object has reach a maximum height ‘h’ before coming down and velocity at maximum height is zero);

u= u;

a = -g (because when object will be going up the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is opposite therefore a is negative);

T = t1;

Putting the values in the equation of motion we get;

.

__Time of descent (t2)__: By Newton’s second equation of motion

Where;

s = Distance travelled;

u = initial velocity;

a = acceleration;

t = time taken;

According to our question;

s = h;

u = 0 (When the object is at maximum height its velocity is zero);

a = g (because when object will be down the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is same therefore a is positive);

T = t2;

Putting the values in the equation we get;

From newton’s third equation of the motion;

Where symbols have usual meanings as above;

When the object is descending down

u = 0 (When the object is at maximum height its velocity is zero);

v = u (Final velocity will be the same as initial velocity);

a = g (because when object will be down the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is same therefore a is positive);

s = ;

Putting values in the equation of motion ;

Hence

Since t1 = t2 =

__Hence the time of ascent and time of descent are equal__;

Question 6.

Answer the following question.

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:

For lifting any body of mass ‘m’ the force(F1) required is equal to ‘mg’ where

g = acceleration due to gravity;

(Since Force= Mass × Accleration

Therefore F1 =

Now if the value of ‘g’ suddenly becomes twice its value than force(F2) required will be

F2 = .

We can see that

Therefore it becomes difficult to pull a heavy object if value of ‘g’ becomes twice its value as double the force is required to overcome the acceleration produced by the force of attraction of earth acting in downward direction

Question 7.

Explain why the value of g is zero at the centre of the earth.

Answer:

The value of ‘g’ changes as we go inside the earth. According to formula of . As we go deep inside the earth the Value of ’R’ decreases therefore according to formula the value of ‘g’ should increase. But it is not so because as we go inside the earth towards its center the part of the earth(M) responsible for the gravitational force also decreases that is the value of the ‘M’ also decreases.

And due to the combined result of decrease of ‘R’ and ‘M’ the value of ‘g’ decreases as we go inside the earth and is zero at the center of the earth.

Question 8.

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 √8 T.

Answer:

By Kepler’s Third law of planetary motion;

Where ‘r’ is the distance of planet from the star; ‘T’ is the period of revolution.

Let T1 be the time period when planet was at a distance of ‘2R’ from the star.

By Kepler’s third law;

Since K is constant and its value is same therefore;

⇒

⇒

__Hence Period of revolution will be____times the period of revolution when planet was at distance ‘R’ from the star.__

Question 9.

Solve the following example.

An object takes 5 s to reach the ground from a height of 5 m on a planet. What is the value of g on the planet?

Answer:

Given;

Time for object to reach ground (t) = 5 s;

Height of object from the ground(s) = 5m;

Acceleration due to gravity (g) =? ;

Since when Object is released from the height of 5m it will be in free fall hence its initial velocity (u) = 0;

Now, By Newton’s second equation of motion

Here u = 0, a = g, t = 5s, s = 5m;

Putting these values in the above equation we get;

⇒ .

⇒ .

⇒ .

__Hence acceleration due to gravity on the planet is 0.4m/s2.__

Question 10.

Solve the following example.

The radius of planet A is half the radius of planet B. If the mass of A is MA, what must be the mass of B so that the value of g on B is half that of its value on A?

Answer:

We know that acceleration due to gravity (g) is given by

Where G = universal gravitational constant;

M = mass of the planet;

R = radius of the planet;

Mass of Planet A = MA;

Radius of Planet A = RA;

Value of ‘g’ on A = gA;

Mass of Planet B = MB;

Radius of Planet B = RB;

Value of ‘g’ on B = gB;

Also it is given that;

Therefore;

(from question )

⇒

__Therefore the mass of planet B should be two times the mass of planet A i.e MB = 2MA__ .

Question 11.

Solve the following example.

