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GREENHOUSE EFFECT – The trapping of heat by a planet’s atmosphere, significantly stronger on Venus than on Earth.

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VENUSIAN ATMOSPHERE – A thick atmosphere composed mainly of carbon dioxide with clouds of sulfuric acid, creating an extreme greenhouse effect.

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VENUS: EARTH’S TWIN?

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POLAR ICE – Despite Mercury’s extreme temperatures, there are deposits of water ice near its poles, protected from the Sun’s heat by deep craters.

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SURFACE COMPOSITION – Mercury’s surface is rich in metal and rock, with large amounts of iron and sulfur.

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TEMPERATURE VARIATIONS – Due to its lack of atmosphere and proximity to the Sun, Mercury experiences some of the most extreme temperature differences in the solar system.

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EXOSPHERE – The thin, rarefied atmosphere of Mercury, composed of atoms and molecules that are constantly escaping into space.

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TIDAL LOCKING – Mercury is in a state of orbital resonance where it rotates three times on its axis for every two revolutions around the Sun.

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MESSENGER MISSION – NASA’s spacecraft that orbited Mercury between 2011 and 2015, gathering detailed information about the planet’s surface, magnetic field, and atmosphere.

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SURFACE GRAVITY – Mercury’s surface gravity is 38% of Earth’s, due to its smaller size and mass.