Gravitation class 9 Notes, Solved Numerical and Work sheet PDF
Gravitation class 9 Notes, Solved Numerical and Work sheet PDF
Introduction:
What
is Gravitation?
•
Gravitation is a natural phenomenon by
which every object in the universe attracts every other object.
•
This attractive force is called the gravitational
force.
•
It acts along the line joining the centers of
the two objects.
Key Points
1.
Gravitation is a universal force – it
acts between any two objects, whether big or small, near or far.
–
Example:
•
Earth attracts an apple (falls down).
•
Earth and Moon attract each other (causing Moon’s
revolution around Earth).
•
Planets revolve around the Sun due to
gravitation.
2.
Gravitation is always an attractive force,
never repulsive.
3.
The force of gravitation depends on:
–
The masses of the objects (heavier
objects exert more force).
–
The distance between the objects
(force decreases as distance increases).
Universal Law of Gravitation:
Introduction
In 1687, Sir Isaac
Newton proposed the Universal Law of Gravitation. He stated that every object
in the universe attracts every other object with a force.
This force:
- Is directly proportional to the product of their masses
- Is inversely proportional to the square of the distance between their centers
Statement of the Law
“Every
particle of matter in the universe attracts every other particle with a force
which is directly proportional to the product of their masses and inversely
proportional to the square of the distance between them.”
F = G (m1 m2) / r²
Where,
F = Gravitational Force
m1 = Mass of First object
m2 = Mass of another object
r = Distance between two objects
G = Universal Gravitational Constant
Value of Universal Gravitational Constant (G):
Experimental Determination of G
The value of G was first calculated by Henry
Cavendish in 1798 using the torsion balance experiment.
- A horizontal rod with two small lead spheres was suspended.
- Two large lead spheres were placed nearby.
- The gravitational attraction between the large and small spheres caused a
twist in the rod.
- By measuring this twist, Cavendish calculated the value of G.
- G = 6.67 × 10⁻¹¹ Nm²/kg²
- It is called universal because it is the same everywhere in the universe.
Examples in Daily Life:
•
Falling
of fruits, raindrops, and objects towards the Earth.
•
Existence
of atmosphere around Earth.
•
Tides
in seas and oceans (caused by gravitational pull of Moon and Sun).
•
Planets
revolving around the Sun.
Important Points
1. Gravitational
force is a central force (acts along the line joining centers).
2. It is an
attractive force.
3. It exists
between all objects, but it is noticeable only when at least one mass is very
large (like Earth, Sun).
4. This law
explains why planets revolve around the Sun and why objects fall on Earth.
Solved Numericals
Numerical 1
Find the
gravitational force between two objects of masses 10 kg and 20 kg kept 5 m
apart.
Solution:
F = G (m₁ m₂) / r²
F = (6.67 × 10⁻¹¹) × (10 × 20) / 5²
F = 6.67 × 10⁻¹¹ × 200 / 25
F = 6.67 × 10⁻¹¹ × 8
F = 5.336 × 10⁻¹⁰ N
The gravitational force is 5.34 × 10⁻¹⁰ N (very small).
Numerical 2
Two objects, each
of mass 1000 kg, are separated by 1 m. Find the force of attraction between
them.
Solution:
F = G (m₁ m₂) / r²
F = (6.67 × 10⁻¹¹) × (1000 × 1000) / 1²
F = 6.67 × 10⁻¹¹ × 10⁶
F = 6.67 × 10⁻⁵ N
The force is 6.67 × 10⁻⁵ N (still very small).
Numerical 3 (Earth’s Attraction)
Find the
gravitational force between the Earth (mass 6 × 10²⁴ kg) and a body of mass 10 kg placed on the Earth’s surface. Radius of
Earth R = 6.4 × 10⁶ m.
