Chapter 11: Problem 1
Why is it impossible to see Mercury or Venus in the sky at midnight?
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Chapter 11: Problem 1
Why is it impossible to see Mercury or Venus in the sky at midnight?
These are the key concepts you need to understand to accurately answer the question.
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Use the Starry Night Enthusiast \({ }^{\mathrm{TM}}\) program to examine Mercury. Select Favourites \(>\) Solar System \(>\) Mercury from the menu. Select View > Feet from the menu to remove the image of the astronaut's spacesuit from the view. Select Options \(>\) Solar System > Planets-Moons. .. from the menu to allow you to examine the complete surface of the planet. In the PlanetsMoons Options dialog box, slide the control next to the label Show dark side all the way to the right (Brighter) end of the scale. Click OK to close the dialog box. Use the Zoom controls in the toolbar to zoom in and out on the view. Rotate the image of Mercury by placing the mouse cursor over the image of the planet, holding down the mouse button, and moving the mouse. (On a two- button mouse, hold down the left mouse button.) As you explore the surface of the planet Mercury, estimate the diameter of the largest craters by measuring their size on the screen with a ruler and comparing to the diameter of Mercury (see Table 11-1). (Note that the rosette patterns surrounding both planetary poles are an artifact of the technique used to produce these images).
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?
Use the Stamy Night Enthusiast \({ }^{\text {M }}\) program to observe solar transits of Venus (see Question 83). Display the entire celestial sphere (select Guides \(>\) Atlas in the Favourites menu). Open the Find pane and click the menu button for Venus (the downwardpointing blue arrow to the left of Venus) in the list. Select Centre from the menu. Use the zoom controls in the toolbar to adjust the field of view to about \(1^{\circ} \times 1^{\circ}\). (a) In the toolbar, Stop time flow and then set the Time and Date to June 8, 2004, at 12:00:00 A.M. Set the Time Flow Rate to 1 hour. Step backward or forward through time using the single-step buttons (the leftmost and the rightmost buttons) and record the times at which the solar transit begins and ends, changing the Time Flow Rate to 1 minute and the field of view to increase the accuracy of your measurement, as necessary. What is the total duration of the solar transit? (b) The ecliptic appears in Starry Night Enthusiast \({ }^{\top M}\) as a green line. During the transit, is Venus precisely on the ecliptic? If not, about how far off is it? (Hint: The Sun has an angular diameter of about 30 arcmin.) (c) Repeat parts (a) and (b) for the solar transit of Venus on June 6,2012 .
Describe the apparent motion of the Sun during a "day" on Venus relative to (a) the horizon and (b) the background stars. (Assume that you can see through the cloud cover.)
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?
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