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Prof. Mukesh N. Tekwani
   Department of Physics
       I. Y. College,
           Mumbai
mukeshtekwani@outlook.com
       © Prof. Mukesh N Tekwani, 2011   1
Circular Motion




   © Prof. Mukesh N Tekwani, 2011   2
Why study Circular Motion?
• To understand
  – Motion of planets
  – Motion of electrons around the nucleus
  – Motion of giant wheel
  – Motion of space stations
  – Motion of moon and satellites




                  © Prof. Mukesh N Tekwani, 2011   3
Circular Motion
• It is defined as the motion of a particle along a
  complete circle or part of a circle.
• Fore circular motion, it is NOT necessary that
  the body should complete a full circle.
• Even motion along arc of a circle is circular
  motion



                   © Prof. Mukesh N Tekwani, 2011   4
Circular Motion
How do we locate something on a circle?
Give its angular position θ

    y


         f
                                     What is the location of
               i
                   X                 900 or π/2
                   θ=0




                   © Prof. Mukesh N Tekwani, 2011              5
Circular Motion
              y


                     f
                                      is the angular position.

                          i       Angular displacement:
                              x                 f    i




Note: angles measured Clockwise (CW) are negative and
angles measured (CCW) are positive.    is measured in
radians.
              2 radians = 360Tekwani, 1 revolution
                     © Prof. Mukesh N
                                      = 2011                     6
Angular Displacement
• Angular displacement is defined as the angle
  described by the radius vector
                                     Initial position of particle is   a
                                     Final position of particle is     b
                                     Angular displacement in time t is     Θ
                  a



                 © Prof. Mukesh N Tekwani, 2011                                7
Angular Displacement



                        S =r Θ



     © Prof. Mukesh N Tekwani, 2011   8
arclength = s = r
y

                                               s
        f
    r                                          r
               i
                                  is a ratio of two lengths;
                     x       it is a dimensionless ratio!
                             This is a radian measure of
                             angle
                             If we go all the way round s
                             =2πr and Δθ =2 π
            © Prof. Mukesh N Tekwani, 2011                9
Right Hand Rule
If the fingers of the
right hand are curled
in the direction of
revolution of the
particle, then the
outstretched thumb
gives the direction of
the angular
displacement vector.

                   © Prof. Mukesh N Tekwani, 2011   11
Stop & Think – Pg 2
Are the following motions same or different?
1. The motion of the tip of second hand of a
   clock.
2. The motion of the entire second hand of a
   clock.

The motion of the tip of second hand of a clock
   is uniform circular motion.
The motion of the entire second hand is a
   rotational motion.
                  © Prof. Mukesh N Tekwani, 2011   12
Centripetal Force
• UCM is an accelerated motion. Why?
• UCM is accelerated motion because the velocity of
  the body changes at every instant (i.e. every
  moment)
• But, according to Newton’s Second Law, there must
  be a force to produce this acceleration.
• This force is called the centripetal force.
• Therefore, Centripetal force is required for circular
  motion. No centripetal force +> no circular motion.
                     © Prof. Mukesh N Tekwani, 2011   25
Velocity and Speed in UCM
                           Is speed changing?

                           No, speed is constant

                           Is velocity changing?

                           Yes, velocity is changing
                           because velocity is a
                           vector – and direction is
                           changing at every point
        © Prof. Mukesh N Tekwani, 2011                 26
Velocity and Speed in UCM
                           Is speed changing?

                           No, speed is constant

                           Is velocity changing?

                           Yes, velocity is changing
                           because velocity is a
                           vector – and direction is
                           changing at every point
        © Prof. Mukesh N Tekwani, 2011                 27
Examples of Centripetal force
A body tied to a string
and whirled in a
horizontal circle – CPF
is provided by the
tension in the string.




                  © Prof. Mukesh N Tekwani, 2011   28
Examples of Centripetal force
• For a car travelling
  around a circular
  road with uniform
  speed, the CPF is
  provided by the
  force of static
  friction between
  tyres of the car
  and the road.

                   © Prof. Mukesh N Tekwani, 2011   29
Examples of Centripetal force
• In case of electrons revolving around the
  nucleus, the centripetal force is provided by
  the electrostatic force of attraction between
  the nucleus and the electrons

• In case of the motion of moon around the
  earth, the CPF is provided by the ______ force
  between Earth and Moon

                  © Prof. Mukesh N Tekwani, 2011   30
Centripetal Force
• Centripetal force
  – It is the force acting on a particle performing UCM and
    this force is along the radius of the circle and directed
    towards the centre of the circle.

  REMEMBER!
  Centripetal force
     - acting on a particle performing UCM
     - along the radius
     - acting towards the centre of the circle.
                       © Prof. Mukesh N Tekwani, 2011      31
Properties of Centripetal Force
1.   Centripetal force is a real force
2.   CPF is necessary for maintaining UCM.
3.   CPF acts along the radius of the circle
4.   CPF is directed towards center of the circle.
5.   CPF does not do any work
6.   F = mv2/ r



                       © Prof. Mukesh N Tekwani, 2011   32
Radial Acceleration
                                Let P be the position of the particle
Y                               performing UCM
             v
                 P(x, y)        r is the radius vector
N
                                Θ = ωt . This is the angular displacement of
         r                      the particle in time t secs
    y
         θ                      V is the tangential velocity of the particle at
    O        x   M       X      point P.

                                Draw PM ┴ OX

                                The angular displacement of the particle in
                                time t secs is

                                LMOP = Θ = ωt
                 © Prof. Mukesh N Tekwani, 2011                            33
Radial Acceleration
Y
                                The position vector of the particle at
             v                  any time is given by:
                 P(x, y)
                                r = ix + jy
N
         r                      From ∆POM
    y
         θ
                                sin θ = PM/OP
    O        x   M       X
                                ∴ sin θ = y / r

                                ∴y = r sin θ

                                But θ = ωt

                                 ∴ y = r sin ωt
                 © Prof. Mukesh N Tekwani, 2011                      34
Radial Acceleration
Y
                                Similarly,
             v
                                From ∆POM
                 P(x, y)
N
                                cos θ = OM/OP
         r
    y
                                ∴ cos θ = x / r
         θ
    O        x   M       X      ∴ x = r cos θ

                                But θ = ωt

                                 ∴ x = r cos ωt



                 © Prof. Mukesh N Tekwani, 2011   35
Radial Acceleration
The velocity of particle at any instant (any time) is called its
instantaneous velocity.

