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Classical Gravity

  • A2-13: ELLIPSE DRAWING BOARD

    A2-13
    Demonstrate one method of drawing ellipses
    The ends of a string loop are hooked around two pegs on the board and kept tight by the chalk holder. Moving the string around one complete turn produces an ellipse. This procedure creates the locus of points where R1 + R2 = Constant, the equation for an ellipse. Changing the peg position changes the eccentricity of the ellipse.

    Consider inviting students to make predictions about how the shape of the ellipse will change in response to changing the foci in different ways. This can be related to a variety of mathematical and astronomical phenomena.

    FS2
  • E1-01: CAVENDISH EXPERIMENT - MODEL

    E1-01
    Aid in describing the Cavendish experiment.
    The black (steel) balls are temporarily rigidly fixed in space. A steel barbell is mounted to a stiff wire on the axis of the barbell with a small mirror attached to the wire just above the barbell. Light reflects off the mirror, indicating the oscillations of the barbell. This models how, in the full experiment, the equilibrium position for oscillations of the barbell would show the displacement corresponding to the gravitational force between the two pairs of balls, and is observed by noting the movement of the light reflected off the mirror.
    FS2, LS1
  • E1-11: POTENTIAL WELL -MODEL

    E1-11
    Demonstrates motion of planets or satellites in an inverse square gravitational field

    Giving a small ball a tangential velocity near the outer radius of the well, one can create elliptical orbits which demonstrate conservation of angular momentum as the ball rolls around the well.

    Invite students to predict how changing the ball’s starting velocity (in magnitude or direction) will affect its path. This is a good opportunity for one or more student volunteers to participate.

    Background

    The surface of this “potential well" is shaped so as to model an inverse square gravitational force. When a ball enters the well enters the well, it is attracted to the center; if it has no initial velocity, it will fall directly to the center. But if it enters with some velocity tangential to the center, it will fall into an elliptical orbit that gradually decays to the center as the ball rolls around the well.

    When you roll the ball across the surface, you use some initial force to start it moving. Once it is rolling on its own, though, the only forces acting on it are the force of gravity, pulling downwards, and the normal force and frictional force of the surface holding it up. So the ball accelerates as it rolls down the surface, exchanging potential energy for kinetic energy, until it falls into the hole.

    FS1, E1
  • E1-12: MARBLE IN GLASS BOWL

    E1-12
    Demonstrate orbits in a gravitational potential well.
    Start the marble rolling tangentially in the bowl to obtain an orbit, then observe the effects of conservation of angular momentum.
    E1, I6