Horizons: Exploring the Universe (MindTap Course List)
14th Edition
ISBN: 9781305960961
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Textbook Question
Chapter 17, Problem 4P
What is the maximum angular diameter of Phobos as seen from Earth? (Hint: Use the small-angle formula in Reasoning with Numbers 3-1.) (Note: Useful data can be found in the chapter text and in Appendix Table A-10.)
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What is the angular diameter of Saturn (in degrees) as seen from the surface of Dione?
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Chapter 17 Solutions
Horizons: Exploring the Universe (MindTap Course List)
Ch. 17 - Prob. 1RQCh. 17 - Why does Mercury have lobate scarps but Earth,...Ch. 17 - What evidence indicates that plate tectonics does...Ch. 17 - Prob. 4RQCh. 17 - Why are the atmospheres of Venus and Mars mostly...Ch. 17 - Prob. 6RQCh. 17 - Prob. 7RQCh. 17 - Why do astronomers conclude that the crust on Mars...Ch. 17 - Prob. 9RQCh. 17 - Prob. 10RQ
Ch. 17 - Prob. 11RQCh. 17 - Prob. 1DQCh. 17 - Imagine that you visit a planet orbiting another...Ch. 17 - Imagine that a spacecraft has landed on Mercury...Ch. 17 - Prob. 2PCh. 17 - The smallest detail visible through Earth-based...Ch. 17 - What is the maximum angular diameter of Phobos as...Ch. 17 - Phobos obits Mars at a distance of 9376 km from...Ch. 17 - Volcano Sif Mons on Venus is shown in the radar...Ch. 17 - Prob. 2LTL
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- If you were to record the spectrum of Saturn as well as the A ring, you would find light from one edge of the rings red shifted and light from the other edge blueshifted. If you observed a spectral line at a wavelength of 500.000 nm, what difference in wavelength should you expect between the opposite edges of the rings? (Hints: See Problem 9, and use the formula for Doppler shift, Eq. 7-3.)arrow_forwardWhat is the maximum angular diameter of the dwarf planet Ceres when it is closest to Earth? Could Earth-based telescopes detect surface features? Could the Hubble Space Telescope? (Hint: Use the small-angle formula, Eq. 3-1.) (Notes: Ceress average distance from the Sun is 2.8 AU and its diameter is 950 km. The best angular resolution of Earth-based telescopes at visual wavelengths is about 1 arc second and of Hubble about 0.1 arc second.)arrow_forwardWhat is the angular size of Phobos observed from Earth when Mars and Earth are at closest approach? Compare that with the resolution limit of about 1 arc second for ground-based telescopes. (Hint: Use the small-angle formula, Eq. 3-1.) (Notes: Necessary data to derive the distance between the objects in that situation are given in the Celestial Profiles for Earth in Chapter 19 and Mars in this chapter. For the size of Phobos, use the maximum dimension given in the text.)arrow_forward
- Calculate the mass of Callisto using a value for its density of 1.8 g/cm3. Convert your answer to units of kg, and compare to the mass of Ganymede given in Problem 5. (Notes: Density is mass divided by volume, and the volume of a sphere is 43r3. Necessary data are given in Appendix Table A-11.) 4. What is the escape velocity from the surface of Ganymede? Ganymedes mass is 1.5 1023 kg and its radius is 2.6 103 km. (Hint: Use the formula for escape velocity, Eq. 5-1b. The formula requires input quantities in kg and m.)arrow_forwardHow are the atmospheres of Earth and Triton similar?arrow_forwardAt what average distances from the Sun would you expect to find Kirkwood gaps where the orbital period of asteroids are respectively one-third, and one-quarter, of the orbital period of Jupiter? Compare your results with Figure 24-9. (Hint: Use Keplers third law, Eq. 4-1.)arrow_forward
- What is the angular diameter of Jupiter as seen from the surface of Callisto? (Hint: Use the small-angle formula, Eq. 3-1) (Note: Necessary data are given in Celestial Profile: Jupiter and Appendix Table A-11.)arrow_forwardWhat is the orbital velocity and period of a ring particle at the outer edge of Saturns A ring? (Hint: Use the formula for circular velocity, Eq. 5-1a. The formula requires input quantities in kg and m.) (Note: The radius of the outer edge of the A ring is 136,500 km.)arrow_forwardThe smallest detail visible through Earth-based telescopes is about 1 arc second in diameter. What linear size does that correspond to on Mercury when Mercury is at a distance of 1 AU? Can Caloris Basin be resolved? (Hint: Use the small-angle formula, Eq. 3-1.) (Note: 1 AU is 1.5 108 km.)arrow_forward
- What is the orbital velocity of Miranda around Uranus? (Hint: Use the formula for circular velocity, Eq. 5-1a. The formula requires input quantities in kg and m.) (Note: Necessary data are given in Celestial Profile: Uranus and Appendix Table A-11.)arrow_forwardWhat is the difference between a centaur and a NEO?arrow_forwardWhat evidence shows that Venus has been resurfaced within the past half-billion years?arrow_forward
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