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The ____________________ of a telescope is determined by the size of the objective.

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light-gath...

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An achromatic lens


A) is used to correct spherical aberration in reflecting telescopes.
B) is used to correct chromatic aberration in refracting telescopes.
C) is used to correct spherical aberration in refracting telescopes.
D) is used to correct chromatic aberration in reflecting telescopes.
E) contains two mirrors and focuses the light back through the primary mirror.

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Which of the waves below has the shortest wavelength?


A) gamma rays
B) X-rays
C) visible light
D) infrared
E) radio

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A larger-objective lens shows ____________ a smaller-objective lens.


A) more detail than
B) less detail than
C) the same amount of detail as

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The ____________________ is a measure of the finest detail that can be seen in an image.

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One of the advantages of charge-coupled devices over photographic plates is that a CCD can record bright and faint objects on the same exposure.

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Radio telescopes which use dishes to gather radio waves are ____ telescopes.


A) reflecting
B) refracting
C) deflecting
D) compound
E) retracting

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Far infrared astronomy must be done from high-flying aircraft because


A) far infrared radiation is absorbed low in Earth's atmosphere.
B) far infrared photons are quite energetic.
C) far infrared telescopes are not very heavy.
D) far infrared sources are very bright.
E) none of the above.

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Chromatic aberration occurs in a ____ telescope when ____.


A) reflecting; different colors of light do not focus at the same point
B) refracting; different colors of light do not focus at the same point
C) reflecting; light of different wavelengths get absorbed by the mirror
D) refracting; light of different wavelengths get absorbed by the lens

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The ____________________ is a measure of how many times larger the angular size of an object appears through a telescope.

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Why must telescopes that observe in the far infrared be cooled?

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Telescopes that observe in the far infra...

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____ is absorbed by ozone in Earth's atmosphere that is located between 20 km and 40 km above Earth's surface. Therefore, telescopes to observe this radiation must be placed in space.


A) Infrared radiation
B) Ultraviolet radiation
C) Radio wave radiation
D) X-ray radiation
E) Visible light

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The amount of energy a photon carries depends on its wavelength.

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Long wavelength visible light


A) will have a greater energy than short wavelength visible light.
B) will have a speed that is faster than short wavelength light.
C) has a higher frequency than short wavelength visible light.
D) will appear blue in color to the average human eye.
E) will appear red in color to the average human eye.

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The Hubble Space Telescope objective mirror is not affected by


A) bad seeing.
B) chromatic aberration.
C) diffraction.
D) Answers b and c
E) Answers a and b

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____ is absorbed by water in Earth's atmosphere and requires that telescopes for observing at these wavelengths be placed on mountain tops or in space.


A) Infrared radiation
B) Ultraviolet radiation
C) Radio wave radiation
D) X-ray radiation
E) Visible light

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The Very Long Baseline Array (VLBA)


A) is the highest resolution optical telescope ever built.
B) is located in Arecibo, Puerto Rico.
C) is a matched pair of 8 m telescopes, one of which is in Chile and the other in Hawaii.
D) is an air-borne infrared telescope.
E) is a set of radio telescopes linked together electronically to provide very high resolution.

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A(n) ____________________ uses a mirror as its objective.

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reflecting...

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In a reflecting telescope, the objective is a mirror.

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The resolving power for light of 550 nm of an optical telescope with a diameter of 232 cm is


A) 0.05 arc seconds.
B) 232 arc seconds.
C) 2.32 arc seconds.
D) 5 arc seconds.
E) 11.6 arc seconds.

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