Which method of astronomical measurement is the precise measurement of brightness? |
photometry |
The primary purpose of a telescope is to |
collect a large amount of light and bring it into focus |
The tendency of a wave to bend as it passes from one transparent medium to |
refraction |
Compared to optical telescopes, radio telescopes are built large because |
radio photons don’t carry much energy |
The amount of diffraction a telescope creates depends upon: |
the wavelength and the diameter of the telescope objective |
What is the resolution of a telescope? |
its ability to distinguish two adjacent objects close together in the sky |
In which part of the electromagnetic spectrum have astronomers been unable to get any information? |
We now can access information in all spectral lengths |
What problem is adaptive optics designed to correct? |
the effects of atmospheric turbulence |
Which of the following greatly improves the angular resolution of radio maps? |
use of interferometers |
It is diffraction that limits the ________ of a telescope’s objective. |
resolution |
It is diffraction that limits the ________ of a telescope of a given objective diameter. |
resolution |
The amount of diffraction and thus the resolution of the scope depends upon |
the wavelength used and the size of the main telescope objective lens or mirror |
In astronomy, an interferometer can be used to |
improve the angular resolution of radio telescopes |
The convex secondary mirror in this design focuses light down through a hole cut in the concave primary mirror. |
Cassegrain reflector |
Which design has a convex primary mirror and flat secondary mirror, with the eyepiece located on the top side of the telescope tube? |
Newtonian reflector |
What is true of radio telescopes? |
They have poorer angular resolution than a refractor. |
A mountain top is an especially good site for infrared telescopes since: |
All of the above are factors |
What type of telescope is the Subaru telescope (shown below)? |
Cassegrain reflector |
Which of the following is currently supplying high resolution x-ray images from space? |
Chandra |
This design involves only one optical surface, a concave mirror. |
prime focus reflector |
What is the primary purpose of an astronomical telescope? |
To collect a lot of light and bring it to a focus |
What is the light-gathering power of an 8 inch telescope compared to a 4 inch telescope? |
4x better |
What is the resolving power of the telescope? |
the ability to distinguish adjacent objects in the sky |
A major advantage of a Newtonian reflector over a refractor is |
the elimination of chromatic aberration |
How much better resolution would a 60 mm objective lens have than your eye’s 6 mm exit pupil? |
10x |
Which of the following is a problem inherent in all large radio telescopes? |
Radio waves have long wavelengths, so radio telescopes have poor resolution |
Why are most large telescopes reflectors, not refractors? |
All of the above |
What problem do refractor telescopes have that reflectors don’t? |
chromatic aberration |
The design of modern x-ray telescopes depends on |
grazing incidence optics |
Which of these devices helps correct coma in fast reflectors? |
Schmidt corrector plate |
Diffraction is the tendency of light to |
spread around corners |
Radio dishes are large in order to: |
increase their angular resolution and collect the very weak radio photons. |
The process occurring when photons bounce off a polished surface is called |
reflection |
What are two advantages of large scopes over smaller ones? |
Large telescopes have more light grasp and better resolution |
The name of the new Infrared Orbiting Observatory is the: |
Spitzer Space Telescope |
The Chandra X-ray telescope must use |
grazing incidence optics to focus the short wavelengths |
Refractor telescopes suffer from this separation of light into its component colors |
chromatic aberration |
Which type of telescope has the simplest light path? |
prime focus reflector |
One advantage of the Hubble Space telescope over ground based ones is that |
in orbit, it can operate close to its diffraction limit at visible wavelengths |
Compared to a 5 inch prime focus reflector, a 5 inch Newtonian reflector will |
have the same light gathering power |
A telescope with a 60 mm objective lens collects how many times as much light as does your eye’s 6 mm exit pupil? |
100x |
The angular resolution of an 8 inch diameter telescope is _______ greater than that of a 2 inch diameter telescope. |
4x |
Green light has a shorter wavelength than orange light. In a 5 inch telescope, green light will |
provide better angular resolution than orange light |
The most important advantage of CCDs over film is that |
they record much more light in a given exposure time |
What is "seeing"? |
a measurement of the image quality due to air stability |
What problem does adaptive optics correct? |
turbulence in the earth’s atmosphere which creates twinkling |
The Arecibo radio telescope is laid out like which optical telescope design? |
prime focus reflector |
This design combines the radiation from two different telescopes to greatly enhance resolution via computer synthesis. |
interferometer |
What type of telescope is the Hubble Space Telescope? |
cassegrain |
Which design is subject to chromatic aberration? |
refractor |
*Essay: What are some advantages of radio telescopes over optical scopes? |
Radio telescopes can be used day or night, they are much less affected by cloudy skies, and they open a new window to observe the Universe. They allow us to observe astronomical objects at a different wavelength than an optical telescope, thus giving an opportunity to compare and contrast the images. |
Astronomy Ch 5
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