


Study with the several resources on Docsity
Earn points by helping other students or get them with a premium plan
Prepare for your exams
Study with the several resources on Docsity
Earn points to download
Earn points by helping other students or get them with a premium plan
In the mid-nineteenth century, astronomers thought that Mercury should be tidally locked to the Sun, meaning it would rotate once for every revolution around the Sun. This scenario would be similar to how the Moon is tidally locked in its orbit around Earth. However in the 1960s, astronomers determined that Mercury is not tidally locked to the Sun. The large eccentricity (exaggerated in the figure) of Mercury's orbit causes large variations in its orbital speed, which prevents tidal locking.
Typology: Assignments
1 / 4
This page cannot be seen from the preview
Don't miss anything!



Part A The Moon has two distinct types of terrain: the maria and the highlands. On the image of the Moon below, label the specified regions as either maria or highlands. Part B The Moon's maria and highlands can be described by the characteristics present in each. Sort the following characteristics by whether they describe the maria or the highlands.
Part C The relative number of craters found in the maria and the highlands greatly differs. In addition, we have inferred that the maria formed from molten lava welling up from the Moon's mantle. Use this information to rank the following images of lunar regions in order of relative age, from oldest to youngest.
Part A Compare the magnitude of the Sun's gravitational force on Mercury at locations A, B, and C. (Figure not to scale.) Part B In the mid-nineteenth century, astronomers thought that Mercury should be tidally locked to the Sun, meaning it would rotate once for every revolution around the Sun. This scenario would be similar to how the Moon is tidally locked in its orbit around Earth. However in the 1960s, astronomers determined that Mercury is not tidally locked to the Sun. The large eccentricity (exaggerated in the figure) of Mercury's orbit causes large variations in its orbital speed, which prevents tidal locking. Rank the following orbital locations from the fastest orbital speed to the slowest.
Part B A theory is a framework of ideas and assumptions used to explain some set of observations and to make predictions about the real world. Each of the three theories for the formation of the Moon lead to different predictions about evidence that we should find. Which of the following predictions should be true if each theory is correct? Part C To be effective, a scientific theory must be continually tested. If observations and experiments favor it, a theory can be further developed and refined. If they do not, the theory must be reformulated or rejected. Comparing what you know about the predictions of each Moon formation theory, determine which of the following observations and experiments have been verified. Earth has a large iron core; the Moon does not. The mantles of Earth and the Moon have similar compositions. Computer simulations predict that a collision between Earth and a Mars-sized object would produce a Moon-sized satellite with a stable orbit. Part D Based on the evidence for the impact theory, what was the most probable order of events for the collision that led to the formation of the Moon?