Deck 4: Light and Telescopes
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Deck 4: Light and Telescopes
1
Which of the following photons carry the least amount of energy?
A) a blue photon of the visible spectrum, whose wavelength is 450 nm
B) an infrared photon, whose wavelength is 10-5 meter
C) a red photon in the visible spectrum, whose wavelength is 700 nm
D) a microwave photon, whose wavelength is 10-2 meter
A) a blue photon of the visible spectrum, whose wavelength is 450 nm
B) an infrared photon, whose wavelength is 10-5 meter
C) a red photon in the visible spectrum, whose wavelength is 700 nm
D) a microwave photon, whose wavelength is 10-2 meter
a microwave photon, whose wavelength is 10-2 meter
2
How does the speed of light traveling through a medium (such as air or glass)compare to the speed of light in a vacuum?
A) It is the same as the speed of light in a vacuum.
B) It is always less than the speed of light in a vacuum.
C) It is always greater than the speed of light in a vacuum.
D) Sometimes it is greater than the speed of light in a vacuum, and sometimes it is less, depending on the medium.
A) It is the same as the speed of light in a vacuum.
B) It is always less than the speed of light in a vacuum.
C) It is always greater than the speed of light in a vacuum.
D) Sometimes it is greater than the speed of light in a vacuum, and sometimes it is less, depending on the medium.
It is always less than the speed of light in a vacuum.
3
A red photon has a wavelength of 650 nm.An ultraviolet photon has a wavelength of 250 nm.The energy of an ultraviolet photon is ________ than a red photon.
A) 2.6 times larger
B) 6.8 times larger
C) 2.6 times smaller
D) 6.8 times smaller
A) 2.6 times larger
B) 6.8 times larger
C) 2.6 times smaller
D) 6.8 times smaller
2.6 times larger
4
If the wavelength of a beam of light were to double,how would that affect its frequency?
A) The frequency would be four times larger.
B) The frequency would be two times larger.
C) The frequency would be two times smaller.
D) The frequency would be four times smaller.
E) There is no relationship between wavelength and frequency.
A) The frequency would be four times larger.
B) The frequency would be two times larger.
C) The frequency would be two times smaller.
D) The frequency would be four times smaller.
E) There is no relationship between wavelength and frequency.
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5
The part of the human eye that acts as the detector is the:
A) retina.
B) pupil.
C) rods.
D) cones.
A) retina.
B) pupil.
C) rods.
D) cones.
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6
Using the figure below,which type of electromagnetic wave has a wavelength of approximately 10-⁵ meter? 
A) X-rays
B) infrared
C) microwave
D) radio

A) X-rays
B) infrared
C) microwave
D) radio
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7
The speed of light in a vacuum is:
A) 300,000 m/s.
B) 300,000 mph.
C) 300,000 km/s.
D) 300,000,000 mph.
E) infinite.
A) 300,000 m/s.
B) 300,000 mph.
C) 300,000 km/s.
D) 300,000,000 mph.
E) infinite.
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8
What are two properties shared between the eye and all other astronomical detectors?
A) integration time and wavelength sensitivity
B) quantum efficiency and integration time
C) wavelength sensitivity and signal strength
D) quantum efficiency and signal strength
A) integration time and wavelength sensitivity
B) quantum efficiency and integration time
C) wavelength sensitivity and signal strength
D) quantum efficiency and signal strength
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9
As wavelength increases,the energy of a photon ________ and its frequency ________.
A) increases; decreases
B) increases; increases
C) decreases; decreases
D) decreases; increases
A) increases; decreases
B) increases; increases
C) decreases; decreases
D) decreases; increases
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10
Which formula denotes how the speed of light is related to its wavelength and frequency?
A) c = lf
B) c = l/f
C) c = f/l
D) c = 1/lf
A) c = lf
B) c = l/f
C) c = f/l
D) c = 1/lf
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11
Before CCDs were invented,what was the device most commonly used for imaging with optical telescopes?
A) Polaroid cameras
B) photographic glass plates
C) high-speed film
D) video cameras
A) Polaroid cameras
B) photographic glass plates
C) high-speed film
D) video cameras
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12
Light with a wavelength of 600 nm has a frequency of:
A) 5.0 × 106 Hz.
B) 5.0 × 1014 Hz.
C) 5.0 × 1011 Hz.
D) 2.0 × 1015 Hz.
A) 5.0 × 106 Hz.
B) 5.0 × 1014 Hz.