The instantaneous velocity is given by

v = dr / dt

∴ v = d/dt [ ir cos wt + jr sin wt]

∴ v = - i r w sin wt + j r w cos wt



                          © Prof. Mukesh N Tekwani, 2011           36
Radial Acceleration
The linear acceleration of the particle at any instant (any time) is
called its instantaneous linear acceleration.




                         © Prof. Mukesh N Tekwani, 2011            37
Radial Acceleration
Therefore, the instantaneous linear
acceleration is given by

∴ a = - w2 r                                                 r

                                                         a
Importance of the negative sign:
The negative sign in the above
equation indicates that the linear
acceleration of the particle and the
radius vector are in opposite
directions.


                        © Prof. Mukesh N Tekwani, 2011           38
Relation Between Angular
Acceleration and Linear Acceleration
The acceleration of a particle         ∵ r is a constant radius,
is given by

              ………………. (1)
                                       ∴
But v = r w
                                       But
∴
                                       α is the angular acceleration

∴a =                 .... (2)          ∴ a=rα            ………………………(3)

                        © Prof. Mukesh N Tekwani, 2011                 39
Relation Between Angular
Acceleration and Linear Acceleration
                                          ∴
v=wxr
Differentiating w.r.t. time t,             ∴ linear acceleration
                                          a = a T + aR
                                          aT is called the tangential component of
                                          linear acceleration

                                          aR is called the radial component of
                                          linear acceleration
But                                       For UCM, w = constant, so

and                                       ∴ a = aR
                                          ∴ in UCM, linear accln is centripetal accln
                          © Prof. Mukesh N Tekwani, 2011                            40
Centrifugal Force
1. Centrifugal force is an imaginary force (pseudo force)
   experienced only in non-inertial frames of reference.
2. This force is necessary in order to explain Newton’s laws of
   motion in an accelerated frame of reference.
3. Centrifugal force is acts along the radius but is directed away
   from the centre of the circle.
4. Direction of centrifugal force is always opposite to that of the
   centripetal force.
5. Centrifugal force

6. Centrifugal force is always present in rotating bodies
                          © Prof. Mukesh N Tekwani, 2011              41
Examples of Centrifugal Force
1. When a car in motion takes a sudden turn towards left,
   passengers in the car experience an outward push to the right.
   This is due to the centrifugal force acting on the passengers.

2. The children sitting in a merry-go-round experience an
   outward force as the merry-go-round rotates about the
   vertical axis.


Centripetal and Centrifugal forces DONOT constitute an action-
reaction pair. Centrifugal force is not a real force. For action-
reaction pair, both forces must be real.
                        © Prof. Mukesh N Tekwani, 2011          42
Banking of Roads
1. When a car is moving along a curved road, it is performing
   circular motion. For circular motion it is not necessary that the
   car should complete a full circle; an arc of a circle is also
   treated as a circular path.

2. We know that centripetal force (CPF) is necessary for circular
   motion. If CPF is not present, the car cannot travel along a
   circular path and will instead travel along a tangential path.




                         © Prof. Mukesh N Tekwani, 2011           43
Banking of Roads
3. The centripetal force for circular motion of the car can be
   provided in two ways:
   • Frictional force between the tyres of the car and the road.
   • Banking of Roads




                        © Prof. Mukesh N Tekwani, 2011        44
Friction between Tyres and Road
The centripetal force for circular motion of the car is provided by
the frictional force between the tyres of the car and the road.
Let m = mass of the car
V = speed of the car, and
R = radius of the curved road.

Since centripetal force is provided by the frictional force,
CPF   =   frictional force        (“provide by” means “equal to” )

                   (µ is coefficient of friction between tyres & road)

So                   and
                             © Prof. Mukesh N Tekwani, 2011          45
Friction between Tyres and Road
Thus, the maximum velocity with which a car can safely travel
along a curved road is given by


If the speed of the car increases beyond this value, the car will be
thrown off (skid).
If the car has to move at a higher speed, the frictional force
should be increased. But this cause wear and tear of tyres.
The frictional force is not reliable as it can decrease on wet roads
So we cannot rely on frictional force to provide the centripetal
force for circular motion.
                          © Prof. Mukesh N Tekwani, 2011           46
Friction between Tyres and Road
                             R1 and R2 are reaction forces due
                             to the tyres

                             mg is the weight of the car,
Center of                    acting vertically downwards
 circular
   path
                             F1 and F2 are the frictional forces
                             between the tyres and the road.

                             These frictional forces act
                             towards the centre of the
                             circular path and provide the
                             necessary centripetal force.
                © Prof. Mukesh N Tekwani, 2011                 47
Friction between Tyres and Road




           © Prof. Mukesh N Tekwani, 2011   48
Friction between Tyres and Road –
            Car Skidding




           © Prof. Mukesh N Tekwani, 2011   49
Banked Roads
What is banking of roads?
The process of raising the
outer edge of a road over
the inner edge through a
certain angle is known as
banking of road.




                    © Prof. Mukesh N Tekwani, 2011   50
Banking of Roads
Purpose of Banking of Roads:
Banking of roads is done:
1. To provide the necessary centripetal force for
   circular motion
2. To reduce wear and tear of tyres due to friction
3. To avoid skidding
4. To avoid overturning of vehicles




                    © Prof. Mukesh N Tekwani, 2011    51
Banked Roads




  © Prof. Mukesh N Tekwani, 2011   52
Banked Roads

What is angle of                                              R cos θ
                                                 R
banking?                                              Θ

The angle made by the                  R sin θ
surface of the road with
the horizontal surface is
called as angle of banking.                               Θ
                                                                 Horizontal



                                                      W = mg
                     © Prof. Mukesh N Tekwani, 2011                           53
Banked Roads

Consider a car moving                                     R cos θ
                                             R
along a banked road.                              Θ

                                   R sin θ
Let
m = mass of the car
V = speed of the car                                  Θ

θ is angle of banking

                                                  W = mg
                 © Prof. Mukesh N Tekwani, 2011                     54
Banked Roads

The forces acting on the                                   R cos θ
                                              R
car are:                                           Θ

