Exam 4: Light and Telescopes

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The angular resolution of the largest single-dish radio telescope in the United States,the 300-ft Green Bank Telescope,is __________ when it operates at a wavelength of 20 cm.

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What type of telescope is shown in the image below? What type of telescope is shown in the image below?

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It is possible for light to travel slower than 300,000 km/s.

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Calculate the resolution of an interferometric array consisting of five 10-m radio telescopes,each located 1,000 meters apart from each other and observing a distant object at a wavelength of 21 cm.

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A prism is able to spread white light out into a spectrum of colors based on the property of:

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If the wavelength of a beam of light were to double,how would that affect its frequency?

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The light-gathering power of a 4-m telescope is __________ than that of a 2-m telescope.

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Using the figure below,list the different types of electromagnetic waves in order of increasing wavelength. Using the figure below,list the different types of electromagnetic waves in order of increasing wavelength.

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Why do reflecting telescopes usually have a secondary mirror in addition to a primary mirror?

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The major advantage CCDs have over other imaging techniques is that:

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The light-year is a unit of:

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The part of the human eye that acts as the detector is the:

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Which of the following lists different types of electromagnetic radiation in order of increasing wavelength?

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Using the figure below,list the different types of electromagnetic waves in order of increasing frequency. Using the figure below,list the different types of electromagnetic waves in order of increasing frequency.

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The angular resolution of a ground-based telescope is usually set by:

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In the past,astronomers have placed telescopes in highflying aircraft in an effort to rise above the water vapor in the Earth's atmosphere.

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Explain two major advantages of CCDs over other imaging techniques.

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Arrays of radio telescopes can produce much better resolution than single-dish telescopes because they work based on the principle of:

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Explain why chromatic aberration is a problem for refracting mirrors but not reflecting mirrors.

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The image quality of most optical telescopes is limited by differential atmospheric refraction experienced by light as it passes through the Earth's atmosphere.

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