Taken from the NSW Board of Studies past School Certificate Examination Papers Year 10 How the universe came to be School Certificate Questions Use the diagram to answer Questions 1 and 2. The diagram represents a neutral atom with a subatomic particle being released. 1. What type of particle has been released? (A) Electron (B) Neutron (C) Nucleus (D) Proton 2. As the subatomic particle is released, it has kinetic energy. What was the original form of this energy? (A) Gravitational (B) Light (C) Nuclear (D) Sound 3. Which of the following is associated with the ‘death’ explosion of a massive star? (A) Asteroid (B) Comet (C) Galaxy (D) Supernova 4. This statement describes part of a scientific theory: ‘An instant after creation, the universe rapidly expanded.’ To which theory does the statement refer? (A) The atomic theory (B) The big-bang theory (C) The particle theory of matter (D) The theory of evolution Taken from the NSW Board of Studies past School Certificate Examination Papers Use the diagram to answer Questions 5-7. The diagram illustrates the formation of a black hole. Objects in the diagram are not drawn to scale. 5. Which element must be present in the cloud of gas and dust for a star to form? (A) Carbon (B) Helium (C) Hydrogen (D) Oxygen 6. How many times bigger is the radius of the star when it ‘burns’ helium than when it ‘burns’ hydrogen? (A) 2 (B) 10 (C) 14 (D) 140 7. Which of the following correctly compares the ‘burning’ in stars with the burning of fossil fuels? Taken from the NSW Board of Studies past School Certificate Examination Papers The diagram represents a distant galaxy. 8. What instrument would be most useful to collect information about a distant galaxy? (A) Light microscope (B) Light telescope (C) Radio telescope (D) Satellite Use this information to answer Questions 9 and 10. When carbon-14 undergoes radioactive decay, it forms nitrogen-14. The graph shows the amount of carbon-14 remaining over time. At time 0, there was no nitrogen-14 present. 9. What is the approximate amount of nitrogen-14 produced after 8 X 103 years? (A) 23 g (B) 37 g (C) 63 g (D) 77 g Taken from the NSW Board of Studies past School Certificate Examination Papers 10. Which graph shows the amount of nitrogen-14 produced over the same period? Use this information to answer Questions 11-13. The graph shows: • The present-day temperature and brightness of most stars in the Universe (dotted line X); • The predicted evolutionary path of our Sun (solid line Y) including its present-day conditions. Taken from the NSW Board of Studies past School Certificate Examination Papers 11. According to this information, what will be the final evolutionary stage of our Sun? (A) Blue giant (B) Interstellar cloud (C) Red dwarf (D) White dwarf 12. How did our Sun change during its initial formation from interstellar cloud? (A) It became larger. (B) It became smaller. (C) It became hotter. (D) It became colder. 13. How much brighter than our Sun is a blue giant of temperature 30 000 K? (A) 5 times (B) 10 times (C) 1 000 times (D) 10 000 times Use this diagram to answer Questions 14 and 15. The diagram summarises the life cycles of some stars. 14. What is the final stage for a star of one solar mass? (A) Black dwarf (B) Black hole (C) Enriched cloud (D) Gas cloud Taken from the NSW Board of Studies past School Certificate Examination Papers 15. Why have these models describing the life cycle of stars only recently been developed? (A) The evolution of stars is a very slow process. (B) There have been disputes about theories of the origin of the universe. (C) Technologies to gather data about stars were not previously available. (D) It takes a long time for electromagnetic radiation from stars to reach Earth. 16. Table 1 shows the average distance from the Sun and the average orbital speed of some of the planets in our solar system. Table 2 shows the five largest asteroids and their average distances from the Sun. Taken from the NSW Board of Studies past School Certificate Examination Papers (a) On the grid provided, draw a line graph of the average distance from the Sun and the average orbital speed for the planets listed. (b) Use the graph to predict the range of orbital speeds for the asteroids listed in Table 2.