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Chapter 4: Making Sense of The Universe: Matter, Energy

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Kinetic (motion) - Potential (stored) - Radiative (electromagnetic) ... Kinetic Energy. When mass is moved it is Kinetic Energy (T=1/2 mv2) ... – PowerPoint PPT presentation

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Title: Chapter 4: Making Sense of The Universe: Matter, Energy


1
Chapter 4 Making Sense of The Universe Matter,
Energy Gravity
2
What Is Matter?
  • Matter is the stuff that makes up our things
  • Matter is composed of atoms and their
    constituents
  • These elements combine to form the molecules of
    life
  • Matter has MASS - Mass is an intrinsic property
    of matter

3
What Is Energy?
  • Energy comes in different forms - Kinetic
    (motion)- Potential (stored)- Radiative
    (electromagnetic)
  • Mass can be turned into Energy
  • Energy can become Mass
  • Emc2

4
Matter is composed of atoms
5
  • The Periodic Chart

These elements all have unique chemical
properties, based on the number of protons,
neutrons and electrons they are composed of. If
you add or remove neutrons from the most common
form of an element, you create Isotopes. Strippin
g electrons from an atom is called Ionization.
6
Phases of Matter
  • Solid
  • Liquid
  • Gas
  • Plasma

The state changes as you increase the temperature
(add energy)
7
Atoms Orbits
  • Matter appears solid, but is composed of mostly
    empty space!
  • Electrons orbit atoms in clouds, with higher
    energy electrons in farther orbits

8
Atomic Energy States
9
Potential Energy
  • Potential Energy is the energy something has just
    because it has mass and is where it is
  • Think of a boulder on a hill as an example, when
    it rolls down it turns potential energy into
    Kinetic Energy(Umgh)
  • Simply by having mass that can be turned into
    energy is potential

10
Kinetic Energy
  • When mass is moved it is Kinetic Energy (T1/2
    mv2)
  • Adding energy to a system, i.e. as heat, will
    make the atoms more energetic and they will move
    more, colliding with other atoms this is
    Kinetic Motion
  • Temperature Energy

11
Conservation of Energy
  • In a closed system, the sum total of the energy
    is conserved

12
The UniversalLaws of Motion
13
Motion
  • What is the difference between Speed, Velocity
    Acceleration?
  • Speed is a scalar, that means that it is how fast
    you go, but without specific direction
  • Velocity is a vector, it gives speed and
    direction
  • Acceleration is found when an object is speeding
    up or slowing down

14
Formulae
  • v ?x/ ?t
  • a ?v/ ?t
  • g 9.81 m/s2

15
Mass Momentum
  • Mass is an intrinsic property of matter. The
    atomic mass is invariant, regardless of your
    gravitational field (or speed)
  • Weight is a Force, it changes depending on your
    gravitational field
  • Momentum is mass x velocity, it tells you that
    big-fast things are harder to stop than
    small-slow things.
  • p mv

16
Newtons Laws of Motion
  • First Law An object at rest remains at rest, and
    an object in motion remains in motion, unless
    acted upon by an external force
  • Second Law F ma ?p/ ?tForce depends on rate
    of change of momentum.
  • Third Law For every force, there is an equal and
    opposite force

17
Conservation of Momentum
  • Newtons laws imply the concept of conservation
    of momentum. The total momentum in a system is
    conserved.
  • Angular momentum acts on a body in orbit around
    another, held by the gravitational force. In the
    absence of net torque, the angular momentum
    remains constant.angular momentum mvr

18
Newtons Universal Law of Gravitation
  • Every mass attracts other mass through the force
    called gravity
  • The force of attraction between any two objects
    is directly proportional to the product of their
    masses
  • The force of attraction between two objects
    decreases with the square of the distance between
    their centers
  • Fg GM1M2/d2
  • (note that G is the gravitational constant)

19
Newtons Influence
  • Some 70 years after Kepler published his three
    laws of orbital motion, Newton was able to
    explain why they held true!
  • Science strives to observe, determine
    relationships and eventually discover why
    things work the way they do.
  • Newtons laws remained unchallenged until an
    upstart named Albert Einstein developed a general
    theory of gravity that was more precise in 1905.

20
Gravity Rules!
  • The gravitational influence of the Moon cause the
    tides
  • Leaving the surface of Earth takes a lot of
    energy, it is like crawling out of a deep well.
    The escape velocity is about 40,000 km/hr. (pg
    135)
  • While the other fundamental forces
    (electromagnetic, strong and weak) are much
    stronger, their range is short and the motion of
    the stars and galaxies are bound by gravity.

21
Free Fall
  • Why are astronauts weightless in space?They are
    in a constant state of free fall.The Force from
    gravity in the space station from Earth is not
    much less than on the surface! (p.121)
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