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MATERIALS and WORKSHEET:
Worksheet:
DIRECTIONS: Part 1
Part 2
Part 3
Part 4
Measurement & Prediction ExtensionsYou might want to add two extensions to this activity if working with older or more advanced students. One extension involves having students make predictions about results before trying each setup. A second extension involves having the students make measurements of the distances between the magnets.
BACKGROUND INFORMATION: Your students need to realize that magnets have two poles (North and South) to understand this activity. They need to know that like poles (N and N or S and S) repel each other, and that opposite poles (N and S) attract each other. The poles on the disk magnets are on the flat sides. Image one of the disk magnets is a coin (with a hole in the middle!). Heads is North, tails is South (or vice versa - but the point is that the flat sides are the poles). In Step 2 of Part 1 of the activity (see Figure 1), two like poles are facing each other, so the magnets repel each other. The magnetic force between the two magnets pushes the top magnet upward, preventing it from sliding down on top of the bottom magnet. The force of gravity pulls down on the top magnet, preventing it from flying up off the top of the post. So in Step 3, the two forces at play are gravity (pulling down) and magnetism (pushing up). The two forces are at equilibrium (they "balance out" each other), causing the top magnet to levitate a few cenimeters above the bottom magnet. In Step 4, students will discover that the top magnet undergoes a damped oscillation (it bounces up and down for a while, but eventually stops) when they press down and release the magnet. Oscillations are very common phenomena in both natural and human-made systems. This is a damped oscillation because it doesn't just go on forever; friction between the magnet and the post stops it pretty quickly. Ask your students to mentions systems they are familiar with that behave similarly; a good example is the suspension of a car when it hits a bump. In Step 4 of Part 3 (Figure 4), the middle magnet (B) should be closer to the bottom magnet (A) than it was in the case shown in Figure 1. The weight of the top magnet (C) is pushing down on the middle magnet (B). The magnetic repulsion that keeps A and B apart was just holding up the weight of one magnet in Figure 1; it is holding up the weight of two in Figure 4; so magnet B "rides" lower. Note that this is comparable to the case in Figure 3; the position of the middle magnet is a consequence of having the weight of two magnets pressing down on it. This is more obvious in Figure 3, where the top two magnets are touching, than in Figure 4, where the force of the weight of the top magnet is not pressing down on the middle magnet via direct contact; instead, the weight (force) of the top magnet is "pressing" down on middle magnet via the magnetic repulsion force between the two magnets. When the students bounce the magnets in the Figure 4 setup, the damped oscillatory motion will be similar to the Figure 1 case, though a little more complex. The "bouncing" probably won't last a noticeably longer or shorter time. If anything, the bouncing should stop more quickly in the Figure 4 setup.. The forces in the Figure 4 case are quite interesting. If we assume that the top side of magnet A is a North, then the bottom side of B is a North as well (so the two repel). That means the top of B is a South, and thus the bottom of C is also South. So A and C are actually pulling on each other a little bit. The North top of A "sees" the South bottom of C and is attracted to it (even with B in between). The force is quite small since the magnets are a ways apart. However, the distance from A to C is a little less because of this slight effect. The change is almost certainly not noticeable to the eye, and probably cannot be measured in this simple setup. It is a good puzzle to test your brighter students with, however. In Step 7 of Part 3 this relationship plays out when we remove the middle magnet (B) and A and C stick together. In Step 2 of Part 4, the magnets should end up with a spacing something like that shown in Figure 5. The bottom magnets (A and B) should be closest together; the top two (D and E) furthest apart. Magnet B "feels" its own weight plus the weight of the three magnets above it pushing down; it only has the force of one magnet (A) pushing up on it. Gravity wins out, with a score of four to one. Magnet C "feels" the downward weight of three magnets (itself plus D and E), and the upward repulsive magnetic force from the magnet directly below it (B). So the score is three down to one up, and C "floats" a little higher above B than B does above A. And so on up the stack. There are other minor attractive magnetic forces at play, as described above for the case of Figure 4; but they are much smaller effects and not readily noticeable (if at all). What happens when you "bounce" the five-magnet system? Hopefully, the students should notice that the bouncing stops (damps out) more quickly than in the figure 1 case. More complex systems (with more "degrees of freedom") tend to be harder to keep oscillating that simple systems with fewer parts. There are exceptions, but in general if you "wiggle" a complex structure it will tend to damp out pretty quickly, whereas a simple structure might continue oscillating for a longer time. Figures 2 & 3 illustrate the setups for Part 2. In each case we are combining two or more magnets to increase the magnetic force. When we put two on the bottom and one on top (Step 3, Figure 2), the top magnet "floats" higher (than when just one is on the bottom). The weight of the single top magnet is countered by a greater upward force from two magnets pushing upward together from below. In Step 7 (Figure 3), the magnetic force pushing up is the same as in Figure 2, but the weight on the top is doubled, so the gap between is smaller than in Figure 2. RELATED SECTIONS OF THE WINDOWS TO THE UNIVERSE WEBSITE: References & Background Information: Last modified March 16, 2005 by Randy Russell. The source of this material is Windows to the Universe, at http://www.windows.ucar.edu/ at the University Corporation for Atmospheric Research (UCAR). © 2005 University Corporation for Atmospheric Research. All Rights Reserved. |