Correct Answer
verified
Multiple Choice
A) Earth and Venus.
B) Mars and Earth.
C) the Moon and Mars.
D) Pluto and the Moon.
E) Ceres and Pluto.
Correct Answer
verified
True/False
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verified
Multiple Choice
A) they must be younger than the older, darker mare.
B) they range from 4.6-4.4 billion years old, on average.
C) the largest impacts are the youngest, such as Copernicus and Tycho.
D) the oldest rocks are at least as old as the mare, but some craters are much younger.
E) most of the asteroids must have hit the Moon, not the Earth.
Correct Answer
verified
Multiple Choice
A) atoms that have been kicked off the surface by the solar wind.
B) volcanic outgassing.
C) residual gases from Mercury's formation.
D) impacts of asteroids or comets.
Correct Answer
verified
Multiple Choice
A) Mercury's is much denser, like Venus, with much carbon dioxide.
B) They are about equal, each only 1% as dense as ours.
C) The cooler Moon retains a thicker nitrogen atmosphere.
D) As no spacecraft has yet landed there, no information exists about Mercury's atmosphere.
E) Neither body has a permanent true atmosphere.
Correct Answer
verified
Multiple Choice
A) The rotational period is longer.
B) The orbital period is longer.
C) The rotational period varies with the Moon's phase.
D) They are equal.
E) The orbital period is greatest at full Moon.
Correct Answer
verified
Essay
Correct Answer
verified
View Answer
Short Answer
Correct Answer
verified
True/False
Correct Answer
verified
Multiple Choice
A) It always keeps one face tidally locked toward the Sun, as our Moon does with us.
B) Its year is much shorter, only 88 days, than its slow rotation of 243 days on its axis.
C) Its rotation rate is 2/3 as long as its year, due to tidal resonances.
D) Its day is the same length as its year.
E) It does not spin at all, being tidal stopped by the solar tides.
Correct Answer
verified
Multiple Choice
A) rays around the latest eruptions
B) craters all over the Moon
C) vents seen erupting in the mountainous highlands
D) rilles associated with lava flows accompanying the mare formation
E) the Orientale Basin
Correct Answer
verified
Multiple Choice
A) every other orbit.
B) all the time, just like our Moon.
C) every 12 hours.
D) every third orbit.
E) twice every orbit.
Correct Answer
verified
Multiple Choice
A) both cores are more iron rich than the rest of the body and the core is solid throughout.
B) both cores are large in proportion to the object with a solid inner core and fluid outer core.
C) both cores are more iron rich than the rest of the body, with a solid inner core and fluid outercore.
D) both cores are small in proportion to the object, with a fluid inner core and solid outer core.
Correct Answer
verified
Multiple Choice
A) the lunar mare are darker than Mercury's intercrater plains.
B) Mercury has "weird terrain" opposite its huge Caloris Basin.
C) Mercury has striking scarps due to the shrinking of its core.
D) Mercury does not always keep the same face toward the Sun, while the Moon does have theEarthside always facing us.
E) All of the above are correct.
Correct Answer
verified
Multiple Choice
A) Mercury is low in iron.
B) Mercury spins too rapidly to produce a stable dynamo.
C) It's still too hot for its core to have differentiated.
D) The dynamo theory predicted that Mercury was spinning too slowly for one.
E) Mercury lacks an iron core.
Correct Answer
verified
Essay
Correct Answer
verified
View Answer
Multiple Choice
A) dynamo action, like the Earth's magnetic field.
B) a mechanism entirely unique to Mercury.
C) being close to the Sun.
D) being a fossil remnant dating back to the distant past when the core was more liquid.
Correct Answer
verified
Essay
Correct Answer
verified
View Answer
Essay
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verified
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