Gravitation and Related Terms Class 11 Notes | EduRev

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Gravitation 

Introduction:

Newton observed that an object, an apple, when released near the earth surface is accelerated towards the earth. As acceleration is caused by an unbalanced force, there must be a force pulling objects towards the earth. 

If someone throws a projectile with some initial velocity, then instead of that object moving off into space in a straight line, it is continuously acted on by a force pulling it back to earth. If we throw the projectile with greater velocity then the path of projectile would be different as well and its range is also increased with initial velocity. 

Gravitation and Related Terms Class 11 Notes | EduRevFig: Difference between gravitation and gravity

If the projection velocity is further increased until at some initial velocity, the body would not hit the earth at all but would go right around it in an orbit. But at any point along its path the projectile would still have a force acting on it pulling it toward the surface of earth.

Newton was led to the conclusion that the same force that causes the apple to fall to the earth also causes the moon to be pulled to the earth. Thus the moon moves in its orbit about the earth because it is pulled toward the earth. 

But if there is a force between the moon and the earth, why not a force between the sun and the earth or why not a force between the sun and the other planets? 

Newton proposed that the same force, named gravitational force which acts on objects near the earth surface also acts on all the heavenly bodies. 

He proposed that there was a force of gravitation between each and every mass in the universe.

1.1 Newtons's Law of Universal Gravitation:

All physical bodies are subjected to the action of the forces of mutual gravitational attraction. The basic law describing the gravitational forces was stated by Sir Issac Newton and it is called Newton's Law. of Universal gravitation.

The law is stated as : "Between any two particles of masses mI and m2 at separation r from each other there exist attractive forces and directed from one body to the other and equal in magnitude which is directly proportional to the product of the masses of the bodies and inversely proportional to the square of the distance between the two". Thus we can write

Gravitation and Related Terms Class 11 Notes | EduRev ...(1)

Where G is called universal gravitational constant. Its value is equal to 6.67 × 10-11 Nm2/kg. The law of gravitation can be applied to the bodies whose dimensions are small as compared to the separation between the two or when bodies can be treated as point particles.

Gravitation and Related Terms Class 11 Notes | EduRev

If the bodies are not very small sized, we can not directly apply the expression in equation-(1) to find their natural gravitational attraction. In this case we use the following procedure to find the same. The bodies are initially split into small parts or a large number of point masses. 

Now using equation-(1) the force of attraction exerted on a particle of one body by a particle of another body can be obtained. Now we add all forces vectorially which are exerted by all independent particles of second body on the particle of first body. 

Finally the resultants of these forces is summed over all particles of the first body to obtain the net force experinced by the bodies. 

In general we use integration or basic summation of these forces.

⇒ Gravitational force is a conservative force.

⇒ Gravitational force is a central force.

⇒ Gravitational force is equal in magnitude & opposite in direction

⇒ Gravitational forces are action - reaction pair.

⇒ Gravitational force acts along the line joining the two masses.

⇒ Gravitational force doesn't depend upon the medium

⇒ Gravitational force is an attractive force.

Gravitation and Related Terms Class 11 Notes | EduRev

[Head of is placed at that position where we have to evaluate force]


2. Gravitational Field: 

We can state by Newton's universal law of gravitation that every mass M produces, in the region around it, a physical situation in which, whenever any other mass is placed, force acts on it, is called gravitational field. This field is recognized by the force that the mass M exerts another mass, such as m, brought into the region.

Gravitation and Related Terms Class 11 Notes | EduRevFig: Gravitational field around the earth

2.1 Strength of Gravitational Field: 

We define gravitational field strength at any point in space to be the gravitational force per unit mass on a test mass (mass brought into the field for experimental observation).

Thus for a point in space if a test mass m0, experiences a force Gravitation and Related Terms Class 11 Notes | EduRev, then at that point in space, gravitational field strength which is denoted by Gravitation and Related Terms Class 11 Notes | EduRev, is given as Gravitation and Related Terms Class 11 Notes | EduRev

Gravitational field strength Gravitation and Related Terms Class 11 Notes | EduRev is a vector quantity and has same direction as that of the force on the test mass in field.

