Chapter 5: Problem 1
When Jupiter is undergoing retrograde motion as seen from Earth, would you expect the eclipses of Jupiter's moons to occur several minutes early, several minutes late, or neither? Explain.
Chapter 5: Problem 1
When Jupiter is undergoing retrograde motion as seen from Earth, would you expect the eclipses of Jupiter's moons to occur several minutes early, several minutes late, or neither? Explain.
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Get started for freeUse the Staryy Night Enthusiast \({ }^{\text {TM }}\) program to examine the temperatures of several relatively nearby stars. First display the entire celestial sphere (select Guides \(>\) Atlas in the Favourites menu). You can now search for each of the stars listed below. Open the Find pane, click on the magnifying glass icon at the left side of the edit box at the top of the Find pane, select Star from the menu that appears, type the name of the star in the edit box and click the Enter (Return) key. (i) Altair; (ii) Procyon; (iii) Epsilon Indi; (iv) Tau Ceti; (v) Epsilon Eridani; (vi) Lalande 2118.5. Information for each star can then be found by clicking on the Info tab at the far left of the Stary Night Enthusiast \(^{\mathrm{TM}}\) window. For each star, record its temperature (listed in the Info pane under Other Data). Then answer the following questions. (a) Which of the stars have a longer wavelength of maximum emission \(\lambda_{\max }\) than the Sun? Which of the stars have a shorter \(\lambda_{\max }\) than the Sun? (b) Which of the stars has a reddish color?
How is the energy of a photon related to its wavelength? What kind of photons carry the most energy? What kind of photons carry the least energy?
What is the Doppler effect? Why is it important to astronomers?
Turn on an electric stove or toaster oven and carefully observe the heating elements as they warm up. Relate your observations to Wien's law and the Stefan-Boltzmann law.
Use the Starry Night Enthusiast \({ }^{\mathrm{TM}}\) program to examine some distant celestial objects. First display the entire celestial sphere (select Guides \(>\) Atlas in the Favourites menu) and ensure that deep space objects are displayed by opening View \(>\) Deep Space and clicking on Messier Objects and Bright NGC Objects. You can now search for objects (i), (ii), and (iii) listed below. Click the Find tab at the left of the main view window to open the Find pane, click on the magnifying glass icon at the left of the edit box at the top of the Find pane and select Search All from the menu, and then type the name of the object in the edit box followed by the Enter (Return) key. The object will be centered in the view. For each object, use the zoom controls at the right-hand end of the Toolbar (at the top of the main window) to adjust your view until you can see the object in detail. For each object, state whether it has a continuous spectrum, an absorption line spectrum, or an emission line spectrum, and explain your reasoning. (i) The Lagoon Nebula in Sagittarius. (Hint: See Figure 5-18.) (With a field of view of about \(6^{\circ} \times 4^{\circ}\), you can compare and contrast the appearance of the Lagoon Nebula with the Trifid Nebula just to the north of it.) (ii) M31, the great galaxy in the constellation Andromeda. (Hint: The light coming from this galaxy is the combined light of hundreds of billions of individual stars.) (ii) The Moon. (Hint: Recall from Section \(3-1\) that moonlight is simply reflected sunlight.)
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