Venus has a highly eccentric orbit, accounting for its large temperature extremes.
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Q6: Like our own, the magnetic field of
Q7: Venus can be seen during daytime when
Q8: Every time the Earth and Venus are
Q9: Venus is almost the same size, mass,
Q10: Venus's surface temperature is fairly uniform, hot
Q12: Venus's rotation period is longer than its
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
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