Generally magnitude of test mass is very small such that its gravitational field does not modify the field that is being measured. 

It should be also noted that gravitational field strength is just the acceleration that a unit mass would experience at that point in space.

2.2 Gravitational Field Strength of Point Mass: 

As per our previous discussion we can state that every point mass also produces a gravitational field in its surrounding. To find the gravitational field strength due to a point mass, we put a test mass m0 at a point P at distance x from a point mass m then force on m0 is given as:

Gravitation and Related Terms Class 11 Notes | EduRev   
Gravitation and Related Terms Class 11 Notes | EduRev

Now if at point P, gravitational field strength due to m is gp then it is given as

Gravitation and Related Terms Class 11 Notes | EduRev

The expression written in above equation gives the gravitational field strength at a point due to a point mass.

It should be noted that the expression in equation written above is only applicable for gravitational field strength due to point masses. It should not be used for extended bodies.

However, the expression for the gravitational field strength produced by extended masses has already been derived in electrostatics section.

[Just replace k by -G & Q by M in those expressions].

So we will just revise the expression of gravitational field strength at points due to various extended masses. Gravitational field strength :

1. At a point on the axis of Ring = Gravitation and Related Terms Class 11 Notes | EduRev

2. At a point on the axis of disc = Gravitation and Related Terms Class 11 Notes | EduRev

3. At an axial point of a rod = Gravitation and Related Terms Class 11 Notes | EduRev

4. Due to a circular Arc = Gravitation and Related Terms Class 11 Notes | EduRev

5. Due to a long infinite thread = Gravitation and Related Terms Class 11 Notes | EduRev

6. Due to long solid cylinder

(a) at an outer point = Gravitation and Related Terms Class 11 Notes | EduRev (where r is mass density per volume)

(b) at an inner point = - 2G r πx

7. Due to hollow sphere :

Gravitation and Related Terms Class 11 Notes | EduRev

(a) for outer points = Gravitation and Related Terms Class 11 Notes | EduRev (Behaving as a point mass)           

(b) for points on surface = Gravitation and Related Terms Class 11 Notes | EduRev (Behaving as a point mass)

(c) for inner points = 0 (As no mass is enclosed within it)

8. Due to solid sphere

Gravitation and Related Terms Class 11 Notes | EduRev

(a) For outer points = Gravitation and Related Terms Class 11 Notes | EduRev (Behaving as a point mass)
(b) For points on surface = Gravitation and Related Terms Class 11 Notes | EduRev (Behaving as a point mass)
(c) For inner points = Gravitation and Related Terms Class 11 Notes | EduRev


3. Interaction Energy: 

This energy exists in a system of particles due to the interaction forces between the particles of system. Analytically this term is defined as the work done against the interaction of system forces in assembling the given configuration of particles. 

To understand this we take a simple example of interaction energy of two points masses.

Figure (a) shows a system of two point masses m1 and m2 placed at a distance r apart in space. here if we wish to find the interaction potential energy of the two masses, this must be the work done in bringing the two masses from infinity (zero interaction state) to this configuration. 

For this we first fix m1 at its position and bring m2 slowly from infinity to its location. If in the process m2 is at a distance x from m1 then force on it is

Gravitation and Related Terms Class 11 Notes | EduRev

Gravitation and Related Terms Class 11 Notes | EduRev     Gravitation and Related Terms Class 11 Notes | EduRev

This force is applied by the gravitational field of m1 to m2. If it is further displaced by a distance dx towards m1 then work done by the field is

Gravitation and Related Terms Class 11 Notes | EduRev = Gravitation and Related Terms Class 11 Notes | EduRev

Now in bringing m2 from infinity to a position at a distance r from m1, the total work done by the field is

Gravitation and Related Terms Class 11 Notes | EduRev = - G m1 m2Gravitation and Related Terms Class 11 Notes | EduRev

Gravitation and Related Terms Class 11 Notes | EduRev

Thus during the process field of system has done Gravitation and Related Terms Class 11 Notes | EduRev amount of work. The work is positive because the displacement of body is in the direction of force.

