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Newton, Einstein and Gravity

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Jupiter's gravity at cloud level: g = 24.5m/s2. Mars' gravity at the ... Speed: how fast your location changes. Velocity: your speed in a certain direction ... – PowerPoint PPT presentation

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Title: Newton, Einstein and Gravity


1
Newton, Einstein and Gravity
  • Chapter 5
  • Do not read section 5-3

2
Gravity is an Acceleration
  • Does not depend on mass.
  • Earths gravity at sea level g 9.81 m/s2
  • Moons gravity at the surface g 1.6 m/s2
  • Jupiters gravity at cloud level g 24.5m/s2
  • Mars gravity at the surface g 3.63 m/s2

3
Momentum and Force
  • Linear Momentum a quantity of motion p mv
    mass x velocity
  • Ex. throwing a baseball vs. throwing a bowling
    ball at same speed.
  • Bowling ball has more momentum at the same speed
  • Force how momentum changes F ma
    mass x acceleration
  • Ex. accelerating an empty storage box vs.
    accelerating a full storage box
  • Empty box takes less force at the same
    acceleration

4
Mass and Weight
  • They are not the same thing.
  • Mass is a property of an object, no matter where
    in the universe it is located. Mass is how much
    stuff?
  • Weight is dependent upon the local gravity (g).
    The Moons gravity is 6 times less on than
    Earths.
  • Weight mg mass x gravity
  • Notice that this is a force (Fma), where a g.

5
Speed, Velocity, Acceleration
  • Speed how fast your location changes
  • Velocity your speed in a certain direction
  • Acceleration how fast velocity changes
  • speed or direction can change
  • You can feel acceleration, but not velocity

6
Newtons Laws of Motion
  • 1st Law An object moves with a constant velocity
    in the absence of a net force.
  • 2nd Law In the presence of a net force, the
    force is how fast your momentum changes, or force
    mass x acceleration.
  • F ma
  • 3rd Law For any force there is an equal and
    oppositely directed reactionary force.

7
Examples
8
Gravitation
  • Newtons Law of Universal Gravitation Masses
    attract each other with a force that is directly
    proportional to their masses and inversely
    proportional to their separation distance.

9
Orbits and Escape Velocity
  • Orbiting the Earth is NOT getting away from
    gravity - it is a constant freefall.
  • If you can go fast enough, you can escape the
    Earths gravitational influence.

10
Freefall and Weightlessness
  • Freefall is when your acceleration is solely due
    to gravity.
  • Exs. Jump from an airplane. Stand in an elevator
    whose cable has been cut.
  • This gives the appearance of having no weight. A
    scale would read zero.

11
Angular Momentum
  • Momentum in circular motion.
  • Includes rotations (spins) and revolutions
    (orbits)
  • L mvr mass x velocity x radius of the circle

12
Newton and Kepler
  • Newtons form of Keplers Third Law Is more
    general than K3, and applies in any situation
    where two masses orbit each other.
  • Ex. Two stars, two galaxies, a star and its
    galactic center, a star and planet, a planet and
    a moon, etc.
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