Chapter 13: Problem 16
What is the origin of the electric current that flows through Io?
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Chapter 13: Problem 16
What is the origin of the electric current that flows through Io?
These are the key concepts you need to understand to accurately answer the question.
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Use the Starry Night Enthusiast \({ }^{\text {TM }}\) program to view Saturn from its satellite Enceladus. First click the Home button in the toolbar. Select Options \(>\) Viewing Location ... from the menu. In the dialog window that appears at the top of the Viewing Location, set the drop-down box next to the "View from:" label to read "the surface of" and set the second drop-down box to read "Enceladus" (listed under Saturn). In the list of locations that appears under the List tab on Enceladus, scroll to "Ahmad." Click on this entry to highlight it and then click the Set Location button. To see Saturn from this location on Enceladus, center on Saturn by double-clicking the entry for this planet in the Find pane. (a) Stop the time flow and set the Time Flow Rate to 1 minute in the toolbar, then click on the Run Time Forward button (a triangle that points to the right). How do the stars appear to move as seen from this location on Enceladus? How does Saturn appear to move? What do these observations tell you about the relationship between the orbital period and rotation period of Enceladus? (b) Set the Time Flow Rate to 1 hour. By stepping forward through time using the rightmost single-step button, determine how much time elapses from when Saturn appears full from this location to when it next appears full. Explain why this is the same as the orbital period of Enceladus, and compare this to the value of the orbital period given in Appendix 3 .
In what ways does the system of Galilean satellites resemble our solar system? In what ways is it different?
If you observed the Galilean satellites through a telescope for a single night, could you notice their motions around Jupiter?
In the classic science-fiction film 2010: The Year We Make Contact, an alien intelligence causes Jupiter to contract so much that nuclear reactions begin at its center. As a result, Jupiter becomes a star like the Sun. Is this possible in principle? Explain your answer.
Use the Starry Night Enthusiast \({ }^{\mathrm{TM}}\) program to observe the Galilean satellites of Jupiter. Open the Favourites pane and click on Guides \(>\) Atlas to display the entire celestial sphere. Open the Find pane and double-click the entry for Jupiter to center this planet in the view. Using the controls at the right-hand end of the toolbar, zoom in to a field of view of approximately \(13^{\prime} \times 9^{\prime}\). Stop time flow and in the toolbar, set the date and time to March 4,2004 , at 12:00:00 A.M to see Jupiter at opposition. Set the Time Flow Rate to 20 minutes by clicking on the number in the Time Flow Rate box and setting the value with the keyboard. Then click on the Run Time Forward button (a triangle that points to the right). You will see the four Galilean satellites orbiting Jupiter. (If these moons appear to move too quickly, adjust the Time Flow Rate to 10 minutes.) (a) Are all four satellites ever on the same side of Jupiter? (b) Observe the satellites passing in front of and behind Jupiter and look for their shadows upon the planet. (Zoom in as needed). Explain how your observations tell you that all four satellites orbit Jupiter in the same direction.
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