Initially when the separation between m1 and m2 was very large (at infinity) there was no interaction between them. We conversely say that as a reference when there is no interaction the interaction energy of the system is zero and during the process system forces (gravitational forces) are doing work so system energy will decrease and becomes negative (as initial energy was zero). 

As a consequence we can state that in general if system forces are attractive, in assembling a system of particles work will be done by the system and it will spend energy in assembling itself. Thus finally the interaction energy of system will be negative. On the other hand if in a given system of particles, the system forces are repulsive, then in assembling a system some external forces have to be work against the system forces and in this case some work must be done by external forces on the system hence finally the interaction energy of the system of particles must be positive.

In above example as work is done by the gravitational forces of the system of two masses, the interaction energy of system must be negative and it can be given as

Gravitation and Related Terms Class 11 Notes | EduRev ...(1)

As gravitational forces are always attractive, the gravitational potential energy is always taken negative.

3.1 Interaction Energy of a System of Particles: 

If in a system there are more than two particles then we can find the interaction energy of particle in pairs using equation (1) and finally sum up all the results to get the total energy of the system. For example in a system of N particles with masses m1, m2........mn separated from each other by a distance r12........ where r12 is the separation between m1 and m2 and so on.

In the above case the total interaction energy of system is given as:

Gravitation and Related Terms Class 11 Notes | EduRev

In this expression the factor Gravitation and Related Terms Class 11 Notes | EduRev is taken because the interaction energy for each possible pair of system is taken twice during summation as for mass m1 and m3

Gravitation and Related Terms Class 11 Notes | EduRev = Gravitation and Related Terms Class 11 Notes | EduRev

Now to understand the applications of interaction energy we take few examples.


Ex. 1 Three particles each of the mass m are placed at the corners of an equilateral triangle of side d and shown in figure. Calculate (a) the potential energy of the system, (b) work done on this system if the side of the triangle is changed from d to 2d. 

 Gravitation and Related Terms Class 11 Notes | EduRev

Sol. (a) As in case of two-particle system potential energy is given by (-Gm1m2/r), so

U = U12 + U23 +  U31 or Gravitation and Related Terms Class 11 Notes | EduRev

(b) When d is changed to 2d,

Uf = - Gravitation and Related Terms Class 11 Notes | EduRev

Thus work done in changing in potential energy is given as

W = U - Ui = Gravitation and Related Terms Class 11 Notes | EduRev


Ex. 2 Two particles m1 and m2 are initially at rest at infinite distance. Find their relative velocity of approach due to gravitational atraction when their separation is d. 

Sol. Initiallly when the separation was large there was no interaction energy and when they get closer the system gravitational energy decreases and the kinetic energy increases.

When separation between the two particles is d, then according to energy conservation we have

Gravitation and Related Terms Class 11 Notes | EduRev

As no other force is present we have according to momentum conservation

m1v1 = m2v2

From equations written above

Gravitation and Related Terms Class 11 Notes | EduRev or Gravitation and Related Terms Class 11 Notes | EduRev

And on further solving we get

Gravitation and Related Terms Class 11 Notes | EduRev

Thus approach velocity is given as

Gravitation and Related Terms Class 11 Notes | EduRev


Ex. 3 If a particle of mass 'm' is projected from a surface of bigger sphere of mass '16M' and radius '2a' then find out the minimum velocity of the particle such that the particle reaches the surface of the smaller sphere of mass M and radius 'a'. Given that the distance between the centres of two spheres is 10 a. 

Sol. When the particle is at the surface of bigger sphere it is attracted more by the bigger sphere and less by the smaller sphere. As it is projected the force of attraction from bigger sphere decreases and that from smaller sphere increass and thus the particle reaches the state of equilibrium at distance x from the centre smaller sphere

Gravitation and Related Terms Class 11 Notes | EduRev

Gravitation and Related Terms Class 11 Notes | EduRev

(10a - x)2 = 16x

10a - x = 4x ⇒ x = 2a

Gravitation and Related Terms Class 11 Notes | EduRev

After this point the attraction on the particle from the smaller sphere becomes more than that from the bigger sphere and the particle will automatically move towards the smaller sphere. Hence the minimum velocity to reach the smaller sphere is the veloicty required to reach the equilibrium state according to energy conservation, we have,

