Exam 5: Light: the Cosmic Messenger

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The greater the wavelength of light, the greater its energy.

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Suppose an astronomer proposed to build a major observatory on the campus of your school. Would it make a good observing site? Explain why or why not.

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Answers will vary somewhat with location, but in general campuses are bright environments that are poor observing sites from a light pollution standpoint. Other factors students may mention might include light from surrounding or nearby cities, excessive cloudiness or rain, windy area with a lot of turbulence, and low altitude with lots of atmosphere above.

Which of the following conditions lead you to see an absorption line spectrum from a cloud of gas in interstellar space?

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How many atoms fit across the period at the end of this sentence?

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What is an artificial star?

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Which of the following is always true about images captured with X- ray telescopes?

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Imagine that the sun began glowing half as bright at all visible wavelengths, but glowed much brighter in the infrared. How would this look to us, and why?

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X- rays from astronomical objects can only be detected from telescopes in space.

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The most common isotope of gold has atomic number 79 and atomic mass number 197. How many protons and neutrons does the gold nucleus contain? Assuming the gold is electrically neutral, how many electrons does it have?

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How does the light- collecting area of an 8- meter telescope compare to that of a 2- meter telescope?

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One of the absorption lines of hydrogen has a rest wavelength of 656 nm (at rest means with respect to the observer, like in a lab). You observe several stars and measure the wavelength of this same hydrogen absorption line in each star. Based on the measured wavelength of this line, which star is moving towards the Earth the fastest?

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What do astronomers mean by light pollution?

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When atoms of an element are heated enough that they lose electrons, their emission and absorption spectra change.

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Lines of a particular element appear at the same wavelength in both emission and absorption line spectra.

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The resolution of a 10- meter telescope is about 0.01 arcsecond for visible light. Would you expect the angular resolution of a 10- meter radio telescope to be better than, equal to, or worse than 0.01 arcsecond? Explain.

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Why do astronomers need different telescope designs to observe across the electromagnetic spectrum?

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Without telescopes or other aid, we can look up and see the Moon in the night sky because it

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What is the purpose of interferometry?

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Briefly explain why spectral lines are useful in determining the chemical composition of their source.

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Observatory construction sites: Consider the factors that go into selecting telescope construction sites. What type of site would you look for to build a large visible- light observatory? Where would you want to build an X- ray telescope? Would these be the same or different, and why?

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