                                    R sin θ
(i) Its weight mg acting
vertically downwards.
                                                       Θ
(ii) The normal
reaction R acting
perpendicular to the                               W = mg
surface of the road.
                  © Prof. Mukesh N Tekwani, 2011                     55
Banked Roads
The normal reaction can be                                    R cos θ
resolved (broken up) into                        R
                                                      Θ
two components:
                                       R sin θ
1. R cosθ is the vertical
   component
                                                          Θ
2. R sinθ is the horizontal
   component
                                                      W = mg
                     © Prof. Mukesh N Tekwani, 2011                     56
Banked Roads
Since the vehicle has no                                      R cos θ
vertical motion, the weight                      R
                                                      Θ
is balanced by the vertical
component                              R sin θ
R cosθ = mg …………… (1)
                                                          Θ
(weight is balanced by
vertical component means
weight is equal to vertical
component)                                            W = mg
                     © Prof. Mukesh N Tekwani, 2011                     57
Banked Roads
The horizontal component                                     R cos θ
is the unbalanced                R
                                                     Θ
component . This horizontal
component acts towards      R sin θ
the centre of the circular
path.
                                                         Θ
This component provides
the centripetal force for
circular motion
                                                     W = mg
R sinθ =      …………… (2)
                    © Prof. Mukesh N Tekwani, 2011                     58
Banked Roads
Dividing (2) by (1), we get
                                        θ = tan-1      ( )
R sinθ =            mg
                                     Therefore, the angle of banking
R cos θ
                                     is independent of the mass of
                                     the vehicle.

So,                                  The maximum speed with
                                     which the vehicle can safely
tan θ =                              travel along the curved road is


                      © Prof. Mukesh N Tekwani, 2011                   59
Banked Roads
   A car travels at a constant speed
   around two curves. Where is the
   car most likely to skid? Why?


                                        2
                                   mv
                  F = ma
                                    r
      Smaller radius: larger centripetal
      force is required to keep it in
      uniform circular motion.
  © Prof. Mukesh N Tekwani, 2011            60
Maximum Speed of a Vehicle on a
  Banked Road with Friction
                Consider a vehicle moving along a
                curved banked road.

                Let
                m = mass of vehicle
                r = radius of curvature of road
                θ = angle of banking
                F = frictional force between tyres
                and road.
                The forces acting on the vehicle
                are shown in the diagram.
           © Prof. Mukesh N Tekwani, 2011       61
Maximum Speed of a Vehicle on a
        Banked Road with Friction
The forces acting on the vehicle are:
1) Weight of the vehicle mg, acting vertically downwards
2) Normal reaction N acting on vehicle, perpendicular to
   the surface of the road.
3) Friction force between tyres and road.

Forces N and frictional force f are now resolved into two
components



                        © Prof. Mukesh N Tekwani, 2011      62
Maximum Speed of a Vehicle on a
       Banked Road with Friction
Resolving the Normal reaction         The normal reaction N is
                                      resolved into 2 components:

                                      1) N cos θ is vertical
                                         component of N
                                      2) N sin θ is horizontal
                                         component of N




                         © Prof. Mukesh N Tekwani, 2011          63
Maximum Speed of a Vehicle on a
        Banked Road with Friction
Resolving the frictional force
                                       The frictional force f is
                                       resolved into 2 components:

      f cos θ
                                       1) f cos θ is horizontal
                                          component of f
          f
                θ   f sin θ
                                       2) f sin θ is vertical
                                          component of f



                              © Prof. Mukesh N Tekwani, 2011         64
Maximum Speed of a Vehicle on a
                Banked Road with Friction
                                      All forces acting on vehicle

              N                              The vertical component N cos θ is
                            N cos θ
                                             balanced by the weight of the
                        θ                    vehicle and the component f sin θ
              N sin θ
f cos θ
          f
                  θ
                            f sin θ          ∴ N cos θ = mg + f sin θ
                            mg
                                             ∴ mg = N cos θ - f sin θ .…. (1)



                                          © Prof. Mukesh N Tekwani, 2011    65
Maximum Speed of a Vehicle on a
                Banked Road with Friction
                                      All forces acting on vehicle

              N                              The horizontal component N sin θ
                            N cos θ
                                             and f cos θ provide the centripetal
                        θ                    force for circular motion
              N sin θ
f cos θ                                                            mv 2
          f
                  θ
                            f sin θ          ∴ N sin θ + f cos θ =
                                                    2
                                                                      r
                            mg                  mv
                                             ∴         = N sin θ + f cos θ … (2)
                                                  r


                                          © Prof. Mukesh N Tekwani, 2011      66
Maximum Speed of a Vehicle on a
                Banked Road with Friction
                                      All forces acting on vehicle

              N                              Dividing (2) by (1), we get
                            N cos θ
                                                      2
                                               mv
                        θ
              N sin θ                           r                          N sin θ + f cos θ
f cos θ           θ                                               =
          f                 f sin θ                                        N cos θ - f sin θ
                                                  mg
                            mg

                                                     v2                    N sin θ + f cos θ
                                              ∴         =
                                                     rg                    N cos θ - f sin θ

                                          © Prof. Mukesh N Tekwani, 2011                       67
Maximum Speed of a Vehicle on a
                Banked Road with Friction
                                         Let Vmax be the maximum speed of
              N
                                         the vehicle.
                            N cos θ

                        θ                Frictional force at this speed will be
              N sin θ                    fm = µs N
f cos θ           θ
          f                 f sin θ
                                                   2              N sin θ + fm cos θ
                            mg              v   max
                                        ∴                 =
                                                rg                N cos θ - fm sin θ



                                      © Prof. Mukesh N Tekwani, 2011                   68
Maximum Speed of a Vehicle on a
               Banked Road with Friction
But fm = µs N                                                         N sin θ µs N cos θ
                                                                             +
                                                              2       N cos θ N cos θ
    v
           2       N sin θ + µs N cos θ                v
∴       max
               =                                  ∴        max
                                                                  =
        rg         N cos θ - µs N sin θ
                                                           rg          N cos θ µs N sin θ
                                                                              -
                                                                       N cos θ N cos θ

Dividing numerator and                                       2              tan θ + µs
                                                      v   max =
denominator of RHS by                             ∴
cos θ, we get                                             rg              1 - µs tan θ



                                 © Prof. Mukesh N Tekwani, 2011                          69
Maximum Speed of a Vehicle on a
          Banked Road with Friction
                       tan θ + µs               For a frictionless road, µs = 0
        2
∴   v   m ax   = rg
                      1 - µs tan θ                                  tan θ + 0
                                              ∴ v m ax = r g
                                                                     1 - 0

                         tan θ + µs
∴   v m ax     = rg
                       1 - µs tan θ               vmax        rg tan
This is the maximum velocity
with which a vehicle can travel
on a banked road with friction.
                            © Prof. Mukesh N Tekwani, 2011                   70
Conical Pendulum
                   Definition:

                   A conical pendulum is a
                   simple pendulum which is
                   given a motion so that the
                   bob describes a horizontal
                   circle and the string
                   describes a cone.



