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Mercury Surface Essay

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One of the most distinct features of Mercury’s surface is the fact that it looks wrinkled: this is due to the cooling of the planet’s iron core which led to the surface contracting. Mercury lost a third of its radius during this process (was reduced from 1.8 to 1.2 miles). Named “Scarps” by scientists, the wrinkles can be up to one mile high, and stretch over numerous miles.

Another particularity of Mercury is that it is covered in craters, making it the most cratered planet in the entire Solar System. All of these craters strongly vary in shape and size, and originate from numerous encounters with comets and meteoroids. The largest one, Caloris Basin which was discovered in 1974, has a diameter of 1.550 kilometres and is surrounded by a …show more content…
All other compounds only exist in very small amounts, such as hydrogen chloride and hydrogen fluoride. The surface temperature can reach 462 °C / 863 °F, which makes Venus the hottest planet in the entire Solar System. There are no significant changes in terms of temperature between day and night, which makes it impossible for any life to live on the surface of …show more content…
The exact number cannot be stated, as this depends on how they are defined, but the major ones are the African, Antarctic, Eurasian, North American, South American, Pacific and Indo-Australian, as well as numerous smaller ones. While the plates that is moving the fastest are the Oceanic and Pacific plates, the Eurasian plate only moves about 21 mm per year and is therefore the slowest one. Generally, movement paces can differ between 0 and 100 mm in a year. These tectonic plates consist of oceanic lithosphere and rather thick continental lithosphere, and are surrounded by an individual crust

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