Physics Class 9 Chapter 1 Motion Full Chapter Book Lakhmir Singh and Manjit kaur with book Image
Chapter motion
WHAT IS MOTION
Motion, in physics, change with time of the position or orientation of a body.
Motion along a line or a curve is called translation. Motion that changes
the orientation of a body is called rotation. In both cases all points in
the body have the same velocity (directed speed) and the same acceleration
(time rate of change of velocity). The most general kind of motion combines
both translation and rotation.
हिंदी में
⇩
गति, भौतिकी में, शरीर की स्थिति या अभिविन्यास के समय के साथ बदलती है। किसी रेखा या वक्र के अनुदिश गति को अनुवाद कहते हैं। वह गति जो किसी पिंड के उन्मुखीकरण को बदल देती है, घूर्णन कहलाती है। दोनों ही मामलों में शरीर के सभी बिंदुओं का वेग (निर्देशित गति) और समान त्वरण (वेग के परिवर्तन की समय दर) समान होता है। सबसे सामान्य प्रकार की गति अनुवाद और रोटेशन दोनों को जोड़ती है।
Distance And
Displacement
Distance
and displacement are two quantities that seem to mean the same but are
distinctly different with different meanings and definitions. Distance is the
measure of “how much ground an object has covered during its motion” while
displacement refers to the measure of “how far out of place is an object.” In
this article, let us understand the difference between distance and
displacement.
What is Distance?
Distance
is the total movement of an object without any regard to direction. We can
define distance as to how much ground an object has covered despite its
starting or ending point.
Let’s
understand the concept of distance with the help of the following diagram:
Explanation
of distance
Distance
here will be = 4m + 3m + 5m = 12 m
Distance Formula
Δd=d1+d2
How is Displacement defined?
Displacement is
defined as the change in position of an object. It is a vector quantity and has
a direction and magnitude. It is represented as an arrow that points from the
starting position to the final position. For example- If an object moves from A
position to B, then the object’s position changes. This change in position of an
object is known as Displacement.
Displacement = Δx=xf−x0
xf
= Final Position
x0
= Initial Position
Δx
= Displacement
Examples of Distance and
Displacement
Question 1. John travels 250 miles to North but then back-tracks to
South for 105 miles to pick up a friend. What is John’s total displacement?
Answer: John’s starting position Xi= 0.
Her final position Xf is the distance travelled N minus the distance
South.
Calculating displacement, i.e.D.
D = ΔX = (Xf – Xi)
D = (250 mi N – 105 mi S) – 0
D = 145 mi N
Question 2. An object moves along the grid through points A, B, C,
D, E, and F as shown below. The side of square tiles measures 0.5 km.
a) Calculate the distance covered by the moving object.
b) Find the magnitude of the displacement of the object.
Solution:
a) The distance covered by the moving object is calculated as follows:
AB + BC + CD + DE + EF
3 + 1 + 1.5 + 0.5 + 0.5 = 6.5 km
The distance covered by the moving object is 6.5 km.
b) The initial point is A and the final point is F, hence the magnitude
of the displacement is equal to the distance AF which is calculated by applying
Pythagoras’s theorem to the triangle AHF as shown in the figure below
Applying the Pythagorean formula, we get
AF2=AH2+HF2
Substituting the formula, we get
AF2=(0.5×4)2+(0.5×3)2=6.25 AF=√6.25km=2.5km
The magnitude of displacement is 2.5 km.
Distance vs Displacement
|
Distance |
Displacement |
|
The complete length of the path
between any two points is called distance |
Displacement is the direct
length between any two points when measured along the minimum path between
them |
|
Distance is a scalar quantity
as it only depends upon the magnitude and not the direction |
Displacement is a vector
quantity as it depends upon both magnitude and direction |
|
Distance can only have positive
values |
Displacement can be positive,
negative and even zero |
The difference between scalar and vector quantities
Scalar and vector quantities
A quantity that has magnitude but no particular direction is described as scalar. A quantity that has magnitude and acts in a particular direction is described as vector.
Scalar quantities
Scalar quantities only have magnitude (size).
For example, 11 m and 15 ms-1 are both scalar quantities.
Scalar quantities include:
- distance ⇨ दूरी
- speed ⇨ स्पीड
- time ⇨ समय
- power ⇨ शक्ति
- energy ⇨ ऊर्जा
Scalar quantities change when their magnitude changes.
