The Milky Way Galaxy.docx

The Milky Way Galaxy Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. ____ 1. Herschel's grindstone and Kapteyn's star system were too small because a. they did not count the brightest stars. b. they did not study the southern sky. c. they did not have large enough telescopes. d. they only observed stars in the disk of the galaxy and not the halo. e. they did not know about interstellar dust clouds. ____ 2. Which of the following is not a characteristic of the stars of the disk component of our galaxy? a. circular orbits. b. randomly inclined orbits. c. higher metal abundance. d. young stars. e. star formation regions. ____ 3. A group of 10 to 100 stars that formed at the same time but are so widely scattered in space their mutual gravity cannot hold them together is called a. a globular cluster. b. an open cluster. c. an association d. a spherical component e. an accretion disk. ____ 4. Our galaxy is suspected to be surrounded by a galactic corona because the disk of the galaxy a. rotates faster than expected in its outer region. b. rotates more slowly than expected in its outer region. c. rotates faster than expected in its inner region. d. rotates more slowly than expected in its inner region. e. is much flatter than expected. ____ 5. Younger stars have more heavy elements because a. old stars destroy heavy elements as they age. b. young stars burn their nuclear fuels faster. c. heavy elements were made in previous generations of stars. d. all of these e. heavy elements haven't had time to settle to the core of these younger stars. ____ 6. The first stars to form in our galaxy a. had circular orbits. b. had highly elliptical orbits. c. were population I stars. d. all had orbits in the same plane. e. formed the galactic clusters we see today. ____ 7. Good spiral tracers are all I. very old. II. very young III. very luminous IV. moving with large radial velocities a. I & III b. I & IV c. II & III d. II & IV e. I, III, & IV ____ 8. Radio maps of our galaxy show spiral arms because the a. arms have high Doppler shifts. b. gas in the spiral arms is hot enough to emit photons. c. dust in spiral arms is more dense than it is between the spiral arms. d. gas in spiral arms is more dense than it is between the spiral arms. e. stars in the spiral arms emit most of their energy at radio wavelengths. ____ 9. If the spiral density wave were the only thing producing spiral arms, it would be expected that a. all spiral arms would be dust free. b. all galaxies would have grand design spiral patterns. c. the Milky Way would be more massive than observed d. the Milky Way wouldn't have any spiral arms. e. the halo component of the Milky way would show spiral arms as well. ____ 10. The energy source at the center of our galaxy a. is not visible at optical wavelengths. b. produces gamma rays. c. must be less than 10 AU in diameter. d. all of the above e. none of the above. ____ 11. The magnetic field of the galaxy a. is stronger than the magnetic field of the sun. b. traps cosmic rays in the disk of the galaxy. c. creates the spiral density waves that initiate star formation. d. forces the halo stars to follow highly inclined orbits. e. produces 21-cm radiation that allows us to map the spiral arms. ____ 12. Population II stars I. are primarily found in the disk of the galaxy. II. contain more heavy metals than population I stars. III. are primarily old low mass stars. IV. are located in globular clusters. a. III & IV b. I & II c. II d. IV e. I, II, & III ____ 13. The first scientific attempt to map the Milky Way galaxy a. showed that the sun was located near the edge of the galaxy. b. showed that the halo of the galaxy contained population II stars. c. showed that our galaxy contained spiral arms. d. used globular clusters to determine the location of the center of the galaxy. e. was completed by William and Caroline Herschel. ____ 14. The age of the Milky Way galaxy has been estimated to be at least 13 billion years based on a. observations of globular clusters. b. observations of open clusters. c. 21-cm radiation from H I regions. d. the rotation curve of the galaxy. e. the energy produced by Sagittarius A* ____ 15. CO observations of the galaxy reveal a. the location of dense neutral hydrogen clouds. b. the location of population II stars. c. the location