    © Prof. Mukesh N Tekwani, 2011              71
Conical Pendulum
                   Definition:

                   A conical pendulum is a
                   simple pendulum which is
                   given such a motion that
                   the bob describes a
                   horizontal circle and the
                   string describes a cone.



    © Prof. Mukesh N Tekwani, 2011             72
Conical Pendulum – Time Period
                                    Consider a bob of mass m revolving
                                    in a horizontal circle of radius r.
                 T cos θ
                                    Let
                                    v = linear velocity of the bob
                                    h = height
                 θ
                                    T = tension in the string
                                    Θ = semi vertical angle of the cone
                                    g = acceleration due to gravity
       T sin θ
                                    l = length of the string



                     © Prof. Mukesh N Tekwani, 2011                73
Conical Pendulum – Time Period
                                    The forces acting on the bob at
                                    position A are:
                 T cos θ
                                    1) Weight of the bob acting
                                       vertically downward
                 θ
                                    2) Tension T acting along the
                                       string.
       T sin θ




                     © Prof. Mukesh N Tekwani, 2011                   74
Conical Pendulum – Time Period
                                    The tension T in the string can be
                                    resolved (broken up) into 2
                                    components as follows:
                 T cos θ

                                    i)     Tcosθ acting vertically
                                           upwards. This force is balanced
                 θ
                                           by the weight of the bob

                                           T cos θ = mg ……………………..(1)
       T sin θ




                     © Prof. Mukesh N Tekwani, 2011                  75
Conical Pendulum – Time Period
                                    (ii) T sinθ acting along the
                                    radius of the circle and directed
                                    towards the centre of the circle
                 T cos θ
                                    T sinθ provides the necessary
                                    centripetal force for circular
                 θ                  motion.

                                    ∴ T sinθ =             ……….(2)
       T sin θ
                                    Dividing (2) by (1) we get,

                                                      ………………….(3)
                     © Prof. Mukesh N Tekwani, 2011                  76
Conical Pendulum – Time Period

                                     This equation gives the speed
                 T cos θ             of the bob.
                                     But v = rw
                 θ                   ∴ rw =


       T sin θ                       Squaring both sides, we get



                     © Prof. Mukesh N Tekwani, 2011                  77
Conical Pendulum – Time Period
                                     From diagram, tan θ = r / h
                                     ∴ r 2w2 = rg
                 T cos θ




                 θ



       T sin θ




                     © Prof. Mukesh N Tekwani, 2011                78
Conical Pendulum – Time Period
                                     Periodic Time of Conical Pendulum


                 T cos θ

                                     But

                 θ



       T sin θ
                                     Solving this & substituting sin θ = r/l
                                     we get,


                     © Prof. Mukesh N Tekwani, 2011                      79
Conical Pendulum – Time Period
                                     Periodic Time of Conical Pendulum
                                     But cos θ = h/l

                 T cos θ             So the eqn               becomes,


                                                         l
                 θ                                    lx
                                      T 2                h
                                                       g
       T sin θ
                                                        h
                                           T 2
                                                        g
                     © Prof. Mukesh N Tekwani, 2011                80
Conical Pendulum – Time Period
                                     Factors affecting time period of
                                     conical pendulum:

                 T cos θ             The period of the conical pendulum
                                     depends on the following factors:

                                     i)     Length of the pendulum
                 θ                   ii)    Angle of inclination to the
                                            vertical
                                     iii)   Acceleration due to gravity at
                                            the given place
       T sin θ
                                     Time period is independent of the
                                     mass of the bob

                     © Prof. Mukesh N Tekwani, 2011                          81
Vertical Circular Motion Due to
           Earth’s Gravitation
           A                                  Consider an object
v1
                              v3              of mass m tied to
                mg                            the end of an
               T1
                     r                        inextensible string
       O                      C
                                              and whirled in a
               T2                             vertical circle of
                                              radius r.
           B             v2


                              © Prof. Mukesh N Tekwani, 2011        82
Vertical Circular Motion Due to
           Earth’s Gravitation
           A
                                        Highest Point A:
v1
                              v3
                                        Let the velocity be v1

                mg                      The forces acting on the
               T1
                     r                  object at A (highest point)
       O                      C         are:
                                        1. Tension T1 acting in
               T2
                                            downward direction
                                        2. Weight mg acting in
           B             v2                 downward direction

                              © Prof. Mukesh N Tekwani, 2011          83
Vertical Circular Motion Due to
           Earth’s Gravitation
           A
                                      At the highest point A:
v1
                              v3
                                      The centripetal force acting on
                mg                    the object at A is provided
               T1
                     r                partly by weight and partly by
       O                      C       tension in the string:
               T2



           B             v2                                     …… (1)


                              © Prof. Mukesh N Tekwani, 2011        84
Vertical Circular Motion Due to
           Earth’s Gravitation
           A
                                        Lowest Point B:
v1
                              v3
                                        Let the velocity be v2

                mg                      The forces acting on the
               T1
                     r                  object at B (lowest point) are:
       O                      C         1. Tension T2 acting in
                                           upward direction
               T2
                                        2. Weight mg acting in
                                           downward direction
           B             v2


                              © Prof. Mukesh N Tekwani, 2011          85
Vertical Circular Motion Due to
           Earth’s Gravitation
           A
                                      At the lowest point B:
v1
                              v3


                mg
                                                               …… (2)
               T1
                     r
       O                      C


               T2



           B             v2


                              © Prof. Mukesh N Tekwani, 2011            86
Vertical Circular Motion Due to
           Earth’s Gravitation
                                      Linear velocity of object at highest
           A
v1                                    point A:
                              v3

                                      The object must have a certain
                mg
                                      minimum velocity at point A so as to
               T1
                     r                continue in circular path.
       O                      C
                                      This velocity is called the critical
               T2                     velocity. Below the critical velocity,
                                      the string becomes slack and the
                                      tension T1 disappears (T1 = 0)
           B             v2


