Center for Astrophysical Research in Antarctica
This is the staff copy of the lab and other brainstorming/reflections.
Before class: prepare a bucket of water with the dye, cover with foil, leave outside in the shade to equilibrate to ambient air temperature. (This will save about 30 minutes of class time).
Introductory discussion: We're experimenting with sunlight, but this activity is really
all about understanding energy.(After discussing their answers to questions): Energy is really a very elusive concept.
A standard definition is something like "Energy is the ability to do work." But this
definition doesn't tell us very much at all: What is work, exactly? How do I know if I
have enough energy available, to do the work I want to do?
I'm not going to give you a precise, general definition for energy. Instead we're just
going to work with some examples of it, and of how you can put the concept to
practical use. Once you've worked with it awhile, you can come up with your own
definition, that makes sense to you. Hopefully, you'll also see how powerful and
useful the concept of energy is. But first a few key points about energy:
This is a difficult concept, so a few examples are needed to show how the concept of energy gives you a common ground for talking about seemingly unrelated things: temperature and velocity, for example, are both involved with energy, though they seem very different things.
Return focus to energy from the sun: what are two things that would be different about earth if we didn't have the sun around? (no light, no heat)...forms of energy.
Energy from sun has to travel through empty space (a lot of space: 90 million miles!!) to get to us. It does this in the form of light (which is another name for radiation). We said before that one way we can tell there is energy flowing is that it will heat something up. So lets go outside and see if it feels like there is heat coming from sunlight...(establish their qualitative understanding of the effect we're going to measure quantitatively: remind them that you can really feel the heat transmitted by sunlight.
Next we need some good way to measure more accurately just how much energy there is: emphasize that number only matters as a standard, so that people uniformly can use that number to figure out what they can do with that energy (boil water, heat their house, power a car, run a computer, etc. ...remember Apollo 13, big problem was to be able to run the equipment they needed with the small amount of energy they had available. Try to lead them into suggesting how to do the measurements, then show them materials for building what THEY have suggested.
This afternoon we're going to build a calorimeter to convert the light from the sun into heat. We'll measure how much the sunlight heats some water, and use that information to figure out how many calories or joules are in the sunlight.
See procedure on student activity sheet for how to build the calorimeter, and carry out the rest of the experiment and data analysis.
Mention that same kind of calorimeter is used in chemistry labs
1) What do you think "energy" is? 2) List some things that require energy to make them work (tools, appliances, games, etc.; any kind of activity that you think requires energy): 3) For each of the things you listed above, try to identify the source of the energy it uses (e.g. a battery,...): 4) List anything you can think of that does NOT require energy to make it work:
I'm not going to give you a precise, general definition for energy. Instead we're just going to work with some examples of it, and of how you can put the concept to practical use. Once you've worked with it awhile, you can come up with your own definition, that makes sense to you. Hopefully, you'll also see how powerful and useful the concept of energy is. But first a few key points about energy:
In order to compare amounts of energy which appear in different forms, we need to set up some standard way of measuring the amount of energy. One convenient way to do this is to use energy in the form of heat as a standard. A common unit of energy is the calorie, which is defined as the amount of energy needed to raise one gram of water by one degree Celsius. Another common unit of energy is the Joule, which is 4.186 calories.
Record the surface area of the top surface of the water in the styrofoam cup: _______ ____________________________________________________________________________ Measure out about 200 ml of dyed water into a styrofoam cup. Be sure to note ACCURATELY how much water you used, and record the volume of water here: volume of water used: ______________________ milliliters Attach the probe of the thermometer so that the tip is about in the middle of the cup, away from the sides or bottom, but well submerged in the water. Secure the probe by taping it to the lip of the cup. Cover the mouth of the cup with plastic wrap (aluminum foil), and secure the cover with tape or a rubber band. Get another styrofoam cup, and cut off the top part of the cup (about 1/2 inch wide). Tape this piece to the top of your original cup, and then attach another layer of plastic wrap (aluminum foil) to the top of this. You should now have a cup full of black water, with a thermometer probe in the water. The opening of the cup should be covered by 2 layers of plastic wrap (aluminum foil), one layer separated from the other by about half an inch. This is your calorimeter, which you will use to record how much energy we are receiving from the sun. Move the calorimeter into the shade outside, and monitor the temperature until it stabilizes, and you observe no temperature change for several minutes. Now go out in the sun and prepare a stand for the calorimeter. Use the cardboard to make a ramp on which the calorimeter will be placed. Push a straight pin into the top surface of the ramp, making sure it is perpendicular to the surface. Adjust the angle of the ramp until the shadow of the pin disappears. This indicates that the sun is shining directly onto the surface of the ramp. You are now ready to begin the real experiment. Attach your calorimeter to the ramp using a bit of the putty. Record the starting time, and the temperature reading on your digital thermometer: starting time: _____________ starting temperature: ___________C Keep monitoring the experiment until the temperature has increased by about 3 C or more. (or until the sun is covered by a cloud!). Record the ending time and temperature. ending time: _____________ ending temperature: ___________C Now we have all the data we need, to figure out how much energy your cup of water absorbed from the sun: First subract the start time from the ending time, and convert to seconds, to get the elapsed time (ET): ET = time(end) - time(start) = ____________ seconds Then subtract the starting temperature from the final temperature, to get the temperature increase (TI) in your water: TI = T(end) - T(start)= ___________ C We learned earlier that for each milliliter of water and for each degree C that bit of water has its temperature raised, 4.186 Joules of energy are needed. So multiply TI by the volume of water you used, and then multiply by 4.186, to find out how many Joules of energy were transferred from the sun, into your water: Total energy transferred = (TI) x (4.186) x (volume of water in ml) = _____________Joules This tells you the total amount of energy that was absorbed over the whole area of the surface of the water, in the roughly 20 minute time period of the experiment. To get the amount that was transferred in each second, over each square cm of surface, you need to do some division: Energy flux = (total energy transferred)/ (surface area) / (elapsed time) = ______________________ Joules/cm2/sec Record here the energy flux values for each of the 4 groups, indicating whether plastic wrap or aluminum foil was used in each case: Find the average of the 2 values obtained from the plastic wrap experiments. This is your final result for the energy flux from sun:
1) The standard value for the "average" amount of energy from the sun which reaches the top of the earth's atmosphere, per second, and per square centimeter, is 0.14 Joules/sec/cm2 . If our value came out higher or lower than this standard number, explain why you think this happened. 2) Why did we make the water black, rather than, say, white? [Hints: 1) Think about what happened in the experiments where the cup was covered with aluminum foil, vs. plastic wrap. 2) What happens to the light that hits a black object, to make it look black? What happens to the light hitting a white object, so that it looks white?] 3) Look at the number you recorded for the TOTAL amount of energy you collected from the sun. (If you did the aluminum foil experiment, use the results from someone who did the plastic wrap experiment). How long could you keep a 60 Watt lightbulb lit with the energy you collected? (A Watt is one Joule per second): What does this tell you about the difficulties in using solar energy as a major power supply?
Questions? Comments? email us at caraweb@astro.uchicago.edu Last modified Thursday, 23-Jul-1998 17:35:43 CDT