C) 5.0 × 1011 Hz.
D) 2.0 × 1015 Hz.
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13
The speed of light was first determined by which scientist?
A) Galileo
B) Rømer
C) Kepler
D) Newton
E) Einstein
A) Galileo
B) Rømer
C) Kepler
D) Newton
E) Einstein
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14
The fact that the speed of light is constant (as it travels through a vacuum)means that:
A) photons with longer wavelengths have lower frequencies.
B) radio wave photons have shorter wavelengths than gamma-ray photons.
C) X-rays can be transmitted through the atmosphere around the world.
D) All of the above are true.
A) photons with longer wavelengths have lower frequencies.
B) radio wave photons have shorter wavelengths than gamma-ray photons.
C) X-rays can be transmitted through the atmosphere around the world.
D) All of the above are true.
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15
Which of the following lists different types of electromagnetic radiation in order of increasing wavelength?
A) radio waves, infrared, visible, ultraviolet, X-rays
B) gamma rays, ultraviolet, visible, infrared, radio waves
C) gamma rays, X-rays, infrared, visible, ultraviolet
D) X-rays, infrared, visible, ultraviolet, radio waves
E) radio waves, ultraviolet, visible, infrared, gamma rays
A) radio waves, infrared, visible, ultraviolet, X-rays
B) gamma rays, ultraviolet, visible, infrared, radio waves
C) gamma rays, X-rays, infrared, visible, ultraviolet
D) X-rays, infrared, visible, ultraviolet, radio waves
E) radio waves, ultraviolet, visible, infrared, gamma rays
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16
The light-year is a unit of:
A) time.
B) distance.
C) speed.
D) energy.
A) time.
B) distance.
C) speed.
D) energy.
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17
Using the figure below,which type of electromagnetic wave has a frequency of approximately 3 × 10¹⁷ Hz? 
A) X-rays
B) infrared
C) microwave
D) radio

A) X-rays
B) infrared
C) microwave
D) radio
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18
The Voyager 1 spacecraft is currently 16.5 billion km from Earth and heading out of our Solar System.How long does it take radio messages from Voyager 1 to reach us?
A) 1.5 days
B) 15 hours
C) 1.5 weeks
D) 15 minutes
A) 1.5 days
B) 15 hours
C) 1.5 weeks
D) 15 minutes
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19
How do the wavelength and frequency of red light compare to the wavelength and frequency of blue light?
A) Red light has a longer wavelength and higher frequency than does blue light.
B) Red light has a longer wavelength and lower frequency than does blue light.
C) Red light has a shorter wavelength and higher frequency than does blue light.
D) Red light has a shorter wavelength and lower frequency than does blue light.
A) Red light has a longer wavelength and higher frequency than does blue light.
B) Red light has a longer wavelength and lower frequency than does blue light.
C) Red light has a shorter wavelength and higher frequency than does blue light.
D) Red light has a shorter wavelength and lower frequency than does blue light.
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20
Which properties of light changes in a refractive medium?
A) wavelength
B) frequency, speed, and wavelength
C) wavelength and speed
D) speed
A) wavelength
B) frequency, speed, and wavelength
C) wavelength and speed
D) speed
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21
The angular resolution of a ground-based telescope is usually set by:
A) diffraction.
B) refraction.
C) the focal length.
D) atmospheric seeing.
A) diffraction.
B) refraction.
C) the focal length.
D) atmospheric seeing.
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22
The major advantage CCDs have over other imaging techniques is that:
A) they have a higher quantum efficiency.
B) they have a linear response to light.
C) they yield output in digital format.
D) they operate at visible and near-infrared wavelengths.
E) All of the above are true.
A) they have a higher quantum efficiency.
B) they have a linear response to light.
C) they yield output in digital format.
D) they operate at visible and near-infrared wavelengths.
E) All of the above are true.
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23
The angular resolution of the largest single-dish radio telescope in the United States,the 100 m Green Bank Telescope,is closest to________ when it operates at a wavelength of 20 cm.
A) 0.6°
B) 0.6 arcmin
C) 0.6 arcsec
D) 6 arcsec
A) 0.6°
B) 0.6 arcmin
C) 0.6 arcsec
D) 6 arcsec
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24
The most important improvement that photography provides over naked-eye observations is:
A) it is possible to observe a larger field of view with photographic plates.
B) the quantum efficiency is higher for photographic plates.
C) the image resolution is much better for photographic plates.