Gravitation and Related Terms Class 11 Notes | EduRev

Gravitation and Related Terms Class 11 Notes | EduRev ⇒ Gravitation and Related Terms Class 11 Notes | EduRev


4. Gravitational Potential: 

The gravitational potential at a point in gravitational field is the gravitational potential energy per unit mass placed at that point in gravitational field. Thus at a certain point in gravitational field, a mass m0 has a potential energy U then the gravitational potential at that point is given as:

V = Gravitation and Related Terms Class 11 Notes | EduRev

or if at a point in gravitational field gravitational potential V is known then the interaction potential energy of a point mass m0 at that point in the field is given as

U = m0v

Interaction energy of a point mass m0 in a field is defined as work done in bringing that mass from infinity to that point. In the same fashion we can define gravitational potential at a point in field, alternatively as "Work done in bringing a unit mass from infinity to that point against gravitational forces."

When a unit mass is brought to a point in a gravitational field, force on the unit mass is Gravitation and Related Terms Class 11 Notes | EduRevat a point in the field. Thus the work done in bringing this unit mass from infinity to a point P in gravitational field or gravitational potential at point P is given as

Gravitation and Related Terms Class 11 Notes | EduRev

Here negative sign shown that VP is the negative of work done by gravitation field or it is the external required work for the purpose against gravitational forces.

4.1 Gravitational Potential due to a Point Mass:

We know that in the surrounding of a point mass it produces its gravitational field. If we wish to find the gravitational potential at a point P situated at a distance r from it as shown in figure,

Gravitation and Related Terms Class 11 Notes | EduRev

we place a test mass m0 at P and we find the interaction energy of m0 with the field of m, which is given as

Gravitation and Related Terms Class 11 Notes | EduRev

Now the gravitational potential at P due to m can be written as

Gravitation and Related Terms Class 11 Notes | EduRev

The expression of gravitational potential in equation is a standard result due to a point mass which can be used as an elemental form to find other complex results, we'll see later.

The same thing can also be obtained by using equation

Gravitation and Related Terms Class 11 Notes | EduRev or Gravitation and Related Terms Class 11 Notes | EduRev or Gravitation and Related Terms Class 11 Notes | EduRev

4.2 Gravitational potential: 

1. Due to a rod at an a xial point = - Glln Gravitation and Related Terms Class 11 Notes | EduRev

2. Due to ring at an axial point = Gravitation and Related Terms Class 11 Notes | EduRev

3. Due to ring at the centre = Gravitation and Related Terms Class 11 Notes | EduRev

4. Due to Disc = Gravitation and Related Terms Class 11 Notes | EduRev (where s is mass density per unit area)

5. Due to hollow sphere

Gravitation and Related Terms Class 11 Notes | EduRev

for outer points = Gravitation and Related Terms Class 11 Notes | EduRev

For surface points = Gravitation and Related Terms Class 11 Notes | EduRev

For inner points = Gravitation and Related Terms Class 11 Notes | EduRev

6. Due to solid sphere

Gravitation and Related Terms Class 11 Notes | EduRev

For outer points = Gravitation and Related Terms Class 11 Notes | EduRev

For surface points = Gravitation and Related Terms Class 11 Notes | EduRev

For inner points = Gravitation and Related Terms Class 11 Notes | EduRev

Potential energy of hollow sphere = Gravitation and Related Terms Class 11 Notes | EduRev

Potential energy of solid sphere = Gravitation and Related Terms Class 11 Notes | EduRev


5. Gravitational Lines of Forces: 

Gravitational field can also be represented by lines of force. A line of force is drawn in such a way that at each point the direction of field is tangent to line that passes through the point. Thus tangent to any point on a line of force gives the direction of gravitational field at that point. By convention lines of force are drawn in such a way that their density is proportional to the strength of field.

Gravitation and Related Terms Class 11 Notes | EduRev

Figure shown shows the field of a point mass in its surrounding. We can see that the lines of force are radially inward giving direction of field and as we go closer to the mass the density of lines is more which shows that field strength is increasing.

