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SUPERROTATION – The fast-moving winds in Venus’ upper atmosphere, circling the planet in just a few days.

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MAGELLAN MISSION – A NASA mission that mapped Venus’ surface using radar.

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IMPACT CRATERS – Unlike Earth, Venus has relatively few impact craters because its dense atmosphere burns up many incoming meteoroids.

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TESSERAE – Complex, deformed regions on Venus’ surface that are thought to be tectonically active.

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VOLCANISM ON VENUS – Venus has a surface dominated by volcanic activity, with large shield volcanoes like Maat Mons.

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DAY LENGTH ON VENUS – A Venusian day (one full rotation) is longer than its year due to its slow rotation.

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RETROGRADE ROTATION – The phenomenon where Venus rotates in the opposite direction to most planets, including Earth.

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SULFURIC ACID CLOUDS – Clouds composed of sulfuric acid droplets that reflect sunlight and contribute to Venus’ high albedo.

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SURFACE PRESSURE – The pressure exerted by Venus’ dense atmosphere, which is about 92 times that of Earth’s.

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RUNAWAY GREENHOUSE EFFECT – A process in which a planet’s atmosphere becomes so thick with greenhouse gases that temperatures continuously rise, as seen on Venus.