Chapter 6 – Quiz 6
Observatory X can detect dimmer stars and Observatory Y reveals more detail in images.
Observatory Y both detects dimmer stars and reveals more detail in images.
Both observatories have the same capabilities, but Observatory Y would be cheaper to build.
Observatory X both detects dimmer stars and reveals more detail in images.
Observatory Y can detect dimmer stars and Observatory X reveals more detail in images.
The one that still looks sharp at large size has better (smaller) angular resolution than the one that looks fuzzy.
Both photographs have the same angular resolution, because they are both photographs of the same object.
The one that looks fuzzy at large size has better angular resolution (smaller) than the one that looks sharp.
Both photographs have the same angular resolution, because they were both printed at the same sizes in each case.
It is closer to the stars.
It never has to close because of cloudy skies.
It can observe infrared and ultraviolet light, as well as visible light.
Stars do not twinkle when observed from space.
X-ray telescopes require the use of grazing incidence mirrors.
It was built by NASA.
X rays do not penetrate Earth’s atmosphere.
X rays are too dangerous to be allowed on the ground.
Over the 60-year period, telescopes have gradually gotten bigger and more powerful.
The world’s most powerful telescope remained the same for most of this period, but in the past 20 years many new and more powerful telescopes have been built.
The only major change in telescope power has occurred because of our ability to launch telescopes into space rather than operating them only from the ground.
Although there have been advances in cameras and computing power, telescopes themselves have not changed much in the last 60 years.
CCDs allow long exposures (e.g., minutes or hours) and film does not.
CCDs can record the colors of astronomical objects accurately while film cannot.
CCDs capture a much higher percentage of the incoming photons than film.
CCDs can be attached to modern telescopes more easily than can photographic film.
Dry regions mean less rain and clouds, and mountaintops in dry regions may even allow some infrared observations.
The thin air on mountaintops makes the glass in telescope mirrors less susceptible to warping.
Mountaintops far from cities are generally subject to less light pollution than locations nearer to cities.
Being on a high mountain top means being relatively high in the atmosphere, which tends to limit turbulence.
The photo will seem to show only one star rather than two.
You will see two distinct stars in your photograph.
The two stars will appear to be touching, looking rather like a small dumbbell.
The stars will not show up at all in your photograph.
Radio telescopes are designed to collect sound rather than light.
Objects that emit radio waves are always much larger than objects that emit visible light, and therefore require larger telescopes.
It is because radio telescopes are used in the daytime and visible light telescopes are used at night.
Getting an image of the same angular resolution requires a much larger telescope for radio waves than for visible light.
The 8-meter telescope has 8 times the light-collecting area of the 2-meter telescope.
The answer cannot be determined from the information given in the question.
The 8-meter telescope has 4 times the light-collecting area of the 2-meter telescope.
The 8-meter telescope has 16 times the light-collecting area of the 2-meter telescope.
By using a long exposure time, the photograph can allow you to see objects that would be too dim to see with your eye.
The photograph will have far better angular resolution than you can see with your eye.
If taken with a camera with a sensitive detector such as a CCD, the photograph can capture a much larger percentage of the incoming photons than can your eye.
The photograph provides a more reliable record of what is seen through the telescope than can a drawing made by eye.
the bubbling and boiling of gases on the surfaces of stars
rapid changes in the brightnesses and colors of stars caused by changes in their spectra
turbulence in the Earth’s atmosphere
Determining the age of the solar system.
Studying how a star’s brightness varies over a period of 3 years.
Studying how different planets differ in their surface compositions.
Measuring the rotation rate of a distant star.
The Keck I telescope on Mauna Kea.
The Arecibo radio telescope in Puerto Rico.
The Chandra X-ray Observatory.
The Hubble Space telescope.
Telescopes on the Moon could see objects in all parts of the sky equally well, whereas telescopes on Earth can see only portions of the sky that depend on their latitude.
Radio astronomy would be advantageous on the Moon because human radio transmissions are less likely to cause interference, especially on the far side of the Moon.
It would be possible to put telescopes for ultraviolet and X-ray astronomy on the surface, unlike the case on the surface of the Earth.
Telescopes on the Moon could observe stars even when it is daytime on the Moon.