of population I stars. d. the location of the galactic corona. e. the location of giant molecular clouds. ____ 16. The chemical abundance of population I stars a. indicates that they were formed before the population II stars. b. indicates that the material they formed from had been enriched with material from supernovae. c. indicates that they contain very few heavy metals compared to halo stars. d. depends on the temperature of the star. e. depends on the mass of the star. ____ 17. The center of our galaxy lies in the direction of the constellation of a. Ursa Minor. b. Ursa Major. c. Sagittarius. d. Orion. e. Monoceros. ____ 18. Nucleosynthesis a. is the process by which energy is produced at the center of the galaxy. b. is the process by which hydrogen and helium are converted into heavier elements. c. describes the structure of a globular cluster. d. describes how the magnetic field of the galaxy traps cosmic rays. e. describes the method by which neutral hydrogen produces 21 cm radiation. ____ 19. The nuclear bulge of our galaxy a. contains stars that are primarily population I stars. b. contains relatively large amounts of gas and dust. c. contains stars primarily associated with the spherical component of our galaxy. d. contains stars primarily associated with the disk component of our galaxy. e. a, b and d ____ 20. 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. a. I b. IV c. I & IV d. II & IV e. I & III ____ 21. The traditional theory for the formation of the Milky Way Galaxy suggests that the galaxy formed a. as material accreted around a massive black hole currently at the center of our galaxy. b. from a large cloud of material that formed stars and star clusters and slowly flattened to a disk.. c. from material that had been ejected in the violent explosion of a dying galaxy. d. as a result of mergers between several smaller groups of gas, dust, and stars. e. as two massive galaxies collided. ____ 22. Radio maps of the spiral arms of our galaxy a. reveal that our galaxy is a grand design spiral. b. map the location of Hot O and B stars by the radio radiation they emit. c. reveal that the spiral arms are winding up and growing closer together. d. reveal that the sun is currently located in the center of a spiral arm. e. map the location of dense neutral hydrogen clouds. ____ 23. Halo stars located in the disk are easy to detect because they a. are the only low mass stars in the disk. b. are only found in globular clusters. c. are primarily O and B supergiants. d. move at an angle across the disk. e. emit cosmic rays. ____ 24. A type II Cepheid has been located in a distant globular cluster with a period of 10 days, what is the star's absolute magnitude? a. -1 b. 0 c. -4 d. -6 e. The absolute magnitude of a Cepheid variable cannot be determined unless its distance is known. ____ 25. 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 is 10. What is the distance to this open cluster? a. 100 pc b. 10,000 pc c. 20 pc d. 300 pc e. 2500 pc True/False Indicate whether the sentence or statement is true or false. ____ 31. Astronomers before Shapely underestimated the size of the Milky Way galaxy because they lacked large enough telescopes. ____ 32. Shapley found the distance to the center of the galaxy by studying the distance to open clusters. ____ 33. The disk of the Milky Way is approximately 20,000 ly in diameter. ____ 34. The rapid rotation in the outer disk suggests that our galaxy is more massive than previously thought. ____ 35. Old stars are poor in heavy atoms because there were no previous generations of stars. ____ 36. The disk of the galaxy is older than the halo. ____ 37. Spiral tracers tend to be old, luminous stars. ____ 38. Giant molecular cloud complexes are located in spiral arms. ____ 39. The density wave theory explains spurs and branches along the spiral arms. ____ 40. The center of our galaxy shows signs of past eruptions. Answer Section MULTIPLE CHOICE 1. ANS: E 2. ANS: B 3. ANS: C 4. ANS: A 5. ANS: C 6. ANS: B 7. ANS: C 8. ANS: D 9. ANS: B 10. ANS: D 11. ANS: B 12. ANS: A 13. ANS: E 14. ANS: A 15. ANS: E 16. ANS: B 17. ANS: C 18. ANS: B 19. ANS: C 20. ANS: E 21. ANS: B 22. ANS: E 23. ANS: D 24. ANS: A 25. ANS: B TRUE/FALSE 31. ANS: F 32. ANS: F 33. ANS: F 34. ANS: T 35. ANS: T 36. ANS: F 37. ANS: F 38. ANS: T 39. ANS: F 40. ANS: T