                              © Prof. Mukesh N Tekwani, 2011                 87
Vertical Circular Motion Due to
           Earth’s Gravitation
                                      Linear velocity of object at highest
           A
v1                                    point A:
                              v3


                mg
               T1
                     r
       O                      C


               T2



           B             v2


                              © Prof. Mukesh N Tekwani, 2011                 88
Vertical Circular Motion Due to
           Earth’s Gravitation
                                      Linear velocity of object at highest
           A
v1                                    point A:
                              v3


                mg                      This is the minimum velocity that
               T1                       the object must have at the
                     r
       O                      C         highest point A so that the string
                                        does not become slack.
               T2
                                        If the velocity at the highest point
                                        is less than this, the object can not
           B             v2             continue in circular orbit and the
                                        string will become slack.
                              © Prof. Mukesh N Tekwani, 2011                 89
Vertical Circular Motion Due to
           Earth’s Gravitation
                                      Linear velocity of object at lowest
           A
v1                                    point B:
                              v3
                                        When the object moves from the lowest
                                        position to the highest position, the
                mg
                                        increase in potential energy is mg x 2r
               T1
                     r
       O                      C         By the law of conservation of energy,
                                        KEA + PEA = KEB + PEB
               T2



           B             v2


                              © Prof. Mukesh N Tekwani, 2011                    90
Vertical Circular Motion Due to
           Earth’s Gravitation
                                      Linear velocity of object at lowest
           A
v1                                    point B:
                              v3
                                        At the highest point A, the minimum
                mg                      velocity must be

               T1
                     r
       O                      C
                                         Using this in

               T2
                                         we get,


           B             v2


                              © Prof. Mukesh N Tekwani, 2011                  91
Vertical Circular Motion Due to
           Earth’s Gravitation
                                      Linear velocity of object at lowest
           A
v1                                    point B:
                              v3


                mg
                                       Therefore, the velocity of the particle is
               T1                      highest at the lowest point.
                     r
                                       If the velocity of the particle is less than
       O                      C
                                       this it will not complete the circular path.

               T2



           B             v2


                              © Prof. Mukesh N Tekwani, 2011                          92
Linear Velocity at a point midway between top
    and bottom positions in a vertical circle
                                The total energy of a body performing
          A                     circular motion is constant at all points on
 v1
                       v3       the path.

                                By law of conservation of energy,
                                Total energy at B = Total energy at C
              r
      O                C




          B       v2


                       © Prof. Mukesh N Tekwani, 2011                      93
Kuch Self-study bhi Karo Na!
1. Derive an expression for the tension in the string of
   a conical pendulum.
2. Write kinematical equations for circular motion in
   analogy with linear motion.
3. Derive the expression for the tension in a string in
   vertical circular motion at any position.
4. Derive the expression for the linear velocity at a
   point midway between the top position and the
   bottom position in vertical circular motion, without
   the string slackening at the top.

