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Understanding the Solar System: Key Concepts and Questions

liang avatar
7 diapositives · 208 Views · Aug 01, 2014

Explore fundamental concepts of our solar system through a series of quiz questions addressing planetary characteristics, formation theories, and radiometric dating. Learn about the temperature differences between terrestrial planets and gas giants, the formation of planets according to Laplace's nebula hypothesis, the dynamic changes in spin rates during molecular cloud collapse, and more. Each question provides insight into the processes that shape our celestial neighborhood, offering a deeper understanding of planetary science in an engaging format.

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  1. Test question 7.1 • In the solar system, the temperature difference between terrestrial planets and gas giants is due to • vTheir distance from the sun, • xThe number of their moons • xThe length of their days • xTilt of their spin

  2. Test question 7.2 • Laplace’s nebula hypothesis suggests that planets in the solar system formed • xThrough capture of freely floating planets, B) xOut a piece of the sun which was torn out, from the Sun by a passing star, C) vIn a gaseous disk surrounding the infant Sun, D) xFrom the left over of its companion

  3. Test question 7.3 When a molecular cloud collapses and shrinks its radius to 0.001 times of its original size, its spin rate would become • vFaster by a million times, • xFaster by a thousand times • xStay the same • xSlow down by a thousand times

  4. Test question 7.4 Mercury orbits the Sun at 0.4 AU whereas Pluto’s distance is 40 AU. If there were formed at the present-day location, temperature due to the solar irradiation at Mercury would be: • x100 times hotter than at Pluto • v10 times hotter than at Pluto • xSame as at Pluto • x100 times cooler than at Pluto

  5. Test question 7.5 • Radioactive CAI’s in primitive meteorites provide constraints on • xThe dominant chemical composition of the solar nebula • vTime scale for solar system formation • xThe rate of nuclear energy release from the Sun • xPlanet formation through core accretion

  6. Test question 7.6 • The half life of radioactive C14 is 5760 years. In 17,280 years after one gram of C14 was generated, the amount of it left behind is • xHalf its original amount, • xOne third of its original amount, • xOne quarter of its original amount, • vOne eighth of its original amount.

  7. Test question 7.7 Dense Craters on the moon and mercury indicate: • xTerrestrial planets had many volcano when they were young • vThese objects formed through collisions & impacts • xAll terrestrial planets cool down rapid after their formation • xPlate tectonics is active in these planets.