D) it is possible to detect fainter objects with the use of photographic plates.
A) it is possible to observe a larger field of view with photographic plates.
B) the quantum efficiency is higher for photographic plates.
C) the image resolution is much better for photographic plates.
D) it is possible to detect fainter objects with the use of photographic plates.
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25
Arrays of radio telescopes can produce much better resolution than single-dish telescopes because they work based on the principle of:
A) reflection.
B) refraction.
C) diffraction.
D) interference.
A) reflection.
B) refraction.
C) diffraction.
D) interference.
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26
The light-gathering power of a 4-meter telescope is ________ than that of a 2-meter telescope.
A) 8 times larger
B) 4 times larger
C) 16 times smaller
D) 2 times smaller
A) 8 times larger
B) 4 times larger
C) 16 times smaller
D) 2 times smaller
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27
The 305-meter Arecibo radio telescope in Puerto Rico has a resolution that is closest to that of:
A) the Hubble Space Telescope (0.1 arcsec).
B) a human eye (1 arcmin).
C) the Chandra X-ray Telescope (0.5 arcsec).
D) a 1-meter optical telescope (1 arcsec).
A) the Hubble Space Telescope (0.1 arcsec).
B) a human eye (1 arcmin).
C) the Chandra X-ray Telescope (0.5 arcsec).
D) a 1-meter optical telescope (1 arcsec).
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28
As a beam of light travels from one medium to another,the change in direction of the beam of light depends on:
A) the wavelength of the light.
B) the index of refraction of the medium through which it is traveling.
C) the index of refraction of the medium into which it is moving.
D) all of the above
A) the wavelength of the light.
B) the index of refraction of the medium through which it is traveling.
C) the index of refraction of the medium into which it is moving.
D) all of the above
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29
Ultraviolet radiation is hard to observe primarily because:
A) Earth's atmosphere easily absorbs it.
B) no space-based telescopes operate at ultraviolet wavelengths.
C) only the lowest-mass stars emit ultraviolet light.
D) very few objects emit at ultraviolet wavelengths.
A) Earth's atmosphere easily absorbs it.
B) no space-based telescopes operate at ultraviolet wavelengths.
C) only the lowest-mass stars emit ultraviolet light.
D) very few objects emit at ultraviolet wavelengths.
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30
Both reflecting and refracting telescopes suffer from:
A) chromatic aberration.
B) diffraction effects and chromatic aberration.
C) greater increase in weight for a given increase in aperture.
D) diffraction effects.
A) chromatic aberration.
B) diffraction effects and chromatic aberration.
C) greater increase in weight for a given increase in aperture.
D) diffraction effects.
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31
Which of the following causes the biggest problem in detecting infrared photons from an astronomical object?
A) smog
B) carbon dioxide
C) water vapor
D) light pollution
A) smog
B) carbon dioxide
C) water vapor
D) light pollution
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32
Which of the following properties is (are)improved by placing telescopes in space?
A) quantum efficiency
B) integration time and angular resolution
C) quantum efficiency and integration time
D) ability to observe at multiple wavelength regions and angular resolution
A) quantum efficiency
B) integration time and angular resolution
C) quantum efficiency and integration time
D) ability to observe at multiple wavelength regions and angular resolution
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33
A prism is able to spread white light out into a spectrum of colors based on the property of:
A) reflection.
B) refraction.
C) scattering.
D) interference.
A) reflection.
B) refraction.
C) scattering.
D) interference.
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34
When we determine the angular resolution of an interferometric array of radio telescopes using the formula q µ l/D,the variable D stands for the:
A) diameter of the telescopes.
B) separation between the telescopes.
C) number of telescopes.
D) focal length of the telescopes.
A) diameter of the telescopes.
B) separation between the telescopes.
C) number of telescopes.
D) focal length of the telescopes.
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35
The speed of a light wave:
A) is altered by a refractive medium.
B) is reduced whenever reflection occurs.
C) is not altered by reflection or refraction.
D) is not altered by refraction.
A) is altered by a refractive medium.
B) is reduced whenever reflection occurs.
C) is not altered by reflection or refraction.
D) is not altered by refraction.
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36
The diffraction limit of a 4-meter telescope is ________ than that of a 2-meter telescope.
A) two times larger
B) four times larger
C) two times smaller
D) four times smaller
A) two times larger
B) four times larger
C) two times smaller
D) four times smaller
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37
Cameras that use adaptive optics provide higher spatial resolution images primarily because:
A) they operate above Earth's atmosphere.
