Multiple Choice
What can we say about the abundance of volatile materials on Mercury?
A) The observed abundance of volatile materials is low. This is consistent with Mercury's formation close to the Sun, where volatile materials would be "boiled out" of the solar system.
B) The observed abundance of volatile materials is low. This is consistent with a large planetesimal striking Mercury and taking away the outer mantle-the usual explanation for Mercury's large iron core.
C) The observed abundance of volatile materials is low. This is consistent with the outer mantle of Mercury being stripped away in just a few minutes due to a large impact.
D) The observed abundance of volatile materials is high. This is inconsistent with Mercury's formation close to the Sun.
Correct Answer:

Verified
Correct Answer:
Verified
Q36: The surface temperature of Venus was first
Q37: What can be said about the presence
Q38: Mars rotates toward the east and takes
Q39: Deimos remains over almost the same spot
Q40: What was required to obtain a visible-light
Q42: The circulation pattern in Venus's atmosphere consists
Q43: How did optical illusion mislead early visual
Q44: Phobos and Deimos, the two moons of
Q45: Venus and Earth are about the same
Q46: To what does the phrase "synchronous rotation"