Solution:
F = G (m₁ m₂) / r²
F = (6.67 × 10⁻¹¹) × (6 × 10²⁴ × 10)
/ (6.4 × 10⁶)²
F = (6.67 × 10⁻¹¹) × (6 × 10²⁵) /
4.096 × 10¹³
F = (6.67 × 10⁻¹¹) × (1.465 × 10¹²)
F ≈ 98 N
The force is 98 N, which is equal to the weight of the object.
Free Fall:
Introduction
- When an object falls towards the Earth only under the influence of Earth’s gravitational force, it is said to be in free fall.
- No other forces (like air resistance or push) act on it.
- All objects, whether heavy or light, fall at the same rate in vacuum.
Definition of Free Fall
Free fall is the
motion of a body where gravity is the only force acting on it.
Examples:
- An apple falling from a tree (ignoring air resistance).
- A stone dropped from the top of a building.
- A satellite orbiting the Earth is also in free fall.
Acceleration due to Gravity (g):
During free fall,
objects accelerate towards the Earth with an acceleration called acceleration
due to gravity (g).
Formula: g = GM / R²
Where:
G = 6.67 × 10⁻¹¹ Nm²/kg² (gravitational constant)
M = 6 × 10²⁴ kg (mass of Earth)
R = 6.4 × 10⁶ m
(radius of Earth)
g ≈ 9.8 m/s²
This means the velocity of a freely falling body increases by 9.8 m/s every
second.
Equations of Motion in Free Fall
The same equations
of motion apply, but acceleration a is replaced with g:
1) v = u + gt (Final velocity after time t)
2) s = ut +
½gt² (Distance travelled in time t)
3) v² - u² =
2gs (Relation between velocity and
distance)
Important Points
1. In the absence of
air, all objects fall with the same acceleration (g).
2. On Earth’s
surface, g ≈ 9.8 m/s².
3. The value of g
decreases with height and depth.
4. Weight of a body
in free fall becomes zero (apparent weightlessness).
Differentiate between G and g :
|
Aspect |
G (Gravitational Constant) |
g (Acceleration due to gravity) |
|
Definition |
G is the universal constant of gravitation
that appears in Newton’s law of gravitation. |
G is the acceleration produced in a body
when it falls freely under Earth’s gravity. |
|
Formula |
F = Gm1m2 / r2 |
g = GM / R2 |
|
Meaning |
It gives the strength of gravitational force
between two bodies. |
It tells how fast objects accelerate
towards Earth (or any planet) |
|
Value |
6.67 x 10-11 Nm2/kg2 |
On Earth = 9.8 m/s2 (varies
slightly with location) |
|
Depends
on |
Nothing – It is universal, same everywhere. |
Depends on mass (M) and radius (R) of the
planet. |
|
Nature |
Constant |
Variable (changes from planet to planet,
also with height and depth) |
|
SI
Unit |
Nm2/kg2 |
m/s2 |
Solved Numericals
Numerical 1
A ball is dropped
from a height of 20 m. Find the time taken to reach the ground. (Take g = 10
m/s²)
Solution:
s = ½gt²
20 = ½ × 10 × t²
20 = 5t²
t² = 4 → t = 2 s
Time taken = 2 seconds.
Numerical 2
A stone is thrown
vertically downward with velocity 5 m/s from a height of 50 m. Find the time
taken to reach the ground. (g = 10 m/s²)
Solution:
s = ut + ½gt²
50 = 5t + ½(10)t²
50 = 5t + 5t²
5t² + 5t - 50 = 0
t² + t - 10 = 0
t = (-1 + √41)/2 ≈ 2.7 s
Time taken = 2.7 seconds.
Numerical 3
A body falls freely
from rest. Find its velocity after 3 s.
Solution:
v = u + gt
v = 0 + 9.8 × 3 = 29.4 m/s
Final velocity = 29.4 m/s.
Mass and Weight:
Mass:
- Mass is the
amount of matter contained in a body.
- It is constant everywhere in the universe.
- SI Unit: kilogram (kg).
- Mass is a scalar quantity.
Weight:
- Weight is the
force with which Earth (or any planet) attracts a body.