Gravitation and Related Terms Class 11 Notes | EduRev

Figure shown shows the configuration of field lines for a system of two equal masses separated by a given distance.

Here we can see that there is no point where any two lines of force intersects or meet. The reason is obvious that at one point in space there can never be two direction of gravitational fields. It should be noted that a line of force gives the direction of net gravitational field in the region. Like electric field gravitational field never exists in closed loops.

  • Gravitational Flux :Gravitation and Related Terms Class 11 Notes | EduRev 
  • Gravitational Gauss law : Gravitation and Related Terms Class 11 Notes | EduRev

Here Gravitation and Related Terms Class 11 Notes | EduRev is the gravitational field due to all the masses. Min is the mass inside the assumed gaussian surface.

5.1 Gravitational Field Strength of Earth: 

We can consider earth to be a very large sphere of mass Me and radius Re. Gravitational field strength due to earth is also regarded as acceleration due to gravity or gravitational acceleration. Now we find values of g at different points due to earth.

  • Earth behaves as a non conducting solid sphere.

 5.2 Value of g on Earth's Surface: 

Gravitation and Related Terms Class 11 Notes | EduRev

If gs be the gravitational field strength at a point A on the surface of earth, then it can be easily obtained by using the result of a solid sphere. Thus for earth, value of gs can be given as

Gravitation and Related Terms Class 11 Notes | EduRev ...(1)

5.3 Value of g at a Height h Above the Earth's Surface:

Gravitation and Related Terms Class 11 Notes | EduRev

If we wish to find the value of g at a point P as shown in figure shown at a height h above the Eath's surface. Then the value can be obtained as

Gravitation and Related Terms Class 11 Notes | EduRev or Gravitation and Related Terms Class 11 Notes | EduRev

If point P is very close to Earth's surface then for h << Re we can rewrite the expression in given equation as

Gravitation and Related Terms Class 11 Notes | EduRevGravitation and Related Terms Class 11 Notes | EduRev [Using binomial approximation] ...(2)

5.4 Value of g at a Depth h Below the Earth's Surface: 

Gravitation and Related Terms Class 11 Notes | EduRev

If we find the value of g inside the volume of earth at a depth h below the earth's surface at point P as shown in figure, then we can use the result of g inside a solid sphere as

Gravitation and Related Terms Class 11 Notes | EduRev

Here x, the distance of point from centre of earth is given as

x = Re - h

Thus we have Gravitation and Related Terms Class 11 Notes | EduRev ...(3)

From equation (1), (2) and (3) we can say that the value of g at earth's surface is maximum and as we move above the earth's surface or we go below the surface of earth, the value of g decrease.

5.5 Effect of Earth's Rotation on Value of g: 

Let us consider a body of mass m placed on Earth's surface at a latitude q as shown in figure. This mass experiences a force mgs towards the centre of earth and a centrifugal force mwe2 Re sinθ relative to Earth's surface as shown in figure.

Gravitation and Related Terms Class 11 Notes | EduRev

If we consider geff as the effective value of g on earth surface at a latitude q then we can write

geff = Gravitation and Related Terms Class 11 Notes | EduRev = Gravitation and Related Terms Class 11 Notes | EduRev

Gravitation and Related Terms Class 11 Notes | EduRev is very very small

So we can write Gravitation and Related Terms Class 11 Notes | EduRev

Gravitation and Related Terms Class 11 Notes | EduRev » g - we2 R sin2q ...(i)

From equation (1) we can find the value of effective gravity at poles and equatorial points on Earth as

At poles q = 0   ⇒   gpoles = gs = 9.83 m/s2

At equator q = Gravitation and Related Terms Class 11 Notes | EduRev    ⇒  gequator = gs - w2Re = 9.78 m/s2

Thus we can see that the body if placed at poles of Earth, it will only have a spin, not circular motion so there is no reduction in value of g at poles due to rotation of earth. Thus at poles value of g on Earth surface is maximum and at equator it is minimum. But an average we take 9.8 m/s2, the value of g everywhere on earth's surface.


