Take the Astra 2E satellite and the TLE set of Nov 2; you may model the satellite as one flat plate, taking only solar panels into account; look up the appropriate values. At 4pm UTC, choose the point on the Earth, which has the Astra 2E in the zenith at that time. Assume the Sun is an extended source!. Assume your telescope has an aperture with diameter 1 meter, a secondary mirror with diameter 6cm, a quantum efficiency of 65%, a loss function of 80%, and a pixel scale of 1 arcseconds per pixel, and you choose an integration time of 5 seconds. You can use 600nm as a mean wavelength. (a) Where is your station located? (b) What is the magnitude of the object at your station?

Principles of Heat Transfer (Activate Learning with these NEW titles from Engineering!)
8th Edition
ISBN:9781305387102
Author:Kreith, Frank; Manglik, Raj M.
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Chapter11: Heat Transfer By Radiation
Section: Chapter Questions
Problem 11.11P
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For the sation location, the question says "At 4pm UTC, choose the point on the Earth, which has the Astra 2E in the zenith at that time". Does that mean the station is directly beneath the satellite? Does that give a hint to its location?

Take the Astra 2E satellite and the TLE set of Nov 2; you may model the satellite as one flat
plate, taking only solar panels into account; look up the appropriate values. At 4pm UTC,
choose the point on the Earth, which has the Astra 2E in the zenith at that time. Assume the
Sun is an extended source!. Assume your telescope has an aperture with diameter 1 meter, a
secondary mirror with diameter 6cm, a quantum efficiency of 65%, a loss function of 80%,
and a pixel scale of 1 arcseconds per pixel, and you choose an integration time of 5 seconds.
You can use 600nm as a mean wavelength.
(a) Where is your station located?
(b) What is the magnitude of the object at your station?
Transcribed Image Text:Take the Astra 2E satellite and the TLE set of Nov 2; you may model the satellite as one flat plate, taking only solar panels into account; look up the appropriate values. At 4pm UTC, choose the point on the Earth, which has the Astra 2E in the zenith at that time. Assume the Sun is an extended source!. Assume your telescope has an aperture with diameter 1 meter, a secondary mirror with diameter 6cm, a quantum efficiency of 65%, a loss function of 80%, and a pixel scale of 1 arcseconds per pixel, and you choose an integration time of 5 seconds. You can use 600nm as a mean wavelength. (a) Where is your station located? (b) What is the magnitude of the object at your station?
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