- Formula: W = m × g
where m = mass of body (kg), g =
acceleration due to gravity (9.8 m/s² on Earth).
- Weight is a vector quantity.
- Weight varies from place to place because g is different on Earth, Moon, or
other planets.
Differentiate
between Mass and Weight:
|
Aspect |
Mass |
Weight |
|
Definition |
Mass is the amount of matter contained in a
body. |
Weight is the force with which a body is
attracted towards the center of the Earth (or any planet) due to gravity. |
|
Formula |
m = W/g |
W = m x g |
|
Nature |
Scalar quantity (only magnitude) |
Vector quantity (magnitude + direction) |
|
SI
unit |
Kilogram (kg) |
Newton (N) |
|
Constant
or Variable |
Constant everywhere in the universe. |
Varies with the value of g (gravity) |
|
Measuring
Device |
Measured by a beam balance or electronic
balance. |
Measured by a spring balance (or weighing
machine) |
|
Effect
of Location |
Same on Earth, Moon, or in space. |
Changes from Earth to Moon (Moon weight =
1/6th of Earth weight) |
|
Example |
A body has 10 kg mass everywhere. |
The same body has a weight of 98 N on Earth
but only 16.3 N on Moon |
Solved Numerical 1:
Q: A stone has a
mass of 5 kg. Find its weight on Earth (take g = 9.8 m/s²).
Solution:
W = m × g = 5 × 9.8
= 49 N
Mass of stone = 5 kg (same everywhere).
Weight of stone on Earth = 49 N.
Weight of an Object on the Surface of Moon:
- The Moon’s
gravity is 1/6th of Earth’s gravity.
gmoon
= (1/6) gearth
- So,
Wmoon = (1/6) Wearth
Solved Numerical 2: Weight on Moon
Q: A boy has a mass
of 60 kg.
(i) Find his weight on Earth.
(ii) Find his weight on Moon. (Take g = 9.8 m/s²).
Solution:
(i) On Earth: Wearth = m × g = 60 × 9.8 = 588 N
(ii) On Moon: Wmoon = (1/6) × 588 = 98 N
Mass of boy = 60 kg (constant).
Weight on Earth = 588 N.
Weight on Moon = 98 N.
Thrust and Pressure:
Thrust:
- Force acting
perpendicularly on a surface.
- SI Unit: Newton (N).
Pressure:
- Pressure is
thrust per unit area.
- Formula: P = F / A
where F = perpendicular force (N), A =
area (m²).
- SI Unit: Pascal (Pa) = 1 N/m².
- Pressure is inversely proportional to area.
Difference
between Thrust and Pressure:
|
Aspect |
Thrust |
Pressure |
|
Definition |
Thrust is the force acting perpendicularly
on a surface. |
Pressure is the thrust (force
perpendicularly) acting per unit area of the surface. |
|
Formula |
F = P x A |
P = F/A |
|
Nature |
Vector quantity (has magnitude + direction) |
Scalar quantity (only magnitude) |
|
SI
unit |
Newton (N) |
Pascal (Pa) = N/m2 |
|
Depends
on |
Only on the force applied. |
Depends on both force applied and the area
of contact. |
|
Effect
of Area |
Independent of area. |
Inversely proportional to area. |
|
Example |
The total force a girl exerts on the ground
while standing is thrust. |
The force per unit area exerted by the girl’s
shoes on the ground is pressure. |
Solved Numerical 3: Thrust and Pressure
Q: A girl weighing
300 N stands on the ground wearing shoes. Each shoe has an area of 200 cm² in
contact with the ground. Find the pressure exerted on the ground.
Solution:
Total area = 2 × 200 = 400 cm² = 0.04 m²
Force = 300 N
Pressure = F / A = 300 / 0.04 = 7500 Pa
Pressure on ground = 7500 Pascal.
Solved Numerical 4: Effect of Area on
Pressure
Q: A sharp knife
has a blade area of 0.5 cm², while a blunt knife has a blade area of 10 cm². If
a force of 50 N is applied on both, calculate the pressure exerted in each
case.
