Erosion on the Earths Moon, Venus and Mercury Assignment - 1

Erosion on the Earths Moon, genus Venus and hydrargyrum - Assignment ExampleIts solid surface and thick crust also support this idea. The right condition why there is so less erosion observed in the surface of Mercury and Venus is that unlike Earth, these planets have no tectonic plates. Since there are no tectonic plates to move with look on to one another, therefore, there remains no room for the energy from the Mantle to escape. Instead, Venus goes through a repetitive process that makes the temperature of the Mantle rise to a critical point, beyond which the crust melts, though it takes instead long for it to renew itself, thereby dissipating whole of the stored heat in the Mantle. Besides, Venus has no moons to produce a tidal effect and accordingly, no erosion results because of a lack of moons gravity. Erosion on the moon is truly less / negligible because there is no wind or precipitation to cause erosion.A planets sizing and its distance from the Sun play a very importa nt role in deciding the gloriole a planet would have. Lets take the example of the planet Earth. Earth is the fifth-largest planet among all and it is two planets (Mercury and Venus) away from the Sun. Unlike many other planets, the huge size of Earth leaves a circularize of room for the heat to accumulate in its interior i. e. the core of Earth. The accumulated heat forces the tectonic plates to sneak past one another so that the heat can be dissipated outside the realm into the atmosphere.Earths geological activity also affects the average temperatures. As a simple example, if there is a colossal volcanic eruption that sends large amounts of dust into the atmosphere, then the dust could block sunlight thereby alter the Earth. (Pandian, 2002).