Foundations of Astronomy
13th Edition
ISBN: 9781305079151
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Chapter 21, Problem 7P
The trenches where Earth’s seafloor slips downward are 1 km or less wide. Could Earth-based telescopes resolve such features on the Moon? Why can you be sure that such features are not present on the Moon? (Hint: Use the small-angle formula, Eq. 3-1.) (Note: Relevant information can be found in Celestial Profile: The Moon.)
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Chapter 21 Solutions
Foundations of Astronomy
Ch. 21 - How does the force of gravity cause tidal coupling...Ch. 21 - As viewed from Earth, how many times does the Moon...Ch. 21 - If the Moon is tidally coupled to Earth, is Earth...Ch. 21 - How can you determine the relative ages of the...Ch. 21 - From looking at images of the Moons near side, how...Ch. 21 - Why did the first Apollo missions land on the...Ch. 21 - Why do planetary scientists hypothesize that the...Ch. 21 - Prob. 8RQCh. 21 - Prob. 9RQCh. 21 - Prob. 10RQ
Ch. 21 - What is the most significant kind of erosion that...Ch. 21 - Provide evidence to support a hypothesis about...Ch. 21 - What evidence can you cite that the Moon had...Ch. 21 - What evidence would you expect to find on the Moon...Ch. 21 - How does the large-impact hypothesis explain the...Ch. 21 - Look at the Celestial Profiles for Earth, the...Ch. 21 - Look at the Celestial Profiles for the Moon and...Ch. 21 - Prob. 18RQCh. 21 - Look at the Celestial Profiles for Earth, the...Ch. 21 - Look at the Celestial Profiles for the Moon and...Ch. 21 - Why are features like the Moons maria not observed...Ch. 21 - What are the relative ages of the intercrater...Ch. 21 - What evidence can you give that Mercury has a...Ch. 21 - Why is it not surprising that there is no evidence...Ch. 21 - What evidence can you give that Mercury had...Ch. 21 - How are the histories of the Moon and Mercury...Ch. 21 - What property of the Moon and Mercury has resulted...Ch. 21 - Prob. 28RQCh. 21 - Prob. 1DQCh. 21 - Prob. 2DQCh. 21 - Prob. 3DQCh. 21 - Prob. 4DQCh. 21 - Look at the right top and bottom images in Figure...Ch. 21 - Calculate the escape velocity of the Moon from its...Ch. 21 - Prob. 3PCh. 21 - Why do small planets cool faster than large...Ch. 21 - The smallest detail visible through Earth-based...Ch. 21 - Prob. 6PCh. 21 - The trenches where Earths seafloor slips downward...Ch. 21 - An Apollo command module orbited the Moon about...Ch. 21 - Prob. 9PCh. 21 - What is the angular diameter of Mercury when it is...Ch. 21 - If you transmit radio signals to Mercury when...Ch. 21 - What is the wavelength of the most intense...Ch. 21 - Suppose you send a probe to land on Mercury, and...Ch. 21 - The smallest detail visible through Earth-based...Ch. 21 - Look at the image of the astronaut on the Moon at...Ch. 21 - Examine the shape of the horizon at the Apollo 17...Ch. 21 - In the photo shown here, astronaut Alan Bean works...
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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_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 maximum angular diameter of Venus as seen from Earth? (Hint: Use the small-angle formula, Eq. 3-1.) (Note: Necessary data to derive the distance between the objects in that situation are given in the Celestial Profiles for Earth in Chapter 19 and Venus in this chapter.)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_forwardWhy is Mars red?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
- The unaided human eye has a resolution of about 100 arc seconds in bright lighting conditions. Could someone looking out the command module window have seen the astronauts on the Moon yes or no?arrow_forwardJupiter's moon Metis has a radius of only 20 km, and a mass of 9 x 1016 kg. Answer the following: a) Calculate this moon's average density. b) Based on your result above, would you say that Metis is made primarily of rock or ice? Justify your answer. (Hint: Density of ice is 920 kg/m3)arrow_forwardThe iron meteorite that created Barringer Crater (Arizona) was 50 m in diameter. It caused a crater 1.2 km (1200 m) in diameter, that is, 24 times bigger than the impactor. Keeping in mind that the size of the crater depends on many factors, such as the type of rocks present in the area, estimate the approximate size of the impactor that produced Mare Serenitatis.arrow_forward
- In the previous lab, we calculated the area in between Mars' and Jupiter's orbit to be ~1.6e18 km2. Since there are roughly 750,000 asteroids, how much area (in km2) is available for one asteroid? Use this calculation to argue whether you are likely (or not) to hit an asteroid while flying through the asteroid belt. (Hint: To answer the first part of the question, find the area per asteroid)arrow_forwardNo handwrittenarrow_forwardKnowing Earth’s rotational frequency W = 7.3 x 10-5 s-1 and the characteristic frequency 1/T=U/L of a particular oceanic motion based on its velocity (U), temporal (T) and spatial (L) scales, a) What is the non-dimensional Rossby Number and What does it mean if this parameter value is lower than one?arrow_forward
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