Exam 8: The Other Terrestrial Planets

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Suppose Mercury had oceans. What would be the length of time between successive high tides?

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Where did some scientists claim that they have found direct evidence for life, either contemporary or ancient, beyond Earth that has since been disproven?

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Suppose Mercury had 5-to-3 spin-orbit coupling and that its sidereal period remained 88 days, as now. An observer sees the Sun directly overhead in the Mercurian sky and then observes again from the same location 88 days later. Where will the Sun be in the sky? (Mercury, like Earth, rotates toward the east.)

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What is the "face" on Mars?

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How does the number of impact craters seen on Venus compare with the number seen on Mercury and the Moon, both of which are significantly smaller than Venus?

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The surface pressure of the atmosphere of Venus compared with the surface pressure of the atmosphere of Earth is

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When Venus is at its brightest as seen from Earth (near greatest elongation), it is

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The gas that is the major constituent of the atmospheres of Venus and Mars and a minor constituent of Earth's atmosphere is

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How have planetary scientists obtained samples of Martian rocks?

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The severe atmospheric conditions that quickly destroyed spacecraft that soft-landed on the surface of Venus were

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Mars has one hemisphere that is at a higher elevation than the other. In this way, it is similar to

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Both impact craters and dormant volcanoes have been found on Mars. Where are they?

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The planet with the highest overall density is

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Where in the solar system did the Viking spacecraft land?

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Which particular chemical associated with volcanic emissions exists in short-lived compounds but has been detected on Venus, indicating the possibility of active volcanoes on that plaent at the present time?

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Which of these is NOT a legitimate reason to believe that the northern hemisphere of Mars has experienced more geologic activity than the southern hemisphere?

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Which of these correctly describes aurorae on Mars?

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Earth and Mars each has about the same tilt of its spin axis with respect to its orbital plane. Earth experiences precession, which causes the DIRECTION of its spin axis to change slowly over time, but the ANGLE of tilt stays relatively constant. By contrast, the ANGLE of tilt of Mars's spin axis is NOT expected to be stable over long periods of time. Which of these is a potential explanation for this?

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Mercury can be characterized as having

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Temperatures on the surface of Mercury are seen to fluctuate between very cold 100 K (-173°C) and extremely hot 700 K (427°C). What does this measurement indicate about conditions on Mercury?

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