Seen from Earth shining brightly in the west at sunset, Venus is called the evening star. It is a rocky planet, and the second-closest planet to the Sun.
Table 6. VENUS DATA
| Diameter (width) at equator | 7,521 miles (12,104 km)
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| Average distance from Sun | 67.2 million miles (108.2 million km)
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| Time to orbit Sun | 224.7 days
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| Time to spin around own axis | 243 days
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| Mass | 0.82 x Earth’s mass
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| Gravity | 0.9 x Earth’s gravity
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| Average surface temperature | 867°F (464°C)
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| Number of moons | 0 |
WHY CAN’T WE SEE VENUS’S SURFACE?
Thick clouds in Venus’s atmosphere stop us from seeing the surface. Radar probes, such as Magellan, can peer through the clouds, revealing a planet dotted with volcanoes and covered with rolling lava plains.
Temperatures on Venus soar to over 860°F (460°C), making it hotter than any other planet. Its carbon dioxide atmosphere, which is 100 times heavier than Earth’s, traps heat like a greenhouse.