Day 56: Heat Engine Lab

Today we use PASCO Heat Engine Apparatus to do useful work using internal energy. First, we tried the cycle a few times, working out the kinks in the procedure. Then, we drew pV diagrams, explaining why we thought each transition is adiabatic, isothermal, isobaric, or isochoric. Then we came up with a formula for the volume as a function of the height of the piston. Then it was time to get quantitative and take data. We then calculated the net work done two ways--by the pV diagram and by the change in gravitational potential energy. We got some great results!
We then talked a little about entropy. We defined microstates and macrostates and talked about how the entropy of the universe is increasing.

Day 55: Whiteboard Speed Dating with the Ideal Gas Model

Today was 100 minutes of pure whiteboard speed dating. I only changed the groups about every 7 or 8 minutes, but the problems were long and complex enough that we still got through two or three "dates" per problem. All the problems were old AP Physics B ideal gas problems, which worked out really well. These problems really helped students talk about how the internal energy, the work done, and the heat exchanged, the temperature change, and the volume change are interrelated.

Day 54: Quantifying Energy in a Gas

We quantified the work done by a gas by looking at the pressure-volume graph, which was easy. We quantified the internal kinetic energy of the gas, which was much harder. The metaphor we used was that of the Koopa Troopa, the Mario turtle that, if you step on it, can bounce back and forth from wall to wall at the same speed forever. It's a good model of many, many elastic collisions even if it isn't realistic. It does require some handwaving to get the derivation, but we know have an expression for the kinetic energy of one molecule of a gas. It also allowed us to explain why there's not much hydrogen gas in our atmosphere.

We then previewed the heat engine lab. We have a lot of practice to do before we get to that lab.

Day 53: Tracking Energy in Ideal Gases

We practicing tracking the energy going into and out of an ideal gas. We practiced the four types of transitions that can happen: isobaric, isovolumetric, isothermal, and adiabatic. Adiabatic is my favorite. We also did Super LOL diagrams, which, if you don't know about, you should read this blog post

We also talked about the first law of thermodynamics, which is pretty obvious if you understand the LOL diagrams. We know that work in and out is related to volume, but we're not sure exactly how, and we know internal energy is related to temperature, but we're not sure how, but I guess that's what tomorrow is for.

Day 52: Extending the Ideal Gas Model

We practiced the ideal gas model today by whiteboarding a few problems that were more difficult than they first appeared. We had to take a little detour over to air pressure and how it is everywhere. It's always fun to play with suction cups. We practiced drawing pressure-volume graphs to describe what's happening to the gas, and started drawing energy bar charts (LOL diagrams) for ideal gases.

It turns out there's only two ways to put energy into a gas: compression and heating the gas. And there's only two ways to take energy out of a gas: expansion and heating the environment. The energy of the gas, for our monatomic ideal gas model, is only translational kinetic energy, so we only need bars in the L's of the LOL for kinetic energy. Now it's time to classify all the different changes a gas can undergo.

Day 50: Reviewing the Ideal Gas Model

How can we extend mechanics? Well, the ideal gas model seems to make sense. According to the kinetic theory of gases, we can model it as a whole lot of particles that collide elastically, and we know about elastic collisions. Everyone takes chemistry before this class, so everyone has seen the ideal gas model, but we still played with the PHeT simulation of gas properties to have that visual of our model. We also talked about the transfer of internal energy, or heating, that can happen, through conduction, convection, and radiation.