                     © Prof. Mukesh N Tekwani, 2011        94
Circular motion

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Circular motion

  • 1. Prof. Mukesh N. Tekwani Department of Physics I. Y. College, Mumbai mukeshtekwani@outlook.com © Prof. Mukesh N Tekwani, 2011 1
  • 2. Circular Motion © Prof. Mukesh N Tekwani, 2011 2
  • 3. Why study Circular Motion? • To understand – Motion of planets – Motion of electrons around the nucleus – Motion of giant wheel – Motion of space stations – Motion of moon and satellites © Prof. Mukesh N Tekwani, 2011 3
  • 4. Circular Motion • It is defined as the motion of a particle along a complete circle or part of a circle. • Fore circular motion, it is NOT necessary that the body should complete a full circle. • Even motion along arc of a circle is circular motion © Prof. Mukesh N Tekwani, 2011 4
  • 5. Circular Motion How do we locate something on a circle? Give its angular position θ y f What is the location of i X 900 or π/2 θ=0 © Prof. Mukesh N Tekwani, 2011 5
  • 6. Circular Motion y f is the angular position. i Angular displacement: x f i Note: angles measured Clockwise (CW) are negative and angles measured (CCW) are positive. is measured in radians. 2 radians = 360Tekwani, 1 revolution © Prof. Mukesh N = 2011 6
  • 7. Angular Displacement • Angular displacement is defined as the angle described by the radius vector Initial position of particle is a Final position of particle is b Angular displacement in time t is Θ a © Prof. Mukesh N Tekwani, 2011 7
  • 8. Angular Displacement S =r Θ © Prof. Mukesh N Tekwani, 2011 8
  • 9. arclength = s = r y s f r r i is a ratio of two lengths; x it is a dimensionless ratio! This is a radian measure of angle If we go all the way round s =2πr and Δθ =2 π © Prof. Mukesh N Tekwani, 2011 9
  • 10. Right Hand Rule If the fingers of the right hand are curled in the direction of revolution of the particle, then the outstretched thumb gives the direction of the angular displacement vector. © Prof. Mukesh N Tekwani, 2011 11
  • 11. Stop & Think – Pg 2 Are the following motions same or different? 1. The motion of the tip of second hand of a clock. 2. The motion of the entire second hand of a clock. The motion of the tip of second hand of a clock is uniform circular motion. The motion of the entire second hand is a rotational motion. © Prof. Mukesh N Tekwani, 2011 12
  • 12. Centripetal Force • UCM is an accelerated motion. Why? • UCM is accelerated motion because the velocity of the body changes at every instant (i.e. every moment) • But, according to Newton’s Second Law, there must be a force to produce this acceleration. • This force is called the centripetal force. • Therefore, Centripetal force is required for circular motion. No centripetal force +> no circular motion. © Prof. Mukesh N Tekwani, 2011 25
  • 13. Velocity and Speed in UCM Is speed changing? No, speed is constant Is velocity changing? Yes, velocity is changing because velocity is a vector – and direction is changing at every point © Prof. Mukesh N Tekwani, 2011 26
  • 14. Velocity and Speed in UCM Is speed changing? No, speed is constant Is velocity changing? Yes, velocity is changing because velocity is a vector – and direction is changing at every point © Prof. Mukesh N Tekwani, 2011 27
  • 15. Examples of Centripetal force A body tied to a string and whirled in a horizontal circle – CPF is provided by the tension in the string. © Prof. Mukesh N Tekwani, 2011 28
  • 16. Examples of Centripetal force • For a car travelling around a circular road with uniform speed, the CPF is provided by the force of static friction between tyres of the car and the road. © Prof. Mukesh N Tekwani, 2011 29
  • 17. Examples of Centripetal force • In case of electrons revolving around the nucleus, the centripetal force is provided by the electrostatic force of attraction between the nucleus and the electrons • In case of the motion of moon around the earth, the CPF is provided by the ______ force between Earth and Moon © Prof. Mukesh N Tekwani, 2011 30
  • 18. Centripetal Force • Centripetal force – It is the force acting on a particle performing UCM and this force is along the radius of the circle and directed towards the centre of the circle. REMEMBER! Centripetal force - acting on a particle performing UCM - along the radius - acting towards the centre of the circle. © Prof. Mukesh N Tekwani, 2011 31
  • 19. Properties of Centripetal Force 1. Centripetal force is a real force 2. CPF is necessary for maintaining UCM. 3. CPF acts along the radius of the circle 4. CPF is directed towards center of the circle. 5. CPF does not do any work 6. F = mv2/ r © Prof. Mukesh N Tekwani, 2011 32
  • 20. Radial Acceleration Let P be the position of the particle Y performing UCM v P(x, y) r is the radius vector N Θ = ωt . This is the angular displacement of r the particle in time t secs y θ V is the tangential velocity of the particle at O x M X point P. Draw PM ┴ OX The angular displacement of the particle in time t secs is LMOP = Θ = ωt © Prof. Mukesh N Tekwani, 2011 33
  • 21. Radial Acceleration Y The position vector of the particle at v any time is given by: P(x, y) r = ix + jy N r From ∆POM y θ sin θ = PM/OP O x M X ∴ sin θ = y / r ∴y = r sin θ But θ = ωt ∴ y = r sin ωt © Prof. Mukesh N Tekwani, 2011 34
  • 22. Radial Acceleration Y Similarly, v From ∆POM P(x, y) N cos θ = OM/OP r y ∴ cos θ = x / r θ O x M X ∴ x = r cos θ But θ = ωt ∴ x = r cos ωt © Prof. Mukesh N Tekwani, 2011 35
  • 23. Radial Acceleration The velocity of particle at any instant (any time) is called its instantaneous velocity. The instantaneous velocity is given by v = dr / dt ∴ v = d/dt [ ir cos wt + jr sin wt] ∴ v = - i r w sin wt + j r w cos wt © Prof. Mukesh N Tekwani, 2011 36
  • 24. Radial Acceleration The linear acceleration of the particle at any instant (any time) is called its instantaneous linear acceleration. © Prof. Mukesh N Tekwani, 2011 37
  • 25. Radial Acceleration Therefore, the instantaneous linear acceleration is given by ∴ a = - w2 r r a Importance of the negative sign: The negative sign in the above equation indicates that the linear acceleration of the particle and the radius vector are in opposite directions. © Prof. Mukesh N Tekwani, 2011 38
  • 26. Relation Between Angular Acceleration and Linear Acceleration The acceleration of a particle ∵ r is a constant radius, is given by ………………. (1) ∴ But v = r w But ∴ α is the angular acceleration ∴a = .... (2) ∴ a=rα ………………………(3) © Prof. Mukesh N Tekwani, 2011 39
  • 27. Relation Between Angular Acceleration and Linear Acceleration ∴ v=wxr Differentiating w.r.t. time t, ∴ linear acceleration a = a T + aR aT is called the tangential component of linear acceleration aR is called the radial component of linear acceleration But For UCM, w = constant, so and ∴ a = aR ∴ in UCM, linear accln is centripetal accln © Prof. Mukesh N Tekwani, 2011 40
  • 28. Centrifugal Force 1. Centrifugal force is an imaginary force (pseudo force) experienced only in non-inertial frames of reference. 2. This force is necessary in order to explain Newton’s laws of motion in an accelerated frame of reference. 3. Centrifugal force is acts along the radius but is directed away from the centre of the circle. 4. Direction of centrifugal force is always opposite to that of the centripetal force. 5. Centrifugal force 6. Centrifugal force is always present in rotating bodies © Prof. Mukesh N Tekwani, 2011 41
