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Telescopes and Detectors |
1. | Compare the light-gathering power of the five meter mirror of the Palomar telescope to that of the human eye. (Assume a pupil size of five millimeters.) |
2. | Most of Galileo's telescopes were only about 2 centimeters in diameter. What is the resolving power of such a telescope? How does this compare to the human eye? (The eye's resolution is about 60 arc sec.) |
3. |
Use the Fourmilab Earth Viewer to view the Earth from
the COBE satellite:
Use the information on this viewer to plot the orbit of COBE over the surface for several successive revolutions (the period is 103 minutes). Update the browser window every 5 minutes, and plot a point on a latitude and longitude map of the Earth and write beside the point the altitude. On the same map, plot simultaneously the position of the Sun (the viewer at
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4. |
Repeat exercise 3, but for the Hubble Space Telescope:
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5. | What is the corresponding frequency in megaherz for the 21 cm hydrogen line? |
6. | Why is it important for an observatory to be located in a high and dry place if it is to be used for IR observations? |
7. | Telescopes used to observe the Sun from the Earth are seldom larger than about 50 cm (mirror diameter). Why not build larger ones? |