Chapter 11: Problem 34
a) What is a runaway greenhouse effect? (b) What is a runaway icehouse effect?
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These are the key concepts you need to understand to accurately answer the question.
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Chapter 11: Problem 34
a) What is a runaway greenhouse effect? (b) What is a runaway icehouse effect?
These are the key concepts you need to understand to accurately answer the question.
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The classic 1950 science-fiction movie Rocketship X-M shows astronauts on the Martian surface with oxygen masks for breathing but wearing ordinary clothing. Would this be a sensible choice of apparel for a walk on Mars? Why or why not?
Use the Starry Night Enthusiast \({ }^{\mathrm{TM}}\) program to observe the appearance of Mars. Select Favourites \(>\) Guides \(>\) Atlas from the menu. Select View \(>\) Celestial Grid from the menu to turn this option off. Open the Find pane and click the menu button for Mars and choose Centre from the menu. Close the Find pane and then use the Zoom controls in the toolbar to set a field of view of approximately \(58^{\prime \prime} \times 40^{\prime \prime}\). (a) Set the Time Flow Rate to 1 hour and then run Time Forward. Describe what you see. (b) Stop time flow. Change the Time Flow Rate to 1 lunar month. Run Time Forward again. Describe what you see. Using a diagram like Figure 4-6, explain the changes in the apparent size of the planet. (c) Stop time flow and zoom out to a field of view of approximately \(\mathbf{2}^{\prime} \times \mathbf{1}^{\prime}\). Change the time and date in the toolbar to \(12: 00: 00\) A.M. on August 28, 2003, to see Mars during a very favourable opposition. You will see Mars and its two moons, Phobos and Deimos. In the toolbar, set the Time Flow Rate to 1 minute. Record the date and time in the display, and note the position of Phobos (the inner moon). Click the Run Time Forward and single time step button (the rightmost time control button) to advance time until Phobos returns to approximately the same position relative to Mars. Record the date and time in the display. From your observations, what is the orbital period of Phobos? How does your result compare with the orbital period given in Appendix 3? (d) Repeat part (c) for Deimos (the outer moon).
Refer to the Universe Web site or eBook for a link to a Web site that calculates the dates of upcoming greatest elongations of Mercury. Consult such magazines as Sky or Telescope and Astronomy, or the Web sites for these magazines, to determine if any of these greatest elongations is going to be a favorable one. If so, make plans to be one of those rare individuals who has actually seen the innermost planet of the solar system. Set aside several evenings (or mornings) around the date of the favorable elongation to reduce the chances of being "clouded out." Select an observing site that has a clear, unobstructed view of the horizon where the Sun sets (or rises). If possible, make arrangements to have a telescope at your disposal. Search for the planet on the dates you have selected, and make a drawing of its appearance through your telescope.
What kind of surface features are found on Mercury? How do they compare to surface features on the Moon? Why are they probably much older than most surface features on the Earth?
Why are naked-eye observations of Mercury best made at dusk or dawn, while telescopic observations are best made during the day?
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