B) they capture infrared light, which has a longer wavelength than visible light.
C) deformable mirrors are used to correct the blurring due to Earth's atmosphere.
D) composite lenses correct for chromatic aberration.
A) they operate above Earth's atmosphere.
B) they capture infrared light, which has a longer wavelength than visible light.
C) deformable mirrors are used to correct the blurring due to Earth's atmosphere.
D) composite lenses correct for chromatic aberration.
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38
How does the resolution of a telescope depend on its focal length?
A) The longer the focal length is the better the resolution is.
B) The longer the focal length is the worse the resolution is.
C) There is no relation between resolution and focal length.
A) The longer the focal length is the better the resolution is.
B) The longer the focal length is the worse the resolution is.
C) There is no relation between resolution and focal length.
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39
Why do reflecting telescopes usually have a secondary mirror in addition to a primary mirror?
A) to increase the light-gathering power
B) to make the telescope shorter
C) to increase the focal length
D) to combat chromatic aberration
A) to increase the light-gathering power
B) to make the telescope shorter
C) to increase the focal length
D) to combat chromatic aberration
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40
One reason to prefer a reflecting over a refracting telescope is its:
A) lack of chromatic aberration.
B) shorter length for the same aperture size.
C) lighter weight for larger apertures.
D) All of the above are valid reasons.
A) lack of chromatic aberration.
B) shorter length for the same aperture size.
C) lighter weight for larger apertures.
D) All of the above are valid reasons.
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41
Does the wavelength of a wave change when entering a refractive medium? Explain.
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42
Discuss two tools that modern astronomers use to explore the cosmos that are different from traditional optical telescopes,and give an example of how and why each is used.
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43
Explain two major advantages of CCDs over other imaging techniques.
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44
The SETI project's Allen Telescope Array will have 350 radio dishes,each with an individual diameter of 6 meters,spread out over a circle whose diameter is 1 km.What would this array's spatial resolution be when it operates at 5 cm?
A) 10 arcsec
B) 0.10 arcsec
C) 10 arcmin
D) 1.0 arcmin
A) 10 arcsec
B) 0.10 arcsec
C) 10 arcmin
D) 1.0 arcmin
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45
Explain how adaptive optics help compensate for atmospheric seeing.
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46
Explain why the largest telescopes are not refracting telescopes.
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47
Give an explanation as to why electromagnetic radiation does not require a medium for propagation.
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48
The image below shows the Very Large Array in New Mexico.What is the benefit of using multiple telescopes in such an array?


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49
Explain why stars twinkle when viewed from the ground.Would they twinkle if viewed from outer space?
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50
What type of telescope is shown in the image below?


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51
How do telescopes advance astronomical science?
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52
Why is the wavelength of a reflected light wave generally equal to that of the incident wave?
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53
A spaceship approaches Earth at 0.9 times the speed of light and shines a powerful searchlight onto Earth.How fast will the photons from this searchlight be moving when they hit Earth?
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54
Using the figure below,list the different types of electromagnetic waves in order of increasing wavelength.


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55
What is the diffraction limit of a 4-meter telescope observing at a wavelength of 650 nm?
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56
Compare and contrast the wavelengths,frequencies,speeds,and energies of red and blue photons.
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57
Which telescope would collect 100 times more light than a 1-meter telescope?
A) 100-meter telescope
B) 50-meter telescope
C) 30-meter telescope
D) 10-meter telescope
A) 100-meter telescope
B) 50-meter telescope
C) 30-meter telescope
D) 10-meter telescope
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58
The two Keck 10-meter telescopes,separated by a distance of 85 meters,can operate as an interferometer.What is its resolution when it observes in the infrared at a wavelength of 2 μm?
A) 0.01 arcsec
B) 0.005 arcsec
C) 0.05 arcsec
D) 0.2 arcsec
A) 0.01 arcsec
B) 0.005 arcsec
C) 0.05 arcsec
D) 0.2 arcsec
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59
Where should telescopes purposed to observe the high energy light from the death of stars be located?
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60
Using the figure below,list the different types of electromagnetic waves in order of increasing frequency.


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61
What is the angular resolution of a 1-meter,ground-based,optical telescope that observes at a wavelength of 600 nm compared to that of a 300-ft,single-dish radio telescope that observes at a wavelength of 21 cm?
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62
Compare the light-gathering power of the human eye to that of a 10-inch telescope.
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