Solution:
Sharp knife: A = 0.5 cm² = 5 × 10⁻⁵ m²
P = 50 / (5 × 10⁻⁵) = 1 × 10⁶ Pa
Blunt knife: A = 10 cm² = 1 × 10⁻³ m²
P = 50 / (10⁻³) = 5 × 10⁴ Pa
Pressure with sharp knife = 1,000,000 Pa
Pressure with blunt knife = 50,000 Pa
This is why sharp knives cut better!
Buoyancy (Upthrust):
- When an object is immersed in a fluid (liquid or gas), the fluid exerts an upward force on it. This upward force is called Buoyant Force or Upthrust.
- It arises because fluid pressure increases with depth, so the bottom of the object experiences more pressure than the top.
- Formula , Fb = ρ × V × g
Numerical
-1:Buoyancy
A wooden block of
volume 0.02 m³ is fully immersed in water. Find the buoyant force on it
(density of water = 1000 kg/m³, g = 9.8 m/s²).
Solution:
Fb = ρ × V × g
= 1000 × 0.02 × 9.8
Fb = 196 N
Factors affecting on buoyant force:
- Volume of fluid displaced
- Density of fluid
- Acceleration due to gravity (g)
Why Objects Sink or Float?
Numerical 2: Sink or Float
Solution:
Mass = 7800 × 0.001
= 7.8 kg
Weight (W) = 7.8 ×
9.8 = 76.44 N
Buoyant force (Fb) = 1000 × 0.001 × 9.8 = 9.8 N
Since W > Fb, the cube sinks.
Answer: Cube sinks
Archimedes’ Principle:
Archimedes’
Principle states: "When a body is immersed fully or partially in
a fluid, it experiences an upward force (upthrust) equal to the weight of the
fluid displaced by it".
- Formula, Fb = Weight of displaced fluid
Applications:
- Designing ships and submarines
- Hydrometer
- Explaining floating of bodies
Numerical 3: Archimedes’ Principle
An object of weight
50 N is immersed in water. It displaces water of weight 20 N.
Find (i) upthrust,
(ii) apparent weight.
Solution:
Upthrust = 20 N
Apparent weight = 50 - 20 = 30 N
Relative Density (R.D.)
- Relative density is the ratio of the density of a substance to the density of water.
- Formula, R.D. = ρsubstance
/ ρwater
Key points:
- It has no unit (ratio)
- RD > 1 → sinks in water
- RD < 1 → floats in water
Numerical 4: Relative Density
A solid weighs 200 g in air and 150 g in water. Find its relative density.
Solution:
Loss of weight =
200 - 150 = 50 g = weight of displaced water
RD = Wair / (Wair – Wwater)
= 200 / 50
RD = 4
Practice Numerical
1)
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 = 9.8 m/s2
(Answer: u = 98.99 m/s and 20.20 sec)
2)
With what speed must
an object be thrown vertically upwards to reach a height of 125 m? (Take g
= 10 m/s2) (Answer: 50 m/s )
3)
An object is thrown
vertically upward to a height of 10 m. calculate its,
4)
A stone is thrown
vertically upwards with an initial velocity of 30 m/s. The time taken for the
stone to rise to its maximum height is (Take g = 10 m/s2) (Answer
: 3sec)
5)
What will be weight of
object on the moon if its weight on Earth is 120 N? (Answer : 20 N )
7)
A block of wood is
kept on a table top. The mass of the wooden block is 5 kg and its dimension are
40 cm × 20 cm × 10 cm. Find the pressure exerted by the wooden block on the
table top if it is made to lie on the table with its sides of dimensions,
(a) 20 cm ×
10 cm (Answer: 2450 Pa)
(b)
40 cm × 20 cm. (Answer: 612.5 Pa)
(Given
g = 9.8 m/s2)
8)
How much force should
be applied on an area of 1 cm2 to get a pressure of 15 Pa? (Answer:
1.5 x 10-3 N)
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