Venus' temperature is fairly uniform over the entire planet,both day and night.
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Q3: Venus has larger volcanoes than Earth's Hawaii.
Q9: The cause of Venus' slow rotation is
Q11: Venus has a highly eccentric orbit, accounting
Q11: Venus can be seen during daytime when
Q13: Carbon dioxide is the predominant atmospheric gas
Q14: The actual slow rotation of Venus was
Q15: As on Earth, continent-like landmasses cover over
Q16: Venus can appear as a crescent through
Q17: The terra of Venus are rare, but
Q20: The clouds of Venus are much higher
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