Venus has a relatively thin crust that undergoes wrinkling and flaking;this model is called "flake tectonics."
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Q6: Venus's atmosphere is extremely hot and dense.
Q7: Opposite the Caloris Basin,a huge crater on
Q8: Venus appears almost completely featureless with neither
Q9: Valles Marineris on Mars is thought to
Q10: No spacecraft have successfully landed on the
Q12: Mars's atmosphere experiences a runaway icehouse effect
Q13: Hot-spot volcanoes on Earth are only found
Q14: Mercury's scarps,numerous long cliffs,were probably formed as
Q15: Jupiter's moon,Io,may have as many as 300
Q16: Mars's atmosphere has always been thin and
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