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Gravitation Class 9 Notes Science Chapter 9

Universal Law of Gravitation

  • Every object in the universe attracts every other object with a force which is proportional to the product of their masses and inversely proportional to the square of the distance between them.
  • The force is along the line joining the centres of two objects.
    Gravitation Class 9 Notes Science Chapter 9

Gravitational Force between two uniform objects is directed along the line joining their centres.

  • Let two objects A and B of masses M and m lie at a distance of d from each other as shown in the figure.
  • Let F be the force of attraction between two objects. According to the universal law of gravitationGravitation Class 9 Notes Science Chapter 9
  • G is called a universal constant because its value does not depend on the nature of the intervening medium temperature or any other physical variable.
  • S.I. unit of G = Nm2/kg
  • Value of G = 6.673 × 10−11 Nm2/kg2 (Found by Henry Cavendish)

Importance of Universal Law of Gravitation

The universal law of gravitation successfully explained several phenomena:
(i) the force that binds us to the earth.
(ii) the motion of the moon around the earth.
(iii) the motion of planets around the Sun.
(iv) the tides due to the moon and the Sun.

Free fall 
When an object falls towards the earth under the gravitational force alone, we say the object is in free fall.
The velocity of a freely falling body changes and is said to be accelerated.
This acceleration is called acceleration due to gravity, denoted by ‘g’. Unit is m/s2.
As F = ma                 (∵ a = g) ...(i)
F = mg                    ...(ii)
and
F = G(Mm/d2) (from Universal law of gravitation) ...(iii)
 From (ii) and (iii)
∴ mg = G(Mm/d2)
∴ g= GM/d2
M = Mass of the earth
d = Distance between the object and the earth
G = Gravitational constant If the object is placed on the earth then
d = R (R = radius of the earth)
Gravitation Class 9 Notes Science Chapter 9 ...(iv)

Earth is not a sphere, it is flattened at the poles.
Gravitation Class 9 Notes Science Chapter 9
Hence Rp − Radius at pole and R− Radius at equator
Gravitation Class 9 Notes Science Chapter 9
∴ The value of ‘g’ is more at poles = (9.9 m/s2) and less at equator = (9.8 m/s2)

Calculation of value of g
Gravitation Class 9 Notes Science Chapter 9
g= G(M/R2
G = 6.67 x 10-11 Nm2/kg2
M = 6 × 1024 kg (Mass of the earth)
R = 6.4 × 106 m
On substituting the given values
Gravitation Class 9 Notes Science Chapter 9

  • Motion of objects under the influence of gravity ‘g’ does not depend on the mass of the body. All objects small, big, heavy, light, hollow or solid fall at the same rate.
  •  The three equations of motion viz.
    (i) v = u + at
    (ii) s = ut + (1/2) at2
    (iii) v2 – u2 = 2 as is true for the motion of objects under gravity. For free fall, the value of acceleration a = g = 9.8 ms–2.
  • If an object is just let fall from a height then in that case u = 0 and a = g = 9.8 m/s2.
  • If an object is projected vertically upward with an initial velocity u, then a = – g = – 9.8 ms–2 and the object will go to a maximum height h where its final velocity becomes zero (i.e., v = 0).

Mass

The mass of an object is the measure of its inertia. It is the matter present in it. It remains the same everywhere in the universe.

Weight

The force of attraction of the earth on the object is known as the weight of the object. Its S.I. unit is Newton.
W = m × g
The weight of an object can change from one place to the other, from one planet to the other.
The weight of an object on the moon is given by the formula
Gravitation Class 9 Notes Science Chapter 9
Wm = weight of an object on the moon
M= Mass of the moon = 7.36 x 1022
Rm = radius of the moon = 1.74 x 106
G = 6.67 x 10-11 Nm2/kg2
Gravitation Class 9 Notes Science Chapter 9
Wm = 1.474 × 1010 G × m
and We = 1.474 × 1011 G × m
Gravitation Class 9 Notes Science Chapter 9
∴ The weight of an object on the moon = (1/6) th the weight of an object on the earth.

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Thrust

It is the net force applied in a particular direction. Its S.I. unit is N.

Pressure

  • It is the force per unit area.
  • Pressure = thrust / area , S.I unit = N/m2   = Pascal (pa) 
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Pressure in fluids 

  • All liquids and gases are fluids, as they can flow.
  • The pressure exerted by a fluid is transmitted in all directions.

Buoyancy 

  • The upward force exerted by water (fluid) on the body is known as upthrust or buoyancy.
  • The magnitude of the buoyant force depends on the density of the fluid.
    Gravitation Class 9 Notes Science Chapter 9A − Wooden block
    B1 − Beaker with tap water
    B2 − Beaker with salty water
    The buoyant force exerted in B2 is more as compared to B1. This is because the density of B2 water is higher.
    The object may float, sink or remain half submerged and half above water, the density of the fluid and object decides this.
    • If the density of an object is less than the fluid, then it will float on the liquid.
    • If the density of an object is more than the fluid, then it will sink in the liquid.
    • If the density of an object is the same as the density of fluid, then it will half float and half sink.
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Archimedes’ Principle

When a body is immersed fully or partially in a fluid, it experiences an upward force that is equal to the weight of the fluid displaced by it.

Its applications are: 

(i) Used in designing ships and submarines,
(ii) In lactometers to find the purity of milk.
(iii) In hydrometer to determine the density of the liquid.

Relative Density

  • Relative density = density of substance/density of water
  • It has no unit.
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FAQs on Gravitation Class 9 Notes Science Chapter 9

1. What is the law of universal gravitation?
Ans. The law of universal gravitation, formulated by Sir Isaac Newton, states that every particle in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. This can be mathematically expressed as \( F = G \frac{m_1 m_2}{r^2} \), where \( F \) is the gravitational force, \( G \) is the gravitational constant, \( m_1 \) and \( m_2 \) are the masses of the two objects, and \( r \) is the distance between their centers.
2. How does gravity affect the motion of planets?
Ans. Gravity is the force that keeps planets in orbit around stars, such as the Earth around the Sun. The gravitational pull from the Sun provides the necessary centripetal force that keeps the planets in their elliptical orbits. According to Kepler's laws of planetary motion, the gravity of the Sun causes planets to move faster when they are closer and slower when they are farther away, maintaining a consistent orbital path.
3. What is gravitational potential energy?
Ans. Gravitational potential energy is the energy an object possesses due to its position in a gravitational field. It is calculated using the formula \( U = mgh \), where \( U \) is the gravitational potential energy, \( m \) is the mass of the object, \( g \) is the acceleration due to gravity, and \( h \) is the height of the object above a reference point. This energy is converted into kinetic energy as the object falls.
4. What role does gravity play in the formation of stars and galaxies?
Ans. Gravity plays a crucial role in the formation of stars and galaxies by causing gas and dust in space to clump together. As regions of higher density form, the gravitational pull increases, attracting more material. This process continues until the core temperature and pressure are sufficient for nuclear fusion to begin, leading to the birth of a star. Over time, the gravitational interactions between stars can lead to the formation of galaxies.
5. How does gravity vary with altitude?
Ans. Gravity decreases with altitude, meaning that as you go further away from the Earth's surface, the force of gravity becomes weaker. This is due to the inverse square law, where gravitational force diminishes as the distance from the center of the Earth increases. Although this change is small at typical altitudes, it can be measured with precise instruments and is significant for satellites and space missions.
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