  • 29. Examples of Centrifugal Force 1. When a car in motion takes a sudden turn towards left, passengers in the car experience an outward push to the right. This is due to the centrifugal force acting on the passengers. 2. The children sitting in a merry-go-round experience an outward force as the merry-go-round rotates about the vertical axis. Centripetal and Centrifugal forces DONOT constitute an action- reaction pair. Centrifugal force is not a real force. For action- reaction pair, both forces must be real. © Prof. Mukesh N Tekwani, 2011 42
  • 30. Banking of Roads 1. When a car is moving along a curved road, it is performing circular motion. For circular motion it is not necessary that the car should complete a full circle; an arc of a circle is also treated as a circular path. 2. We know that centripetal force (CPF) is necessary for circular motion. If CPF is not present, the car cannot travel along a circular path and will instead travel along a tangential path. © Prof. Mukesh N Tekwani, 2011 43
  • 31. Banking of Roads 3. The centripetal force for circular motion of the car can be provided in two ways: • Frictional force between the tyres of the car and the road. • Banking of Roads © Prof. Mukesh N Tekwani, 2011 44
  • 32. Friction between Tyres and Road The centripetal force for circular motion of the car is provided by the frictional force between the tyres of the car and the road. Let m = mass of the car V = speed of the car, and R = radius of the curved road. Since centripetal force is provided by the frictional force, CPF = frictional force (“provide by” means “equal to” ) (µ is coefficient of friction between tyres & road) So and © Prof. Mukesh N Tekwani, 2011 45
  • 33. Friction between Tyres and Road Thus, the maximum velocity with which a car can safely travel along a curved road is given by If the speed of the car increases beyond this value, the car will be thrown off (skid). If the car has to move at a higher speed, the frictional force should be increased. But this cause wear and tear of tyres. The frictional force is not reliable as it can decrease on wet roads So we cannot rely on frictional force to provide the centripetal force for circular motion. © Prof. Mukesh N Tekwani, 2011 46
  • 34. Friction between Tyres and Road R1 and R2 are reaction forces due to the tyres mg is the weight of the car, Center of acting vertically downwards circular path F1 and F2 are the frictional forces between the tyres and the road. These frictional forces act towards the centre of the circular path and provide the necessary centripetal force. © Prof. Mukesh N Tekwani, 2011 47
  • 35. Friction between Tyres and Road © Prof. Mukesh N Tekwani, 2011 48
  • 36. Friction between Tyres and Road – Car Skidding © Prof. Mukesh N Tekwani, 2011 49
  • 37. Banked Roads What is banking of roads? The process of raising the outer edge of a road over the inner edge through a certain angle is known as banking of road. © Prof. Mukesh N Tekwani, 2011 50
  • 38. Banking of Roads Purpose of Banking of Roads: Banking of roads is done: 1. To provide the necessary centripetal force for circular motion 2. To reduce wear and tear of tyres due to friction 3. To avoid skidding 4. To avoid overturning of vehicles © Prof. Mukesh N Tekwani, 2011 51
  • 39. Banked Roads © Prof. Mukesh N Tekwani, 2011 52
  • 40. Banked Roads What is angle of R cos θ R banking? Θ The angle made by the R sin θ surface of the road with the horizontal surface is called as angle of banking. Θ Horizontal W = mg © Prof. Mukesh N Tekwani, 2011 53
  • 41. Banked Roads Consider a car moving R cos θ R along a banked road. Θ R sin θ Let m = mass of the car V = speed of the car Θ θ is angle of banking W = mg © Prof. Mukesh N Tekwani, 2011 54
  • 42. Banked Roads The forces acting on the R cos θ R car are: Θ R sin θ (i) Its weight mg acting vertically downwards. Θ (ii) The normal reaction R acting perpendicular to the W = mg surface of the road. © Prof. Mukesh N Tekwani, 2011 55
  • 43. Banked Roads The normal reaction can be R cos θ resolved (broken up) into R Θ two components: R sin θ 1. R cosθ is the vertical component Θ 2. R sinθ is the horizontal component W = mg © Prof. Mukesh N Tekwani, 2011 56
  • 44. Banked Roads Since the vehicle has no R cos θ vertical motion, the weight R Θ is balanced by the vertical component R sin θ R cosθ = mg …………… (1) Θ (weight is balanced by vertical component means weight is equal to vertical component) W = mg © Prof. Mukesh N Tekwani, 2011 57
  • 45. Banked Roads The horizontal component R cos θ is the unbalanced R Θ component . This horizontal component acts towards R sin θ the centre of the circular path. Θ This component provides the centripetal force for circular motion W = mg R sinθ = …………… (2) © Prof. Mukesh N Tekwani, 2011 58
  • 46. Banked Roads Dividing (2) by (1), we get θ = tan-1 ( ) R sinθ = mg Therefore, the angle of banking R cos θ is independent of the mass of the vehicle. So, The maximum speed with which the vehicle can safely tan θ = travel along the curved road is © Prof. Mukesh N Tekwani, 2011 59
  • 47. Banked Roads A car travels at a constant speed around two curves. Where is the car most likely to skid? Why? 2 mv F = ma r Smaller radius: larger centripetal force is required to keep it in uniform circular motion. © Prof. Mukesh N Tekwani, 2011 60
  • 48. Maximum Speed of a Vehicle on a Banked Road with Friction Consider a vehicle moving along a curved banked road. Let m = mass of vehicle r = radius of curvature of road θ = angle of banking F = frictional force between tyres and road. The forces acting on the vehicle are shown in the diagram. © Prof. Mukesh N Tekwani, 2011 61
  • 49. Maximum Speed of a Vehicle on a Banked Road with Friction The forces acting on the vehicle are: 1) Weight of the vehicle mg, acting vertically downwards 2) Normal reaction N acting on vehicle, perpendicular to the surface of the road. 3) Friction force between tyres and road. Forces N and frictional force f are now resolved into two components © Prof. Mukesh N Tekwani, 2011 62
  • 50. Maximum Speed of a Vehicle on a Banked Road with Friction Resolving the Normal reaction The normal reaction N is resolved into 2 components: 1) N cos θ is vertical component of N 2) N sin θ is horizontal component of N © Prof. Mukesh N Tekwani, 2011 63
  • 51. Maximum Speed of a Vehicle on a Banked Road with Friction Resolving the frictional force The frictional force f is resolved into 2 components: f cos θ 1) f cos θ is horizontal component of f f θ f sin θ 2) f sin θ is vertical component of f © Prof. Mukesh N Tekwani, 2011 64
  • 52. Maximum Speed of a Vehicle on a Banked Road with Friction All forces acting on vehicle N The vertical component N cos θ is N cos θ balanced by the weight of the θ vehicle and the component f sin θ N sin θ f cos θ f θ f sin θ ∴ N cos θ = mg + f sin θ mg ∴ mg = N cos θ - f sin θ .…. (1) © Prof. Mukesh N Tekwani, 2011 65
  • 53. Maximum Speed of a Vehicle on a Banked Road with Friction All forces acting on vehicle N The horizontal component N sin θ N cos θ and f cos θ provide the centripetal θ force for circular motion N sin θ f cos θ mv 2 f θ f sin θ ∴ N sin θ + f cos θ = 2 r mg mv ∴ = N sin θ + f cos θ … (2) r © Prof. Mukesh N Tekwani, 2011 66
  • 54. Maximum Speed of a Vehicle on a Banked Road with Friction All forces acting on vehicle N Dividing (2) by (1), we get N cos θ 2 mv θ N sin θ r N sin θ + f cos θ f cos θ θ = f f sin θ N cos θ - f sin θ mg mg v2 N sin θ + f cos θ ∴ = rg N cos θ - f sin θ © Prof. Mukesh N Tekwani, 2011 67
