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Scientists have analyzed the volcanic past of Mars, using samples of Martian meteorites.On Earth, most of the volcanic processes occur as a result of plate tectonics, which, in turn, is provided by convection in the mantle of the Earth.The mass spectrometer allows us to determine how much argon has accumulated in the samples – it is the result of the natural radioactive decay of potassium.The results of the analysis showed that the volcanic history of Mars went completely different than the earth’s.It is also located in 2000 kilometers to the north of the place where the rover “Curiosity” is now located.At NASA’s disposal, therefore, there are amazingly detailed satellite images of this particular crater.Because of this, the Martian volcanoes (although morphologically similar to the shield volcanoes of the Earth) have grown to much larger sizes than their terrestrial counterparts.For example, Mount Olympus is not only the largest shield volcano on Mars, but also in the solar system.

IEC 60601-2-09 has been developed for use with the third edition of IEC 60601-1 (2005) and its collateral standards.Millions of years ago, the planet also had a certain volcanic activity, which allowed the formation of massive faults and mountains – like Mount Olympus, the largest volcano in the solar system.Until recently, scientists believed that the Martian volcanic activity is controlled by sources other than a tectonic movement that the planet had not had for billions of years.But on Mars, most of the volcanic activity is the result of mantle plumes, which are highly localized upwelling magma rising from the depths of the mantle.This is due to the fact that the surface of Mars remained still and cool during the last several billion years.

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