Vector quantities
Vector quantities have both magnitude and direction. For example, 11 m east and 15 ms-1 at 30° to the horizontal are both vector quantities.
Vector qualities include:
- displacement ⇨ विस्थापन
- velocity ⇨ वेग
- acceleration ⇨ त्वरण
- force ⇨ बल
- weight ⇨ वजन
- momentum ⇨ गति
Vector quantities change when:
- their magnitude changes
- their direction changes
- their magnitude and direction both change
The difference between scalar and vector quantities is an important one.
Speed is a scalar quantity – it is the rate of change in the distance travelled by an object, while velocity is a vector quantity – it is the speed of an object in a particular direction.
Example
A geostationary satellite is in orbit above Earth. It moves at constant speed but its velocity is constantly changing (since its direction is always changing).
- the difference in two vectors quantities = final vector - initial vector
- the difference in two scalar quantities = large value - small value
Uniform Motion
and Non-Uniform Motion
Uniform Motion:
This type of motion is defined as the motion
of an object in which the object travels in a straight line and its velocity
remains constant along that line as it covers equal distances in equal
intervals of time, irrespective of the duration of the time.
If a body
is involved in rectilinear motion and the motion is consistent, then the
acceleration of the body must be zero.
Example of Uniform Motion:
- If the speed of a car is 10
m/s, it means that the car covers 10 meters in one second. The speed is
constant in every second.
- Movement of blades of a
ceiling fan.
Non Uniform Motion:
This type
of motion is defined as the motion of an object in which the object travels
with varied speed and it does not cover same distance in equal time intervals,
irrespective of the time interval duration.
Example of Non Uniform Motion:
- If a car covers 10 meters in
first two seconds, and 15 meters in next two seconds.
- The motion of a train.
Now,
people usually get confused between uniform motion and uniform acceleration. In
the later phenomena, the object is having a constant acceleration in
rectilinear motion, which means the object has different speed in every second,
which clearly defines that motion is changing.
Difference Between
these two types of motions:
|
Comparison Parameters |
Uniform Motion |
Non Uniform Motion |
|
Average
Speed |
The
motion is similar to the actual speed of the object. |
The motion
is different from the actual speed of the object. |
|
Rectilinear
Motion |
It has
zero acceleration. |
It has
non-zero acceleration. |
|
Graph |
Distance-time
graph shows a straight line |
Distance-time
graph shows a curved line |
|
Distance |
Covers
equal distances in equal time interval. |
Covers
unequal distances in equal time interval. |
What is Speed?
Speed
Speed is
defined as
The rate
of change of position of an object in any direction.
Speed is
measured as the ratio of distance to the time in which the distance was covered. Speed is a scalar quantity as it has only direction and no
magnitude.
Speed Formula
The
formula of speed is given in the table below:
Speed =
Distance/Time
|
s=dt |
Where,
- s is the speed in m.s-1
- d is the distance traveled
in m
- t is the time taken in s
Speed Unit
Following
are the units of speed are:
|
SI system |
ms-1 |
|
(2) (3) (4) (5) |
|
|
|
|
What is Velocity?
The
meaning of velocity of an object can be defined as the rate of change of the
object’s position with respect to a frame of reference and time. It might sound
complicated but velocity is basically speeding in a specific direction. It is a
vector quantity, which means we need both magnitude (speed) and direction to
define velocity. The SI unit of it is meter per second (ms-1). If
there is a change in magnitude or the direction in the velocity of a body the
body is said to be accelerating.
Velocity Formula
The
formula of velocity is given in the table below:
Velocity
= Displacmant/Time
|
v=dt |
Where,
- v is the Velocity in m.s-1
- d is the displacement
traveled in m
- t is the time taken in s
Initial and Final Velocity
Initial
velocity describes how fast an object travels when gravity first applies force
on the object. On the other hand, the final velocity is a vector quantity that
measures the speed and direction of a moving body after it has reached its
maximum acceleration.
How to find the final velocity?
Finding
the final velocity is simple with a few calculations and basic conceptual
knowledge.
- Determine the object’s
original velocity by dividing the time it took for the object to travel a
given distance by the total distance. In the equation V = d/t, V is the
velocity, d is the distance and t is the time.
