Essential Cosmic Perspective
Essential Cosmic Perspective
9th Edition
ISBN: 9780135795033
Author: Bennett
Publisher: PEARSON
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Chapter 5, Problem 41EAP

Group Activity: Which Telescope? You represent a research group that wishes to observe matter around a black hole; assume that the mat-ter is emitting photons at all wavelengths. You have the opportunity to make your observations with one of the following four telescopes:

• A radio telescope, 300 meters in diameter, located in Puerto Rico • An infrared telescope, 2 meters in diameter, on a spacecraft in orbit around Earth and observing at a wavelength of micrometers

• An infrared telescope, 10 meters in diameter, equipped with adaptive optics, located on Mauna Kea in Hawaii and observ-ing at a wavelength of micrometers (10-5 m)

• An x-ray telescope, 2 meters in diameter, located at the South Pole Discuss the pros and cons of each telescope for this observing task, then come to a group consensus in which you rank the four choices from best to worst. Compare your rankings to those of other groups in your class. Note: You may wish to do this activity using the same four roles described in Chapter 1, Exercise 39.

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If a star has a surface temperature of 25,000 K (2.50 ✕ 104 K), at what wavelength (in nm) will it radiate the most energy? nm Is this a cool or hot star? (Give your answer relative to the Sun.) coolhot
a) The star 58 Eridani is a feint but naked-eye star similar to the Sun. Suppose that you are observing this star in the night sky without a telescope. Ignoring any interstellar extinction or atmospheric absorption, approximately how many photons per second arrive at your retina? Show all steps in your calculation. Look up any required information about the star using Wikipedia. Use sensible approximations so your calculation is straightforward. For example you could consider only the region of the spectrum where the photon flux peaks. b) The Mid-Infrared Instrument (MIRI, camera and spectrograph) on the James Webb Space Telescope operates in the band 5 – 28 µm. For 58 Eridani, approximately how many photons per second can be used by this instrument? Assume that MIRI takes all the photons from the full JWST mirror. Show all steps in your calculation. Describe briefly two or three other factors which play a role in determining the sensitivity of an instrument such as MIRI?
Tutorial A molecular cloud has a temperature of 46 K and an HI cloud has a temperature of 135 K. What are their wavelengths of maximum intensity? What frequency do these correspond to? In what region of the electromagnetic spectrum can the radiation from these clouds be found? Part 1 of 3 We can use Wien's Law to determine the wavelength of maximum intensity in nanometers for the molecular cloud. 2.90 x 106 Amc Amc Amc XHI ^HI = AHI = We can use Wien's Law again to determine the wavelength of maximum intensity in nanometers for the HI cloud. 2.90 x 106 II = K nm = μm K nm um

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