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Physics 1710 Chapter 14 The Theory of Gravity

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If one pulls on the thread, which way will the spool roll, if the thread comes ... Fact: a moon circling a planet has an acceleration of a = v 2 /r. Fact: a = F/m. ... – PowerPoint PPT presentation

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Title: Physics 1710 Chapter 14 The Theory of Gravity


1
Physics 1710Chapter 14 The Theory of Gravity
  • Quiz
  • Consider a spool of thread. If one pulls on
    the thread, which way will the spool roll, if the
    thread comes over the top or under the bottom of
    the spool?

2
Physics 1710Chapter 14 The Theory of Gravity
  • Quiz
  • What is the mass of the earth?
  • How do you know?

3
Physics 1710Chapter 14 The Theory of Gravity
  • 1' Lesson
  • The force of attraction between two bodies with
    mass M and m respectively is proportional to the
    product of their masses and inversely
    proportional to the distance between their
    centers squared.
  • The proportionality constant in the Universal
    Law of Gravitation G is equal to 6.673 x 10 11 N
    m2 /kg2 .
  • The gravitational force constant g is equal to
  • G M/(Rh) 2, R is the radius of the planet.

4
Physics 1710Chapter 14 The Theory of Gravity
  • 1' Lesson
  • Keplers Laws
  • The orbits of the planets are ellipses.
  • The areal velocity of a planet is constant.
  • The cube of the radius of a planets orbit
  • is proportional to the square of the period.
  • The gravitation field is the force divided by
    the mass.
  • The gravitation potential energy for a point mass
    is proportional to the product of the masses and
    inversely proportional to the distance between
    their centers.

5
Physics 1710Chapter 14 The Theory of Gravity
  • 1' Lesson
  • The total energy of a gravitationally bound
    system is equal to the sum of the kinetic energy
    and (negative) gravitational potential energy.
  • The escape velocity of an object projected
    upwards from the surface of the Earth is the
    velocity with a kinetic energy just equal to the
    gravitational kinetic energy of the particle at
    the radius of the Earth.

6
Physics 1710Chapter 14 The Theory of Gravity
  • Isaac Newtons
  • Universal Law of Gravitation
  • F - G M m/ r 2

7
Physics 1710Chapter 14 The Theory of Gravity
  • How did he discover this?
  • Fact a moon circling a planet has an
    acceleration of a v 2 /r
  • Fact a F/m.
  • Fact Kepler had found that the square of the
    period was proportional to the cube of the
    radius
  • T 2 k r 3 .
  • Thus
  • v 2? r / T

8
Physics 1710Chapter 14 The Theory of Gravity
  • And
  • T 2 (2? r) 2 /(F r /m) k r 3
  • Thus
  • F (2?) 2 m/(k r 2 )
  • An inverse square law. k 1/ (2?) 2 (G M)
  • F G Mm/ r 2 ,
  • But what value is G?

9
Physics 1710Chapter 14 The Theory of Gravity
  • Henry Cavendish
  • And the
  • Cavendish Experiment

10
Physics 1710Chapter 14 The Theory of Gravity
  • G 6.673 x 10-11 N ?m 2 /kg 2
  • G 2/3 x 10-10 N ?m 2 /kg 2
  • (to an accuracy of 0.1)

11
Physics 1710Chapter 14 The Theory of Gravity
  • Keplers Laws
  • The orbits are ellipses. (Contrary to Aristotle
    and Ptolemy.)
  • A central force F ? 1/ r 2 or r 2
  • The areal velocity is a constant.
  • Angular momentum is conserved
  • ½ v r ?t constant implies that
  • rmv L constant.
  • T 2 ? r 3 implies F ? 1/ r 2, only.

12
Physics 1710Chapter 14 The Theory of Gravity
  • Gravitation Field
  • g Fg / m
  • At the surface of the Earth g 9.80 N/ kg.

13
Physics 1710Chapter 14 The Theory of Gravity
  • Gravitational Potential Energy
  • U -? Fd r
  • U -? G Mm / r 2 d r
  • U GMm / r
  • U 0 as r ?8

14
Physics 1710Chapter 14 The Theory of Gravity
  • Total Energy
  • for Gravitationally Bound Mass
  • E K U
  • E ½ m v 2 - GMm/ r
  • E L2 /2mr 2 GMm/ r
  • One dimensional plot.
  • Bound orbit if E 0.
  • E - GMm/2r

15
Physics 1710Chapter 14 The Theory of Gravity
  • Escape Velocity
  • If K is such that E gt 0, then
  • K ½ m v 2 GMm/ r
  • Thus
  • v v 2GM/R

16
Physics 1710Chapter 14 The Theory of Gravity
  • Summary
  • The force of attraction between two bodies with
    mass M and m respectively is proportional to the
    product of their masses and inversely
    proportional to the distance between their
    centers squared.
  • F - G M m/ r 2
  • The proportionality constant in the Universal
    Law of Gravitation G is equal to 6.673 x 10 11 N
    m2 /kg2 .

17
Physics 1710Chapter 14 The Theory of Gravity
  • Summary
  • The gravitational force constant g is equal to
  • G M/(Rh) 2, R is the radius of the planet.
  • Keplers Laws
  • The orbits of the planets are ellipses.
  • The areal velocity of a planet is constant.
  • The cube of the radius of a planets orbit
  • is proportional to the square of the period.
  • The gravitation field is the force divided by
    the mass.
  • g Fg / m

18
Physics 1710Chapter 14 The Theory of Gravity
  • Summary
  • The gravitation potential energy for a point
    mass is proportional to the product of the masses
    and inversely proportional to the distance
    between their centers
  • U GMm / r
  • The escape velocity is the minimum speed a
    projectile must have at the surface of a planet
    to escape the gravitational field.
  • v v 2GM/R
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