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Law of Universal Gravitation

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Title: Law of Universal Gravitation


1
Law of Universal Gravitation
  • Holt Physics
  • Pages 263 - 265

2
Vertical vs horizontal circles
  • Unlike object moving in horizontal circles, an
    object moving in a vertical circle is effected by
    weight.
  • In vertical circles, the speed is not constant
    and neither is the tension in the string.

3
Vertical vs horizontal circles
  • At the top of the circular path, the speed and
    the tension in the string are at a minimum.
  • At the bottom of the circle, the speed and
    tension in the string are at a maximum.

4
forces acting in a vertical circle
5
forces acting in a vertical circle
  • At the top and bottom of the circle, FC ?FV.
  • Therefore, at the top of the circle
  • TS Tension in string(N)
  • m mass (kg)
  • g 9.8 m/s2, down
  • v speed at that point (m/s)
  • r radius of circle (m)

6
forces acting in a vertical circle
  • At the top and bottom of the circle, FC ?FV.
  • Therefore, at the bottom of the circle
  • TS Tension in string (N)
  • m mass (kg)
  • g 9.8 m/s2, down
  • v speed at that point (m/s)
  • r radius of circle (m)

7
  • The formulas you learned that apply to horizontal
    circles can also be used to apply to vertical
    circles at certain points.

8
formulas
T period or time for one revolution (sec) f
frequency or revolutions per second (Hz or
sec-1)
9
formulas
  • T period or time for one revolution (sec)
  • f frequency or revolutions per second (Hz or
    sec-1)

10
formulas
  • ac centripetal acceleration (m/s2)
  • r radius of circle (m)
  • v speed (m/s)

11
formulas
  • ac centripetal acceleration (m/s2)
  • r radius of circle (m)
  • T period or time for one revolution (sec)

12
formulas
  • Fc centripetal force (N)
  • m mass (kg)
  • ac centripetal acceleration (m/s2)

13
formulas
  • Fc centripetal force (N)
  • m mass (kg)
  • v speed (m/s)
  • r radius of circle (m)

14
formulas
  • Fc centripetal force (N)
  • m mass (kg)
  • r radius of circle (m)
  • T period or time for one revolution (sec)

15
Sample Problem
  • A stuntman swings from the end of a 4 m long rope
    along the arc of a circle. At the bottom of his
    path his speed is 9 m/s. (a) What is the
    centripetal acceleration at this point? (b) If
    his mass is 70 kg, find the tension in the rope
    at this point.

a. 20.25 m/s2
b. 2103 N
16
critical velocity
  • The critical velocity is the minimum velocity an
    object can have and remain in a vertical circle
    of constant radius.
  • If an object does not maintain the critical
    velocity, the radius of the orbit begins to decay
    (get smaller).

17
Critical velocity
  • vcrit critical velocity (m/s)
  • r radius (m)
  • g acceleration due to gravity (m/s2)

18
Sample Problem
  • A carnival clown rides a motorcycle down a ramp
    and around a loop-the-loop. If the loop has a
    radius of 18 m, what is the slowest speed the
    rider can have at the top of the loop to avoid
    falling?

13.28 m/s
19
Sample Problem
  • A 75-kg pilot flies a plane in a loop near the
    earths surface. At the top of the loop, where
    the plane is completely upside-down for an
    instant, the pilot hangs freely in the seat and
    does not push against the seat belt. The
    airspeed indicator reads 120 m/s. What is the
    radius of the planes loop?

1469 m
20
Newtons Law of Universal Gravitation
  • Law of Universal Gravitation - there is a force
    of attraction between any two objects with mass.

21
Newtons Law of Universal Gravitation
  • F Force of attraction (N)
  • G 6.67 10-11 Nm2/kg2
  • m1 mass of object one (kg)
  • m2 mass of object two (kg)
  • d distance between the centers of the two
    objects (m)

22
Accepted Values
  • me mass of the Earth
  • (5.98 1024 kg)
  • re radius of the Earth
  • (6.37 106 m)

23
Satellites
  • Satellites actually move in elliptical orbits but
    we will treat them as though they are circular
    orbits. The weight of the satellite is actually
    the gravitational attraction between the
    satellite and the Earth.

24
Acceleration due to Gravity
  • When the weight of the satellite (msg) is set
    equal to the gravitational attraction between the
    earth and the satellite (Gmsme/d2), the mass of
    the satellite will cancel out telling us that the
    acceleration due to gravity at any point can be
    calculated using the following equation.

25
Acceleration due to Gravity
  • G 6.67 10-11 Nm2/kg2
  • m2 mass of the celestial body at the center of
    rotation (kg)
  • d distance between the centers of the two
    objects (m)

26
Satellite Speed
  • The critical speed of a satellite can be
    calculated using

27
Period of a Satellite
  • The period of a satellite can be calculated using

28
Weightlessness
  • True weightlessness does not exist.
  • In order to be truly weightless you would have to
    be infinitely far from all other objects with
    mass, since this is not possible, all objects
    have weight.

29
Weightlessness
  • Astronauts are said to be weightless but in
    actuality they are in freefall toward the Earth
    just as their spaceship is. Hence they are both
    accelerating at the same rate so you have the
    appearance of weightlessness.
  • The misnomer (wrong name) came about due to the
    fact that if you attempted to weigh them the
    scale would register a value of zero since both
    are in free fall

30
  • Therefore, the astronauts would weigh zero but
    would not have a weight of zero.

31
Field Concept
  • A field is a region in which a suitable detector
    experiences a force.
  • A suitable detector for a gravitational field is
    an object with a very small mass.
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