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Mercury's Planet

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Mercury is a very rocky planet, its surface is like the Earths moon. It lacks an atmosphere, but experiences extreme temperature anywhere between 90 to 700 Kelvin. It is geologically dead, however it does have a magnetic field which is generated inside the planets core, it magnetic field is only around one 500th of Earths. Mercury is dominated by its core, it has a radius of around 1800 Kilometres and has a less dense mantle which has a depth of 500-600 kilometres. 60 percent of Mercury's mass in inside it's iron core, the ratio of mercury's core volume to the total planet volume is the greatest in the solar system. Mercury always has one side facing the sun so not only is Mercury and the moons surface alike, but they both have one side always …show more content…
However, there are also traces of other elements and compounds like Monoxide, argon, helium and neon. The atmosphere pressure on Venus is over 90 times heavier than that of earths. On Venus closest to its surface there is a thick layer of carbon dioxide, over that layer are layers of clouds of sulphuric acid which reflects over 90 percent of sunlight that hits Venus. The high reflective nature of Venus's clouds is one of the reasons as to why it is the third brightest planet in the solar system, the other reason being it is very close to earth. The temperature on Venus can range from anywhere between negative 364 to positive 870 degrees Fahrenheit. It is the hottest planet in the solar system even though Venus is a lot further away from the sun that mercury. It has been thought and theorised that Venus once had a climate similar to earths, but the runaway gas effects has permanently impacted venus's …show more content…
These two moons are named Phobos and Deimos, Phobos meaning fear and Deimos meaning panic. They orbit really close to mars, only a few tens of kilometres across and there composition is quite unlike that of the planet. These moons are quite difficult to study because they are so close to mars, its hard to distinguish them next to the bright mars. The Mariner and Viking orbiters studied both the moons in greater detail, finding out that they are both irregularly shaped and heavily cratered. The larger of the two moons is Phobos which is around 28 kilometres long, 20 kilometres wide and 10 kilometres wide crater, this crater is named Stickney. Deimos is 16 kilometres long, 10 kilometres wide and its largest crater is 2.3 kilometres in diameter. Both the moons have dark surfaces which reflects not more than 6 percent of the light falling on them which is another reason as to why they are difficult to observe from earth. It is estimated that the masses of the two moons on basis of measurements of their gravitational effect the viking orbiters. The density of the moons are around 2000 kilograms per square meter, it is probably that these moon are asteroids that were slowed and captured by the outer fringes of the early atmosphere of mars or even possible that they are remnants of a single object that broke during capture. Phobos on its low altitude orbit

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