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Title: Welcome to Physics I !!!


1
Physics I95.141LECTURE 1010/12/10
2
Exam Prep Problem (Conical Pendulum)
  • A mass (m2kg) suspended on a cord (l1m)
    revolves in a circle of radius r. (?30º)
  • A) (10pts) Draw a free body diagram for the mass,
    labeling your coordinate system
  • B) (5pts) What is the Tension in the cord?
  • C) (5pts) What is the acceleration of the ball,
    and in what direction?
  • D) (5pts) What is the tangential velocity of the
    ball?

3
Exam Prep Problem (Conical Pendulum)
  • A mass (m2kg) suspended on a cord (l1m)
    revolves in a circle of radius r. (?30º)
  • A) (10pts) Draw a free body diagram for the mass,
    labeling your coordinate system

4
Exam Prep Problem (Conical Pendulum)
  • A mass (m2kg) suspended on a cord (l1m)
    revolves in a circle of radius r. (?30º)
  • B) (5pts) What is the tension in the cord?

5
Exam Prep Problem (Conical Pendulum)
  • A small mass (m) suspended on a cord (l1m)
    revolves in a circle of radius r. (?30º)
  • C) (5pts) What is the acceleration of the ball,
    and in what direction?

6
Exam Prep Problem (Conical Pendulum)
  • A small mass (m) suspended on a cord (l1m)
    revolves in a circle of radius r. (?30º)
  • D) (5pts) What is the tangential velocity of the
    ball?

7
Outline
  • Highway curves (circular motion)
  • Newtons Law of Universal Gravitation
  • Weightlessness
  • Keplers Laws
  • What do we know?
  • Units
  • Kinematic equations
  • Freely falling objects
  • Vectors
  • Kinematics Vectors Vector Kinematics
  • Relative motion
  • Projectile motion
  • Uniform circular motion
  • Newtons Laws
  • Force of Gravity/Normal Force
  • Free Body Diagrams
  • Problem solving
  • Uniform Circular Motion

8
Highway Curves
  • In order for the car to make a curve without
    slipping/skidding, need sufficient Force from
    friction.
  • This force is a static friction, even though the
    car is moving!!
  • Coordinate system!!!

9
Flat Curves (unbanked)
  • What is the coefficient of static friction
    required to make an unbanked curve with radius R,
    for a car traveling with a speed v?

10
Banked Curves
  • Can a car make a turn on a banked frictionless
    surface without skidding? For speed v, radius R,
    what angle is required?
  • Coordinate system!!

11
Example Problem
  • A car goes around an unbanked curve (R100m) at a
    speed of 50m/s. The concrete/tire interface has
    a coefficient of static friction of 1. Can the
    car make this turn?

12
Example Problem
  • A car goes around an banked curve (R100m) at a
    speed of 50m/s. Ignoring friction, what angle
    should the curve be banked at to allow the car to
    make the curve?

13
Newtons Law of Universal Gravitation
  • We know that falling objects accelerate.
  • We also know that if an object accelerates, there
    must be a force acting on it.
  • The Force that accelerates falling bodies is
    gravity.
  • But what exerts this force?
  • Since all falling objects fall towards the center
    of the Earth, Newton suggested that it is the
    Earth itself which is exerting this Force.

14
Newtons Law of Universal Gravitation
  • What form does this Force take?
  • 1) Dependence on distance
  • Newton knew that the moon orbited the Earth.
  • We know that a circular motion requires an inward
    radial acceleration

15
Newtons Law of Universal Gravitation
  • So if the Force causing the moon to orbit the
    Earth, is the same force which causes object to
    accelerate at the surface of the Earth, then this
    Force goes as the inverse square of the distance
    from the center of the Earth

16
Newtons Law of Universal Gravitation
  • The other thing we should note, is that the Force
    due to gravity produces the same acceleration for
    ALL OBJECTS, regardless of mass. So this is a
    Force which must scale with the mass of the
    object.
  • Symmetry (Newtons 3rd Law) also suggests that
    this Force must depend on the mass of the Earth,
    or the second body.

