Astronomy
Astronomy
1st Edition
ISBN: 9781938168284
Author: Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher: OpenStax
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Chapter 6, Problem 23E

Radio astronomy involves wavelengths much longer than those of visible light, and many orbiting observatories have probed the universe for radiation of very short wavelengths. What sorts of objects and physical conditions would you expect to be associated with emission of radiation at very long and very short wavelengths?

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Radio astronomy involves wavelengths much longer than those of visible light, and many orbiting observatories have probed the universe for radiation of very short wavelengths. What sorts of objects and physical conditions would you expect to be associated with emission of radiation at very long and very short wavelengths? (Select all that apply.) very long wavelengths cold cold gas cosmic background radiation nuclear reactions ++ Opulsars solar corona very high-energy processes very short wavelengths cold gas cosmic background radiation nuclear reactions pulsars solar corona very high-energy processes
Voyager 2. When the Voyager 2 spacecraft was approaching towards its Neptune encounter in 1989, it was 4.5 × 10° km away from the earth. Its radio transmitter, with which it communicated with us (and we communicated with it), broadcast with a mere 22 Watt of power at the S-band (2.1 GHz). (Your home wi-fi router emits around 2 Watt at 2.4 GHz wi-fi band). Assuming the Voyager transmitter broadcast equally in all directions, (a) What signal intensity was received on the earth? (b) What electric and magnetic field amplitudes were detected? (c) How many 2.1 GHz photons were arriving per second on a radio-receiver antenna with a circular cross-section of diameter 34 meters? Two counter-propagating plane waves (a) Let E(z, t) = E0 cos(kz – wt)â + E, cos(kz + wt)x. Write E(z, t) in simpler form and find the associated magnetic field. (b) For the fields in part (a), find the instantaneous and time-averaged electric and magnetic field energy densities. (c) Let E(z, t) = E, cos(kz – wt)x + E,…
Infrared radiation from the center of our galaxy with a wavelength of about 2 μm (2 × 10-6 m) comes mainly from cool stars. Use this wavelength as Amax and find the temperature of the stars.

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