  • 55. Maximum Speed of a Vehicle on a Banked Road with Friction Let Vmax be the maximum speed of N the vehicle. N cos θ θ Frictional force at this speed will be N sin θ fm = µs N f cos θ θ f f sin θ 2 N sin θ + fm cos θ mg v max ∴ = rg N cos θ - fm sin θ © Prof. Mukesh N Tekwani, 2011 68
  • 56. Maximum Speed of a Vehicle on a Banked Road with Friction But fm = µs N N sin θ µs N cos θ + 2 N cos θ N cos θ v 2 N sin θ + µs N cos θ v ∴ max = ∴ max = rg N cos θ - µs N sin θ rg N cos θ µs N sin θ - N cos θ N cos θ Dividing numerator and 2 tan θ + µs v max = denominator of RHS by ∴ cos θ, we get rg 1 - µs tan θ © Prof. Mukesh N Tekwani, 2011 69
  • 57. Maximum Speed of a Vehicle on a Banked Road with Friction tan θ + µs For a frictionless road, µs = 0 2 ∴ v m ax = rg 1 - µs tan θ tan θ + 0 ∴ v m ax = r g 1 - 0 tan θ + µs ∴ v m ax = rg 1 - µs tan θ vmax rg tan This is the maximum velocity with which a vehicle can travel on a banked road with friction. © Prof. Mukesh N Tekwani, 2011 70
  • 58. Conical Pendulum Definition: A conical pendulum is a simple pendulum which is given a motion so that the bob describes a horizontal circle and the string describes a cone. © Prof. Mukesh N Tekwani, 2011 71
  • 59. Conical Pendulum Definition: A conical pendulum is a simple pendulum which is given such a motion that the bob describes a horizontal circle and the string describes a cone. © Prof. Mukesh N Tekwani, 2011 72
  • 60. Conical Pendulum – Time Period Consider a bob of mass m revolving in a horizontal circle of radius r. T cos θ Let v = linear velocity of the bob h = height θ T = tension in the string Θ = semi vertical angle of the cone g = acceleration due to gravity T sin θ l = length of the string © Prof. Mukesh N Tekwani, 2011 73
  • 61. Conical Pendulum – Time Period The forces acting on the bob at position A are: T cos θ 1) Weight of the bob acting vertically downward θ 2) Tension T acting along the string. T sin θ © Prof. Mukesh N Tekwani, 2011 74
  • 62. Conical Pendulum – Time Period The tension T in the string can be resolved (broken up) into 2 components as follows: T cos θ i) Tcosθ acting vertically upwards. This force is balanced θ by the weight of the bob T cos θ = mg ……………………..(1) T sin θ © Prof. Mukesh N Tekwani, 2011 75
  • 63. Conical Pendulum – Time Period (ii) T sinθ acting along the radius of the circle and directed towards the centre of the circle T cos θ T sinθ provides the necessary centripetal force for circular θ motion. ∴ T sinθ = ……….(2) T sin θ Dividing (2) by (1) we get, ………………….(3) © Prof. Mukesh N Tekwani, 2011 76
  • 64. Conical Pendulum – Time Period This equation gives the speed T cos θ of the bob. But v = rw θ ∴ rw = T sin θ Squaring both sides, we get © Prof. Mukesh N Tekwani, 2011 77
  • 65. Conical Pendulum – Time Period From diagram, tan θ = r / h ∴ r 2w2 = rg T cos θ θ T sin θ © Prof. Mukesh N Tekwani, 2011 78
  • 66. Conical Pendulum – Time Period Periodic Time of Conical Pendulum T cos θ But θ T sin θ Solving this & substituting sin θ = r/l we get, © Prof. Mukesh N Tekwani, 2011 79
  • 67. Conical Pendulum – Time Period Periodic Time of Conical Pendulum But cos θ = h/l T cos θ So the eqn becomes, l θ lx T 2 h g T sin θ h T 2 g © Prof. Mukesh N Tekwani, 2011 80
  • 68. Conical Pendulum – Time Period Factors affecting time period of conical pendulum: T cos θ The period of the conical pendulum depends on the following factors: i) Length of the pendulum θ ii) Angle of inclination to the vertical iii) Acceleration due to gravity at the given place T sin θ Time period is independent of the mass of the bob © Prof. Mukesh N Tekwani, 2011 81
  • 69. Vertical Circular Motion Due to Earth’s Gravitation A Consider an object v1 v3 of mass m tied to mg the end of an T1 r inextensible string O C and whirled in a T2 vertical circle of radius r. B v2 © Prof. Mukesh N Tekwani, 2011 82
  • 70. Vertical Circular Motion Due to Earth’s Gravitation A Highest Point A: v1 v3 Let the velocity be v1 mg The forces acting on the T1 r object at A (highest point) O C are: 1. Tension T1 acting in T2 downward direction 2. Weight mg acting in B v2 downward direction © Prof. Mukesh N Tekwani, 2011 83
  • 71. Vertical Circular Motion Due to Earth’s Gravitation A At the highest point A: v1 v3 The centripetal force acting on mg the object at A is provided T1 r partly by weight and partly by O C tension in the string: T2 B v2 …… (1) © Prof. Mukesh N Tekwani, 2011 84
  • 72. Vertical Circular Motion Due to Earth’s Gravitation A Lowest Point B: v1 v3 Let the velocity be v2 mg The forces acting on the T1 r object at B (lowest point) are: O C 1. Tension T2 acting in upward direction T2 2. Weight mg acting in downward direction B v2 © Prof. Mukesh N Tekwani, 2011 85
  • 73. Vertical Circular Motion Due to Earth’s Gravitation A At the lowest point B: v1 v3 mg …… (2) T1 r O C T2 B v2 © Prof. Mukesh N Tekwani, 2011 86
  • 74. Vertical Circular Motion Due to Earth’s Gravitation Linear velocity of object at highest A v1 point A: v3 The object must have a certain mg minimum velocity at point A so as to T1 r continue in circular path. O C This velocity is called the critical T2 velocity. Below the critical velocity, the string becomes slack and the tension T1 disappears (T1 = 0) B v2 © Prof. Mukesh N Tekwani, 2011 87
  • 75. Vertical Circular Motion Due to Earth’s Gravitation Linear velocity of object at highest A v1 point A: v3 mg T1 r O C T2 B v2 © Prof. Mukesh N Tekwani, 2011 88
  • 76. Vertical Circular Motion Due to Earth’s Gravitation Linear velocity of object at highest A v1 point A: v3 mg This is the minimum velocity that T1 the object must have at the r O C highest point A so that the string does not become slack. T2 If the velocity at the highest point is less than this, the object can not B v2 continue in circular orbit and the string will become slack. © Prof. Mukesh N Tekwani, 2011 89
  • 77. Vertical Circular Motion Due to Earth’s Gravitation Linear velocity of object at lowest A v1 point B: v3 When the object moves from the lowest position to the highest position, the mg increase in potential energy is mg x 2r T1 r O C By the law of conservation of energy, KEA + PEA = KEB + PEB T2 B v2 © Prof. Mukesh N Tekwani, 2011 90
  • 78. Vertical Circular Motion Due to Earth’s Gravitation Linear velocity of object at lowest A v1 point B: v3 At the highest point A, the minimum mg velocity must be T1 r O C Using this in T2 we get, B v2 © Prof. Mukesh N Tekwani, 2011 91
  • 79. Vertical Circular Motion Due to Earth’s Gravitation Linear velocity of object at lowest A v1 point B: v3 mg Therefore, the velocity of the particle is T1 highest at the lowest point. r If the velocity of the particle is less than O C this it will not complete the circular path. T2 B v2 © Prof. Mukesh N Tekwani, 2011 92
  • 80. Linear Velocity at a point midway between top and bottom positions in a vertical circle The total energy of a body performing A circular motion is constant at all points on v1 v3 the path. By law of conservation of energy, Total energy at B = Total energy at C r O C B v2 © Prof. Mukesh N Tekwani, 2011 93
  • 81. Kuch Self-study bhi Karo Na! 1. Derive an expression for the tension in the string of a conical pendulum. 2. Write kinematical equations for circular motion in analogy with linear motion. 3. Derive the expression for the tension in a string in vertical circular motion at any position. 4. Derive the expression for the linear velocity at a point midway between the top position and the bottom position in vertical circular motion, without the string slackening at the top. © Prof. Mukesh N Tekwani, 2011 94