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Optical Powers
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Think Before You Experiment:
We can think of telescopes as light funnels, gathering light over a large area and focusing or directing it into a smaller area. In the same way funnels are not much good without a container, the telescope needs something to catch the light it gathers. Usually, we think of a person standing at the end of a telescope. In this case their eye is acting as the light detector, sensing the light coming down the funnel. Your eye sends continuous signals to your brain about the light it is receiving. Your brain interprets the information it receives. The result is you see the light.
More and more often, astronomers are replacing the human eye light detector with a CCD camera. The CCD has the advantage over our eyes of being able to collect light over different periods of time. So, the CCD not only acts as a light detector but also a light bucket. Just as a bucket can collect and store different amounts of water, a CCD camera can collect and store different amounts of light before sending it off to a computer to be analyzed. Astronomers vary the amount of light collected and stored by the CCD by changing the amount of time light is allowed to enter the camera (the funnel is allowed to fill the bucket). EXPOSURE TIME refers to how long the camera is allowed to receive light.
Problem – How do variations in exposure time affect the image we get from a telescope?
The Experiment –
Designing an experiment to find out the answer to this problem depends upon taking a series of images of the same object in the sky on the same night with the same telescope and CCD camera while changing only the exposure time. There are several image sets of different types of object. Each image in the set has a different exposure time. All of these images were taken with the full aperture of the 24 inch telescope at University of Chicago's Yerkes Observatory.
Prediction/hypothesis – It is time for you to make a prediction and write out a hypothesis that addresses the problem. Use as much detail as you can. If you think the image will change in some way, describe how much. There are several image sets. Think about possible differences between objects.
Image Sets –

Although your teacher may assign a specific set of images, we recommend that you study as many sets as you have time.
There are many image sets for this activity. You may work with as many as you have time. As you work with each new image or set of images, record your conclusions about exposure time and note the evidence for your ideas. Click here to see a preview of more of the images.
Analyze the Images and Record Data –
Record your observations and measurements.
Hints: Pay attention to the Min/Max values. Use the HOU aperture tool to measure
starlight. Check out the values for the Sky (brightness of the background). Are there any comparisons you can make
between the different objects at the same exposure? Consider using a
spreadsheet and graphing tools to organize and present your results. Use the HOU Image Processing Tips and
Tricks if you need help.
Conclusions – Look carefully at your results.