Exam 13: Exploring Our Galaxy

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RR Lyrae variable stars are bigger,brighter and have longer periods of pulsation than Cepheid variables.

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In a spin-flip transition of an electron,a photon is emitted.

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Where would you look in our Galaxy to find older,metal-poor stars?

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The major advantage of the measurement of the 21-cm radio emission from hydrogen gas for investigating the spiral structure of our Galaxy is that

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Approximately 10% of the mass of the Galaxy is made up of dark matter.

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What happens when the electron in a hydrogen atom flips its direction of spin,starting parallel to the spin of the proton and ending antiparallel to the spin of the proton?

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Which of the following,above all else,outlines the spiral arms of a spiral galaxy?

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Where are the Population I and Population II stars in the Milky Way Galaxy located?

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What is the difference between grand-design spiral galaxies and flocculent spiral galaxies?

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Which of the following types of stars are not found in the halo of our Galaxy?

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What causes the spiral arm structure of spiral galaxies?

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Who was the first to look at the Milky Way with a telescope?

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The Milky Way is one of myriad

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Put the following objects in order of usual size from smaller to larger.

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In our Galaxy,young metal-rich stars are found

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Interstellar dust obscures our view of distant regions of space at optical wavelengths.Which of the following statements is TRUE concerning this dust obscuration?

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The ratio of thickness to diameter of the Milky Way Galaxy is

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What is the basic shape of a spiral galaxy?

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Where are the hottest stars in the Galaxy?

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Radio waves of 21-cm wavelength originate from which component of the interstellar medium?

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