The mass and weight of an object on earth are 5 kg and 49 N respectively. What will be their values on the moon? Assume that the acceleration due to gravity on the moon is 1/6th of that on the earth.

Answer:

__Mass value:__ Since mass is the amount of matter present in our body and it remains same irrespective of the change in position. Therefore the value of mass will be 5 Kg on moon as well.

__Weight value:__ Weight is the force with which an object is attracted by a planet and it is equal to;

Where m = mass of the object;

g = acceleration due to gravity;

On earth weight(W1) = mg = 49N;

On moon weight(W2) = (acceleration due to gravity is one-sixth of earth).

Hence weight on moon =

__Therefore Mass on moon is 5kg and weight on moon is 8.17N.__

Question 12.

Solve the following example.

An object thrown vertically upwards reaches a height of 500 m. What was its initial velocity? How long will the object take to come back to the earth? Assume g = 10 m/s2

Answer:

From newton’s third equation of the motion;

Where;

V = Final velocity;

U = initial velocity;

T = time taken;

S = distance travelled;

A = acceleration;

According to our question;

The figure below illustrates the situation given in the question

V = 0 (Velocity at maximum height is zero);

S = 500m;

A = -10m/s2 (because when object will be going up the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is opposite therefore a is negative);

Putting the above values we get

⇒u= √1000=100

__Therefore initial velocity is 100m/s__.

From the Newton’s first law of motion;

Where symbols have there usual meanings as above;

v = 0 (velocity at maximum height is zero);

u = initial velocity = 100m/s;

a = - 10m/s2 (because when object will be going up the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is opposite therefore a is negative);

Putting the values we get;

Now we know that time required by an object to go up is same as time required to come down.

Therefore;

Total time = time of ascent + time of descent = 10 + 10 = 20 s

__Hence total time to come back to earth is 20 seconds.__

Question 13.

Solve the following example.

A ball falls off a table and reaches the ground in 1 s. Assuming g = 10 m/s2, calculate its speed on reaching the ground and the height of the table.

Answer:

From the Newton’s first law of motion;

V = Final velocity;

U = initial velocity;

T = time taken;

A = acceleration;

According to our question;

u = 0 (ball is at table and is falling from it (free fall) hence its initial velocity is zero);

A = 10m/s2 (because when object will be down the acceleration due to gravity will be acting downwards to make object to fall. Hence by sign convention direction of motion and acceleration is same therefore a is positive);

T = 1 sec ( given);

The figure below describes the ball falling from the table on ground with final velocity v.

Putting the values we get;

__Hence final velocity on reaching the ground is 10m/s.__

__Height of table__ Now, By Newton’s second equation of motion

According to our question;

s = Table height;

u = 0 (ball is at table (maximum height) and is falling from it hence its initial velocity is zero);

a = 10m/s2.

t = 1s.

Putting the above values we get

__Hence height of the table is 5m__

Question 14.

Solve the following example.

The masses of the earth and moon are 6 x 1024 kg and 7.4x1022 kg, respectively. The distance between them is 3.84 x 105 km. Calculate the gravitational force of attraction between the two?

Use G = 6.7 x 10-11 N m2 kg-2

Answer:

Gravitational force of attraction between two bodies of masses m1 and m2separated by a distance of R is given by;

G = Gravitational constant;

Figure below illustrates the question well;

Putting values of m1 =;

m2 = ;

R = = m (since 1km = 1000m);

__Therefore the gravitational force of attraction between the earth and the moon is____.__

Question 15.

Solve the following example.

The mass of the earth is 6 x 1024 kg. The distance between the earth and the Sun is 1.5x 1011 m. If the gravitational force between the two is 3.5 x 1022 N, what is the mass of the Sun?

Use G = 6.7 x 10-11 N m2 kg-2

Answer:

Gravitational force of attraction between two bodies of masses m1 and m2separated by a distance of R is given by;

G = Gravitational constant

Putting values of m1 = ;

;

.

⇒

Since

Since

.

__Therefore mass of the sun is__