- Determine the object’s
acceleration by dividing the object’s mass by the force and multiply the
answer by the time it took for it to accelerate. For example, if the
object weighs 30 kg and has a force of 15 N applied to it, then the
acceleration would be 4 m/s.
- Add the quantity obtained
from Step 1 and Step 2 to obtain the final velocity. For example, if your
initial velocity was 3 m/s and your object acceleration is 4 m/s, your
final velocity is 7 m/s (3 + 4 = 7).
Constant Velocity
The
motion with constant velocity is the simplest form of motion. We witness
constant motion whenever an object slides over a horizontal, low friction
surface (when a puck slides over a hockey rink.)
The above graph is a graph of
displacement versus time for a body moving with constant velocity. The straight
line in the graph can be algebraically represented as follows:
x=x0+vt In the equation, x0 is the displacement at time t, v is the
constant velocity of the body v=dxdt
Velocity Units
The SI
unit of velocity is m/s (m⋅s−1). Other units and dimensions of
velocity are given in the table below.
|
Unit
of velocity |
|||
|
Common
symbols |
v, v, →v |
||
|
SI unit
|
m/s |
||
|
Other
units |
mph,
ft/s |
||
|
Dimension |
LT−1 |
||
Difference between Speed and Velocity
The
detailed comparison in the tabular format is given below.
|
Velocity
VS Speed |
|
|
SPEED |
VELOCITY |
|
Speed is the quantitative
measure of how quickly something is moving. |
Velocity defines the direction
of the movement of the body or the object. |
|
Speed is primarily a scalar
quantity |
Velocity is essentially a
vector quantity |
|
It is the rate of change of distance |
It is the rate of change of
displacement |
|
Speed of an object moving can
never be negative |
The velocity of a moving object
can be zero. |
|
Speed is a prime indicator of
the rapidity of the object. |
Velocity is the prime indicator
of the position as well as the rapidity of the object. |
|
It can be defined as the
distance covered by an object in unit time. |
Velocity can be defined as the
displacement of the object in unit time. |
What is
Acceleration ?
Acceleration
is defined as
The rate
of change of velocity with respect to time.
Acceleration
is a Vector quantity as it has both magnitude and direction. It is also the
second derivative of position with respect to time or it is the first
derivative of velocity with respect to time.
What is Acceleration Formula?
Acceleration
formula is given as:
Acceleration = (finalvelocity)−(initialvelocity)
time acceleration = changeinvelocitytime a=vf−vit
|
a=Δvt |
Where,
- a is the acceleration in m.s-2
- vf is the
final velocity in m.s-1
- vi is the initial
velocity in m.s-1
- t is the time interval in s
- Δv is the small change in
the velocity in m.s-1
What is the Unit of Acceleration?
The SI
Unit of acceleration is given as:
|
SI unit |
m/s2 |
Uniform and
Non-uniform acceleration
So can we
have a situation when speed remains constant but the body is accelerated?
Actually, it is possible in circular where speed remains constant but since the
direction is changing hence the velocity changes, and the body is said to be
accelerated.
Average
acceleration
The
average acceleration over a period of time is defined as the total change in
velocity in the given interval divided by the total time taken for the change.
For a given interval of time, it is denoted as ā.
Where v2
and v1 are the instantaneous velocities at time t2
and t1 and ā is the average acceleration.
What is Instantaneous Acceleration?
Instantaneous
acceleration is defined as
The ratio
of change in velocity during a given time interval such that the time interval
goes to zero.
What is the difference between Acceleration and
Velocity?
Following
is the table of acceleration vs velocity:
|
Parameter |
Acceleration |
Velocity |
|
Definition |
Acceleration is defined as the
change in the velocity of an object with respect to time |
Velocity is defined as the
speed of an object in a particular direction |
|
Formula |
Velocity/Time |
Displacement/Time |
|
Unit |
m.s-2 |
m.s-1 |
EQUATION
OF UNIFORMLY ACCELERATED MOTION
(1) First Equation of Motion
Motion and Rest
If the position of an object changes with respect to a reference point
then it is said to be in motion wrt.that reference while if it does not changes
then it is at rest wrt.that reference point. For the better understanding or to
deal with the different situations of rest and motion we derive some standard
equation relating terms distance,displacement,speed,velocity and acceleration
of the body by the equation called as equations of motion.
