Exam 12: The Milky Way Galaxy

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Discuss how Harlow Shapley determined the structure of the Milky Way galaxy from his study of globular clusters.

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The Sun will one day pass through the instability strip and become a variable star.

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  The pink color in the above visual image is from __________. The pink color in the above visual image is from __________.

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The energy source at the center of our galaxy is called

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The orbits of population I stars I. are confined to disk of the galaxy. II. are very elliptical. III. are nearly circular. IV. are randomly inclined to the disk of the galaxy.

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The first scientific attempt to map the Milky Way galaxy

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RR Lyrae stars are in the constellation ___________.

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The density wave theory explains spurs and branches along the spiral arms.

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In the diagram below, the approximate absolute magnitude of a Type II Cepheid with a period of 30 days is ____________________. In the diagram below, the approximate absolute magnitude of a Type II Cepheid with a period of 30 days is ____________________.

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Why are all spiral tracers young?

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Figure 12-1 Figure 12-1   Refer to Figure 12-1. A Type I Cepheid has been located in an open cluster. The period of the Cepheid variable is 30 days and the variables apparent visual magnitude, m , is 10. First, use 12-1 to estimate the absolute visual magnitude, M . Calculate the distance to this open cluster? Hint: d <sub>pc</sub> = 10<sup>( m - M + 5)/5</sup> Refer to Figure 12-1. A Type I Cepheid has been located in an open cluster. The period of the Cepheid variable is 30 days and the variables apparent visual magnitude, m , is 10. First, use 12-1 to estimate the absolute visual magnitude, M . Calculate the distance to this open cluster? Hint: d pc = 10( m - M + 5)/5

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  The relative abundance of chemical elements are shown by atomic mass number. Which is/are the metal(s)? The relative abundance of chemical elements are shown by atomic mass number. Which is/are the metal(s)?

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Sgr A* emits radio waves.

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As viewed from above or face-on, a ____________ spiral galaxy has many branches and spurs, making the arms less discernible.

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Stars are eternal and unchanging in your lifetime but not over a star's lifetime

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CO observations of the galaxy reveal

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Which pulsate faster?

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The nuclear bulge of our galaxy

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The energy source at the center of our galaxy

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   The pink color tracing the spiral arms are from emission nebulae. The pink color tracing the spiral arms are from emission nebulae.

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