Explain why moonquakes occur more frequently when the Moon is at perigee than at other locations along its orbit.

Short Answer

Expert verified
Moonquakes occur more frequently during perigee because the gravitational pull from Earth, which causes tidal stresses on the Moon's surface leading to moonquakes, is the strongest at this point in the Moon's orbit.

Step by step solution

01

Defining terms

First, define some key terms which will help to better evaluate the main problem. Moonquakes refer to seismic activities similar to earthquakes but occurring on the moon. Perigee is the point in the Moon's orbit when it is closest to Earth.
02

Understanding the Moon-Earth relationship

The Moon is tied to Earth by gravity. As the Moon orbits the Earth, the gravitational pull exerted by the Earth changes with the Moon's position. This gravitational force is strongest when the Moon is at perigee or the point where it is closest to Earth.
03

Linking the phenomena

The increased gravitational pull from Earth when the Moon is at perigee results in significant tidal stress on the Moon's surface. These stresses give rise to moonquakes.
04

Conclusion

So, moonquakes occur more frequently when the Moon is at perigee because the gravitational pull from Earth is strongest at this point, leading to greater tidal stresses.

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Most popular questions from this chapter

How would our theories of the Moon's history have been affected if astronauts had discovered sedimentary rock on the Moon?

Use the Starry Night Enthusiast \({ }^{\mathrm{TM}}\) program to observe the apparent change in size of the Moon as seen from the surface of the Earth. Click the Home button in the toolbar. Stop the time flow by clicking the Stop time button (the button with a square icon in the Time Flow Rate section of the toolbar). Click each field of the Time and Date display pane in the toolbar and use the keyboard to set the time to \(12: 00: 00 \mathrm{~A} . \mathrm{M}\). and the date to \(\mathrm{O}\) tober 16,2006 . You can now set up the view of the Moon as if you were observing from a transparent Earth in continuous darkness. Open the Options pane by clicking its tab on the left border of the view window. In the Local View layer of the Options pane, uncheck the boxes beside the Daylight and Local Horizon options. Open the Find pane and click the menu button at the left of the entry for the Moon and select Magnify from the menu to display a stationary image of the magnified Moon in the center of the view. Notice the Moon's phase. (a) Select Options > Solar System > PlanetsMoons... from the menu. In the Planets-Moons dialog box, click the slide control next to the Show dark side label near the top of the window and adjust the control all the way to the right (Brighter) side of the scale. Then click the OK button to close the dialog box. Note that the image of the Moon now appears full because Starry Night Enthusiast TM has artificially brightened the dark side of the image of the Moon, effectively removing the appearance of the Moon's phases. (b) Use the + button in the Zoom section of the toolbar to adjust the field of view to about \(55^{\prime} \times 45^{\prime}\). Starry Night Enthusiast \({ }^{\mathrm{TM}}\) can display a reference field of view (FOV) upon this sky. Open the FOV pane by clicking its tab. Select the 30 Arcminutes option. Then click the FOV tab to close the pane. (c) The final view is of the Moon, its dark side artificially brightened, as it would be seen from your home location if the Earth were airless and transparent, surrounded by a yellow FOV circle 30 arcminutes in diameter. Note the size of the Moon relative to this reference circle. Set the Time Flow Rate in the toolbar to 1 minute. Run Time Forward for least 24 hours and observe the apparent size of the Moon relative to the reference circle. (c) Note that the apparent size of the Moon changes somewhat over the course of a day (of simulated time). Explain in terms of the Earth's rotation. (Hint: In this view, Starry Night Enthusiast \({ }^{\text {Tm }}\) has made the Earth transparent, so you can see objects that would normally be below the horizon. As the Earth rotates, your observing location on the surface is carried along and your distance from the Moon changes.) (d) Change the Time Flow Rate to 1 day and again click the Run Time Forward button. Does the apparent size of the Moon always stay the same, or does it vary? Explain what this tells you about the shape of the Moon's orbit.

If the Moon always keeps the same face toward the Earth, how is it possible for Earth observers to see more than half of the Moon's surface?

Describe the evidence that (a) the Moon has a more solid interior than the Earth and (b) the Moon's interior is not completely solid.

Describe the differences between the maria and the lunar highlands. Which kind of terrain covers more of the Moon's surface? Which kind of terrain is more heavily cratered? Which kind of terrain was formed later in the Moon's history? How do we know?

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