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Mercury Surface

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The surface of Mercury is very similar to that of Earth's moon. It is covered in a fine sand, much like moon dust, and many craters caused by the impact of asteroids and comets, which have left a debris field around many of these craters. Some of the craters are so deep that, despite the scorching heat on Mercury (over 750 degrees Fahrenheit), its deepest craters and crevices contain ice because they are so deep that they never get any direct sunlight. The surface is also marked by a raisin-like series of ridges, mountains, and valleys that probably occurred when the core of Mercury shrank, effectively wrinkling its surface. There remains evidence of volcanic activity approximately four billion years ago, leaving areas of smooth plains, including …show more content…
These gasses rotate around the planet quickly, creating winds up to 220 miles per hour in the upper atmosphere, but closer to the surface, wind speeds are similar to that on Earth, although the atmospheric pressure on Venus is quite a bit higher than on Earth -- so high that much of the carbon dioxide on Venus is no longer a gas, but a fluid that forms a sort of "sea" on the planet's surface. The large amounts of carbon dioxide have created a runaway greenhouse effect that brings surface temperatures up as high as 873 degrees Fahrenheit, making Venus the hottest planet in the Solar System, despite the fact that Mercury is closer to the Sun and that much of the Sun's heat and light fail to make it through the thick Venusian atmosphere. Due to this thick atmospheric cover, the temperature on Venus changes very little throughout the year or between day and …show more content…
They were discovered is 1877 and named after the sons of Ares in Greek mythology. Ares was the God of War. His sons, Phobos (which means "fear") and Deimos (which means "dread"), accompanied their father into battle against the war goddess, Enyo. The moon Phobos is seven times larger than the moon Deimos. Phobos orbits closer to Mars and, in fact, it orbits the closest to its planet of any known moon. It is moving closer and closer to Mars and is predicted to collide with Mars within 50 million years. Phobos orbits Mars about twice as fast as Deimos, creating full lunar eclipses virtually every Martian day. Both moons are heavily cratered (Phobos more so of the two) and non-spherical, with low mass, low gravity, and no atmosphere. They are comprised of material too light and porous to be rock, and believed to be the carbonaceous material of

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