Three Equations of Motion
In case of motion with uniform or constant acceleration (one with equal
change in velocity in equal interval of time) we derive three standard
equations of motion which are also known as the laws of constant acceleration.
These equations contain quantities displacement(s), velocity (initial and
final), time(t) and acceleration(a) that governs the motion of a particle.
These equations can only be applied when acceleration of a body is constant and
motion is a straight line. The three equations are,
- v =
u + at
- v² =
u² + 2as
- s =
ut + ½at²
where, s = displacement; u = initial velocity; v = final velocity; a =
acceleration; t = time of motion.
Numerical
Derivation of Equation of Motions
Now let's start the derivation with the first equation of motion i.e.
v=u+at where u is the initial velocity, v is the final velocity and a is the
constant acceleration.
Assuming that a body started with initial velocity “u” and after time t
it acquires final velocity v due to uniform acceleration a.
We know acceleration is defined as the rate of change of velocity, also
which is given by slope of the velocity time graph.
Thus both from definition as well as graph Acceleration = Change
in velocity/Time Taken i.e. a = v-u /t or at = v-u
Therefore, we have: v = u + at
Now to derive the second equation again suppose a body is moving with
initial velocity u after time t its velocity becomes v. The displacement
covered by the during this interval of time is S and the acceleration of the
body is represented by a.
Explanation: We know area under velocity time graph gives total
displacement of the body thus area under velocity time graph is area of
trapezium OABC.
Also area of trapezium = ½(sum of parallel sides)height
Sum of parallel sides=OA+BC=u+v and here,height=time interval t
Thus,area of trapezium = ½(u+v)t
Substituting v=u+at from first equation of motion we get,
Displacement =S =area of trapezium = ½(u+u+at)t
S = ½(2u+at)t=ut+½at2
Which is called the second equation of motion and is the relation
between displacement S,initial velocity u,time interval t and acceleration a of
the particle.
Now in order to derive the third equation again use
Displacement =S =area of trapezium = ½(u+v)t
From first equation v=u+at we get v-u=at ⇒v-u/a=t
Substituting the value of t in S = ½(u+v)t
We get S=½(u+v)(v-u)/a=(v2-u2)/2a
⇒2as=v2-u2
⇒v2 =u2+2as
Which is the third equation of motion and is the relation between final
velocity v,initial velocity u,constant acceleration a and displacement S of the
particle.
We can now also calculate the displacement of particles during the nth
second, using these equations of motion derived above. In order to do so we
will calculate the displacement covered in n seconds and subtract the
displacement covered in n-1 seconds and to get the displacement in nth second
snth =Sn-sn-1=un-u(n-1) + 1/2an2-1/2a(n-1)2
simplifying gives us final equation for displacement in the nth second
is s = u + a(2n-1)/2
This equation is often regarded as modified form of second equation of motion
What is Uniform Circular Motion?
The movement of a body following a circular path is called a circular
motion. Now, the motion of a body moving with constant speed along a circular
path is called Uniform Circular Motion. Here, the speed is constant but the
velocity changes.
If a
particle is moving in a circle, it must have some acceleration acting towards
the centre which is making it move around the centre. Since this acceleration
is perpendicular to the velocity of a particle at every instant, it is only
changing the direction of velocity and not magnitude and that’s why the motion
is uniform circular motion. We call this acceleration centripetal acceleration (or radial acceleration),
and the force acting towards the centre is called centripetal force.
In the
case of uniform circular motion, the acceleration is:
ar = v2r
= ω2r
If the
mass of the particle is m, we can say from the second law of motion that:
F = ma
mv2r=
mω2r
This is
not a special force, actually force like tension or friction may be a cause of
origination of centripetal force. When the vehicles turn on the
roads, it is the frictional force between tyres and ground that provides the
required centripetal force for turning.
NOTE
So if a
particle is moving in a uniform circular motion:
1) Its
speed is constant
2)
Velocity is changing at every instant
3) There
is no tangential acceleration
4) Radial
(centripetal) acceleration = ω2r
5) v=ωr
In case of non-uniform circular motion, there is some tangential acceleration due to which the speed of the particle increases or decreases. The resultant acceleration is the vector sum of radial acceleration and tangential acceleration.
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