5.6 Effect of Shape of Earth on Value of g 

Till now we considered that earth is spherical in its shape but this is not actually true. Due to some geological and astronomical reasons, the shape of earth is not exact spherical. It is ellipsoidal.

As we've discussed that the value of g at a point on earth surface depends on radius of Earth.It is observed that the approximate difference in earth's radius at different points on equator and poles is re - rp 21 to 34 km. 

Due to this the difference in value of g at poles and equatorial points is approximately gp - ge 0.02 to 0.04 m/s2, which is very small. 

So for numerical calculations, generally, we ignore this factor while taking the value of g and we assume Earth is spherical in shape.


Ex. 4 Calculate the mass and density of the earth. Given that Gravitational constant G = 6.67 × 10-11 Nm2/kg2, the radius of the earth = 6.37 × 106 m and g = 9.8 m/s2.

Sol. The acceleration due to gravity on earth surface is given as

ge = Gravitation and Related Terms Class 11 Notes | EduRev or Gravitation and Related Terms Class 11 Notes | EduRev = 6 × 1024 kg

If r be the density of earth, then

M = Gravitation and Related Terms Class 11 Notes | EduRev or r = Gravitation and Related Terms Class 11 Notes | EduRev = Gravitation and Related Terms Class 11 Notes | EduRev = 5.5 × 103 kg/m3


Ex. 5 If the radius of the earth were to shrink by one percent, its mass remaining the same, what would happen to the acceleration due to gravity on the earth's surface? 

Sol. Consider the case of body of mass m placed on the earth's surface (mass of the earth M and radius R). If g is acceleration due to gravity, then we known that

gs = Gravitation and Related Terms Class 11 Notes | EduRev ...(1)

Now, when the radius is reduced by 1%, i.e. radius becomes 0.99 R, let acceleration due to gravity be g', then

Gravitation and Related Terms Class 11 Notes | EduRev ...(2) 

From equation (1) and (2), we get

Gravitation and Related Terms Class 11 Notes | EduRev or Gravitation and Related Terms Class 11 Notes | EduRev or g' = 1.02 g

Thus, the value of g is increased by 2%.


Ex. 6 At what rate should the earth rotate so that the apparent g at the equator becomes zero? What will be the length of the day in this situation ? 

Sol. At earth's equator effective value of gravity is

geq = gs - w2Re

If geff at equator is zero, we have

gs = w2Re or Gravitation and Related Terms Class 11 Notes | EduRev

Thus length of the day will be Gravitation and Related Terms Class 11 Notes | EduRev = 2 × 3.14 Gravitation and Related Terms Class 11 Notes | EduRevGravitation and Related Terms Class 11 Notes | EduRev


Ex. 7 Calculate the acceleration due to gravity at the surface of Mars if its diameter is 6760 km and mass is one-tenth that of earth. The diameter of earth is 12742 km and acceleration due to gravity on earth is 9.8 m/s2.

We know that Gravitation and Related Terms Class 11 Notes | EduRev

So Gravitation and Related Terms Class 11 Notes | EduRev ⇒ Gravitation and Related Terms Class 11 Notes | EduRev or gM = 9.8 × 0.35 = 3.48 m/s2


Ex. 8 Calculate the apparent weight of a body of mass m at a latitude l when it is moving with speed v on the surface of the earth from west to east at the same latitude.  

Sol. 

Gravitation and Related Terms Class 11 Notes | EduRev

If W be the apparent weight of body at a latitude l then from figure shown, we have

W = mg - mw2R cos2λ ...(1)

When body moves at speed v from west to east relative to earth, its net angular speed w can be given as

Gravitation and Related Terms Class 11 Notes | EduRev[we ® earth's angular velocity]

Now from equation (1) we have

Gravitation and Related Terms Class 11 Notes | EduRev

or Gravitation and Related Terms Class 11 Notes | EduRev

Gravitation and Related Terms Class 11 Notes | EduRev

Gravitation and Related Terms Class 11 Notes | EduRev [Neglecting Gravitation and Related Terms Class 11 Notes | EduRev as being very small]

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