17
Newtons Law of Universal Gravitation
  • Finally, Newton argues that if this is the Force
    causing the moon to orbit the Earth, perhaps it
    is also the Force causing the planets to Orbit
    the sun. In fact, perhaps every mass exerts a
    gravitational force on every other mass in the
    universe.
  • And we can write this force as

18
Direction of Gravitational Force
  • Force is a vector, and therefore has a magnitude
    and direction.
  • Direction is along line connecting two masses.

19
Example Problem
  • Imagine 3 Blocks, of equal mass, placed at three
    corners of a square. Draw the gravitational
    Force vectors acting on each block.

1
3
2
20
Gravitational Attraction Between Two People
  • Tom Cruise (160lbs) and Katie Holmes (118lbs) are
    dancing (about 0.5 m apart). What is attractive
    Force of Gravity between them?

21
Gravity at Earths Surface
  • If this law is correct, what should we get for Fg
    at the Earths surface?

22
Satellites
  • Imagine I throw a ball with some horizontal
    velocity vo.
  • In previous chapters, we studied projectile
    motion, which tells us the ball will accelerate
    towards earth and eventually fall to Earth.
  • But this is an approximationthe Earth is not
    flat, and the Force of gravity is not downward,
    but towards the center of the Earth.

23
Satellites
  • In order for an object to travel with uniform
    circular motion, a radial Force is required.
  • What speed would the ball need to have to travel
    in a circular path at the surface of the Earth?

24
Satellites
  • The uniform circular motion due to gravitation is
    known as an orbit, and an orbiting object is
    often referred to as a satellite.
  • We can calculate the speed of a satellite for a
    given orbital radius

25
Geosynchronous Orbit
  • A geosynchronous orbit, is one that orbits at the
    same speed the Earth rotates, so that the
    satellite stays at the same position with respect
    to Earth as it orbits. How can we calculate the
    height of a satellite of mass M in geosynchronous
    orbit?

26
Weightlessness
  • Remember, we define weight as the magnitude of
    the Force of gravity acting on an object.
  • At the surface of Earth this is mg.
  • But we measure weight, by measuring the Force a
    mass exerts on a scale.
  • Imagine we are weighing a mass in an elevator.
  • If the elevator is at rest, or moving at a
    constant velocity, what does the scale read?

27
Weightlessness
  • Now, if the elevator is accelerating upwards with
    ag/2.
  • What is the mass apparent weight?

28
Weightlessness
  • Now, if the elevator is in freefall (a-g).
  • What is the mass apparent weight?

29
Weightlessness
  • The weightlessness one experiences in orbit is
    exactly the same one would feel in a freely
    falling elevator.
  • Remember, the Force causing a satellite to orbit
    is the Force of Gravity.in essence, the
    satellite is freely falling.

30
Keplers Laws
  • Keplers laws of planetary motion
  • Empirical (Experimental)
  • Keplers 1st Law The path of each planet around
    the sun is an ellipse with the sun at one focus

a ? semi-major axis b ? semi-minor axis e ?
eccentricity e ? es/a
es
a
b
31
Keplers Laws
  • Keplers 2nd Law Each planet moves so that an
    imaginary line drawn from the sun to the planet
    sweeps out equal areas in equal periods of time

32
Keplers Laws
  • Keplers 3rd Law The ratio of the squares of the
    periods of any two planets revolving around the
    sun is equal to the ratio of the cubes of their
    semi-major axes.

s2
s1
33
Newtons Synthesis
  • Newton was able to derive Keplers experimental
    laws from his Universal Law of Gravity.
  • Perturbations

34
Keplers 3rd Law Circular Orbit
  • Earths orbit around sun has e0.017, almost
    circular. Can we prove Keplers third law for
    circular orbits?

35
Example Problem
  • If we know the Earths distance from the sun, can
    we determine the suns mass from Keplers laws?
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