Chapter 5: Problem 11
Explain why astronomers are interested in blackbody radiation.
Chapter 5: Problem 11
Explain why astronomers are interested in blackbody radiation.
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Get started for freeTurn on an electric stove or toaster oven and carefully observe the heating elements as they warm up. Relate your observations to Wien's law and the Stefan-Boltzmann law.
Black holes are objects whose gravity is so strong that not even an object moving at the speed of light can escape from their surface. Hence, black holes do not themselves emit light. But it is possible to detect radiation from material falling toward a black hole. Calculations suggest that as this matter falls, it is compressed and heated to temperatures around \(10^{6}\) K. Calculate the wavelength of maximum emission for this temperature. In what part of the electromagnetic spectrum does this wavelength lie?
Obtain a glass prism (or a diffraction grating, which is probably more readily available and is discussed in the next chapter) and look through it at various light sources, such as an ordinary incandescent light, a neon sign, and a mercury vapor street lamp. Do not look at the sun! Looking directly at the Sun causes permanent eye damage or blindness. Do you have any trouble seeing spectra? What do you have to do to see a spectrum? Describe the differences in the spectra of the various light sources you observed.
For each of the following wavelengths, state whether it is in the radio, microwave, infrared, visible, ultraviolet, X-ray, or gamma-ray portion of the electromagnetic spectrum. Explain your reasoning. (a) \(2.6 \mu \mathrm{m}\), (b) \(34 \mathrm{~m}\), (c) \(0.54 \mathrm{~nm}\), (d) \(0.0032\) \(\mathrm{nm}\), (e) \(0.620 \mu \mathrm{m}\), (f) \(310 \mathrm{~nm}\), (g) \(0.012 \mathrm{~m}\).
What is meant by the frequency of light? How is frequency related to wavelength?
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