Stars and Galaxies
9th Edition
ISBN: 9781305120785
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Chapter 3, Problem 5LL
To determine
Show that the Moon always keeps the same side facing the Earth.
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The diameter of the Moon is 3500 km. On Figure 2 it is scaled down to 13.2 cm. What is the diameter of Mare Serenitatis, since on Figure 2 it is 2.2 cm? (Show your calculation)
The smallest detail visible through Earth-based telescopes is about 1 arc second in diameter. What linear size is this on the Moon? (Hint: Use the small-angle formula.)
The Mars Robotic Lander for which we are making these calculations is designed to return samples of rock from Mars after a long time of collecting samples, exploring the area around the landing site, and making chemical analyses of rocks and dust in the landing area. One synodic period is required for Earth to be in the same place relative to mars as when it landed.
Calculate the synodic period (in years) using the following formula:
1/Psyn = (1/PEarth) - (1/PMars)
where PEarth is the sidereal period of the Earth (1 year) and PMars is the sidereal period of Mars.
If 3/4 of a Martian year was spent collecting samples and exploring the terrain around the landing site, calculate how long the Mars Robotic Lander expedition took!
Chapter 3 Solutions
Stars and Galaxies
Ch. 3 - Prob. 1RQCh. 3 - Prob. 2RQCh. 3 - Prob. 3RQCh. 3 - Prob. 4RQCh. 3 - Prob. 5RQCh. 3 - Prob. 6RQCh. 3 - Prob. 7RQCh. 3 - Prob. 8RQCh. 3 - Prob. 9RQCh. 3 - Prob. 10RQ
Ch. 3 - Prob. 11RQCh. 3 - Prob. 12RQCh. 3 - Prob. 13RQCh. 3 - Why do solar eclipses happen only at new moon? Why...Ch. 3 - Prob. 15RQCh. 3 - Prob. 16RQCh. 3 - What is the angular diameter of the Moon in the...Ch. 3 - Why cant the Moon be eclipsed when it is halfway...Ch. 3 - Prob. 19RQCh. 3 - Prob. 20RQCh. 3 - Prob. 21RQCh. 3 - Prob. 22RQCh. 3 - Pretend the Moons orbit around Earth is a perfect...Ch. 3 - Prob. 2PCh. 3 - Prob. 3PCh. 3 - Prob. 4PCh. 3 - Prob. 5PCh. 3 - Prob. 6PCh. 3 - Prob. 7PCh. 3 - Prob. 8PCh. 3 - Prob. 9PCh. 3 - Prob. 10PCh. 3 - Prob. 11PCh. 3 - Examine the list of upcoming lunar eclipses in...Ch. 3 - Prob. 13PCh. 3 - Prob. 14PCh. 3 - Prob. 15PCh. 3 - When will the eclipse described in Problem 15 next...Ch. 3 - Prob. 17PCh. 3 - Prob. 18PCh. 3 - Prob. 1LLCh. 3 - Prob. 2LLCh. 3 - Prob. 3LLCh. 3 - Prob. 4LLCh. 3 - Prob. 5LLCh. 3 - Prob. 6LLCh. 3 - Prob. 7LLCh. 3 - Prob. 9LLCh. 3 - Prob. 10LLCh. 3 - Prob. 11LLCh. 3 - Prob. 12LL
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- The smallest detail visible through Earth-based telescopes is about 1 arc second in diameter. What linear size is this on the Moon? (Hint: Use the small-angle formula, Eq. 3-1.)arrow_forwardAgain using Appendix F, which planets might you expect to have extreme seasons? Whyarrow_forwardWhich is the phase of Venus when it is closest? Which when farthest? How do you know?arrow_forward
- What is the angular diameter of Mercury when it is closest to Earth? How does that compare with the angular diameter of the Moon? (Hint: Use the small-angle formula, Eq. 3-1.) (Note: Relevant information can be found in the Celestial Profiles for the Moon and Mercury and Appendix Table A-10.)arrow_forwardAgain using Appendix F, which planet(s) might you expect not to have significant seasonal activity? Why?arrow_forwardAs viewed from Earth, how many times does the Moon rotate during one orbit? As viewed from outside the EarthMoon system, how many times does the Moon rotate in one orbit? How do you know?arrow_forward
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