Unit 2 Chpt 8: Moon & Mercury

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20 Terms

1
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In relation to the density of Earth's Moon, Mercury's density suggests that the planet

has a dense metal core.

2
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Compared with the phases of Earth's Moon, Mercury goes from new phase to full phase

more slowly.

3
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Compared with the diameter of Earth's Moon, the diameter of Mercury is

larger.

4
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Compared with the surface of Mercury, the surface of Earth's Moon has significantly

more maria.

5
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Every two times Earth's Moon rotates on its axis, it orbits Earth

exactly two times.

6
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Determine a synchronous orbit.

A synchronous orbit is a situation where an orbiting body spins exactly once for every one time it orbits its parent body.

7
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Why does the Moon have a synchronous orbit around the Earth?

The Moon have the synchronous orbit because, over hundreds of millions of years, tidal forces from Earth have been tugging on the Moon, producing a “drag” that has slowed down the Moon’s spin until one side of the Moon was always facing the Earth.

8
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Planets and moons showing the most craters have

the oldest surfaces.

9
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Compared with the Moon, Mercury has

much larger core.

10
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The most likely theory of the formation of Earth's Moon is that it

formed from a collision of Earth with a Mars-sized object.

11
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On the scale of the 5-billion-year age of the solar system, the Moon is

about the same age as Earth.

12
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Mercury, being smaller than Mars, probably cooled and solidified

faster, because it is smaller.

13
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What is the reason that it is so difficult to view Mercury from Earth?

Mercury is always very close to the Sun.

14
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Mercury has the widest variation in surface temperatures between night and day of any planet in the solar system.

True

15
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What is true of the lunar highlands?


They are the oldest part of the lunar surface.

16
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How does Mercury's rotation relate to the Sun?

Its rotation rate is 2/3 as long as its year, due to tidal resonances.

17
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Mercury presents the same side to the Sun:


every other orbit.

18
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Which of these features is attributed to the shrinking of Mercury's core?

scarps

19
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Mercury's Caloris Basin is aptly named, since:

it is the hottest region, turning to face the Sun when Mercury is at perihelion.

20
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Mercury's evolution was different from the Moon's because:

dense Mercury had an iron core that shrank, creating the lobate scarps.