Universal Law of Gravitation | Physics Class 11 - NEET PDF Download

In the 1600s, an English physicist and mathematician named Isaac Newton was sitting under an apple tree. Apparently, an apple fell on his head, and he started wondering why the apple was attracted to the ground in the first place. Today we all know that it happened due to the force of gravitation. 

Newton and fallen Apple led to discovery of Gravity

Newton’s Law Of Universal Gravitation

Newton’s Law of Universal Gravitation states that every particle attracts every other particle in the universe with a force that is directly proportional to the product of the masses and inversely proportional to the square of the distance between them.

The universal gravitation equation thus takes the form

Gravitation Equation

where F is the gravitational force between bodies, m₁ is the mass of one of the objects, m₂ is the mass of the second object, r is the distance between the centers of two objects, and G is the universal gravitational constant.
The constant proportionality (G) in the above equation is known as the universal gravitation constant. Henry Cavendish experimentally determined the precise value of G. 

The value of G is found to be G = 6.673 x 10^-11 N m²/kg².

Properties of Gravitational Force 

• The gravitational force is a conservative force, operating along the central axis connecting two objects, which qualifies it as a central force. 
• It remains unaffected by the medium between the two objects, as well as the characteristics and dimensions of the objects themselves. 
• This force complies with Newton's third law of motion, forming an action-reaction pair, and it remains unaltered by the presence or absence of other bodies in the surrounding environment.

Gravitation Equation Vector Form

The universal gravitation equation is represented in vector form as follows:

where G is the gravitational constant and r is the unit vector from m₁ to m₂. The figure below shows the gravitational force on m₁ due to m₂ along with r where the vector r is (r₂–r₁). 

If we have a collection of point masses, the force on any one of them is the vector sum of the gravitational forces exerted by the other point masses:

The gravitational force on point mass m₁ is the vector sum of the gravitational forces exerted by m₂, m₃ and m₄. Therefore, the total force on m₁ is given by: 

Example 1: Calculate the gravitational force of attraction between the Earth and a 70 kg man standing at sea level, a distance of 6.38 x 10⁶ m from the Earth’s center.
Solution:
Given,
m₁ is the mass of the Earth = 5.98 x 10²⁴ kg
m₂ is the mass of the man = 70 kg 
d = 6.38 x 10⁶ m 
The value of G = 6.673 x 10^-11 N m²/kg² 
Now substituting the values in the Gravitational force formula, we get

Example 2: A sphere of mass 100 kg is attracted by another spherical mass of 11.75 kg by a force of 19.6 x 10^-7 N when the distance between their centers is 0.2 m. Find G.
Solution: Mass of first body = m₁ = 100 kg, mass of second body = m₂ = 11.75 kg, distance between masses = r = 0.2 m, force between them = F =  19.6 x 10^-7 N,
To Find: Universal gravitation constant = G =?
By Newton’s law of gravitation

The value of the universal gravitation constant is 6.672 x 10^-11 N m²/kg².

Example 3: Calculate the gravitational force of attraction between two metal spheres each of mass 90 kg, if the distance between their centers is 40 cm. Given G = 6.67 x 10^-11 N m²/kg². Will the force of attraction be different if the same bodies are taken on the moon, their separation remaining the same?

Solution: Mass of first body = m₁ = 90 kg, mass of second body = m₂ = 90 kg, Distance between masses = r = 40 cm = 40 x 10^-2 m, G = 6.67 x 10-11 N m²/kg² .
To Find: Force of attraction = F =?
By Newton’s law of gravitation

If the same bodies are taken on the moon, their separation remains the same, the force of attraction between the two bodies will remain the same because the force of attraction between two bodies is unaffected by the presence of the third body and medium between the two bodies.
The force of attraction between two metal spheres is 3.377 x 10^-6 N.

Example 4: Three 5 kg masses are kept at the vertices of an equilateral triangle each of side of 0.25 m. Find the resultant gravitational force on any one mass. G = 6.67 x 10^-11 S.I. units.
Solution:  m₁ = 5 kg, m₂ = 5 kg, m₃ = 5 kg, r = 0.25 m, G = 6.67 x 10^-11 N m²/kg².
To find: Force on m1 =?
By Newton’s law of gravitation, the force on mass m₁ due to mass m₂.

By Newton’s law of gravitation, the force on mass m₁ due to mass m₃.
The angle between F₁₂ and F₁₃ is 60°. (Angle of an equilateral triangle). The net force on m₁ is given by
The two forces are equal, hence their resultant act along angle bisector towards centroid.
Force on any mass is 4.621 x 10^-8 N towards the centroid
Example 5: Two bodies of masses 5 kg and 6 x 10²⁴ kg are placed with their centres 6.4 x 10⁶ m apart. Calculate the gravitational force of attraction between the two masses. Also, find the initial acceleration of two masses assuming no other forces act on them.

Solution: Mass of first body = m₁ = 5 kg, mass of second body = m₂ = 6 x 10²⁴ kg, Distance between masses = r = 6.4 x 10⁶ m, G = 6.67 x 10^-11 N m²/kg² .
To Find: Force of attraction between two masses = F =? Initial accelerations of the two masses =?

Ans:
By Newton’s law of gravitation

Initial acceleration of the body of mass 5 kg
By Newton’s second law of motion F = ma
Thus a = F/m = 48.85 / 5 = 9.77 m/s²
Initial acceleration of the body of mass 6 x 10²⁴ kg
By Newton’s second law of motion F = ma
Thus a = F/m = 48.85 / 6 x 10²⁴ = 8.142 x 10^-24 m/s²
The force of attraction between the two masses = 48.85 N

Mass and Weight

In Newton’s law of gravity, we noticed that the mass is a crucial quantity. We consider mass and weight to be the same, but they are related but are different in reality. 

Difference between Mass and Weight

Universality of Gravity

• Gravitation interactions not only exist between the earth and other objects, but they also exist between all objects with an intensity that is directly proportional to the product of their masses.
• The law of universal gravitation helps scientists study planetary orbits. The small perturbations in a planet’s elliptical motion can be easily explained owing to the fact that all objects exert gravitational influences on each other.

Why doesn’t the moon crash into the earth?

The forces of speed and gravity are what keeps the moon in constant orbit around the Earth. The Moon seems to hover around in the sky, unaffected by gravity. However, the reason the Moon stays in orbit is precisely because of gravity. In this video, clearly, understand why the moon doesn’t fall into the earth

Is the force of Gravity the same all over the Earth?

Gravity isn’t the same everywhere on earth. Gravity is slightly stronger over the places with more underground mass than places with less mass. NASA uses two spacecraft to measure the variation in the Earth’s gravity. These spacecraft are a part of the Gravity Recovery and Climate Experiment (GRACE) mission.
Areas in blue have weaker gravity while areas in red have slightly stronger gravity.