Swings and the flying trapeze are examples of one of the classic problems of physics: the pendulum. Hanging a weight from a string and making it swing may be very simple, but the pendulum is a classic example of a nonlinear oscillator, and it is actually impossible to solve its exact motion analytically (but quite easy on a computer) . However, application of conservation of energy allows us to get some important answers without having to know the details. (Image courtesy of the San Francisco School of Circus Arts.)
Gravitational potential energy keeps track of work you do against gravity. For instance, when you bike up a hill, you are probably going quite slow at the top after working very hard to get there. What did all that work do for you? Was it wasted? Some of it was, the work you did against friction that went into heating your gears, bearings and even the tires. But a lot of the work didn't go into friction. It went into getting you up the hill, and we say that it got stored in gravitational potential energy. How do you convert it into kinetic energy? By coasting downhill again, of course.
The concept of work was introduced in the skidmarks chapter: if you move a distance d against a force F you do work W = Fd. Gravitational potential energy just keeps track of the work you do against gravity in going up a hill. Since the force of gravity is mg downward (where m is the mass and g = 9.8 m/s²), the work you do against gravity by rising a height h is mgh. So, labeling vertical position with y, we get the formula for gravitational potential energy:
U = mgy
It doesn't matter where you set y = 0, because it's only changes in U and therefore y that count.An important note: we don't talk about potential energy associated with work done against friction. Friction is a nonconservative force: it's very hard to recover kinetic energy from work that you do against friction. Gravity, on the other hand, is a conservative force: you can recover ALL of the work done against gravity back into kinetic energy. Potential energy is used to keep track of work done against conservative forces.
At the top, the mass is at rest, so its kinetic energy K is zero. Let's set y = 0 to be at the bottom of the swing. The mass is released at a height y = h, so it has gravitational potential energy U = mgh. The basic idea is that total energy is conserved:
E = U + K = constant = mgh
As the mass swings down, it picks up as much kinetic energy as the potential energy it loses. One can therefore calculate K at any height. At the bottom of the swing, U = 0, so K = mgh, which can be solved for v using K = ½mv²:
v =
2gh
is independent of
starting height (called amplitude):
=
2
g/l
Normalized swing period vs starting angle for a pendulum.
= 2
g/l
Sam Hokin / samh@fusion.kth.se