The inner planets
Formation of the inner planets

Click for larger image The inner, or terrestrial planets (Mercury, Venus, Earth, and Mars) are rocky in composition with densities greater than 3 grams per cubic centimetre (g/cm3). The realm of the inner planets is the region inside the asteroid belt. They lack ring systems, and have few or no satellites. Venus, Earth and Mars have atmospheres, but Mercury is too small and too close to the Sun to hold on to any gases. Among the planets of the inner Solar System, only the Earth has a strong magnetic field and is therefore probably the only planet that still has an active inner core of molten iron and nickel. They all show signs of previous volcanic and geological activity of one form or another.

Formation of the inner planets
Close to the forming Sun, in the pre Solar System gas nebula, the temperature was too high for water and ice to form, while at the distances of Jupiter and beyond, ice could form. The planets forming close to the Sun could not hold onto their lighter more volatile molecules and atoms, leaving the heavier molecules and elements like iron and the silicates to form the inner planets. The formation of the inner planets, including the Earth, was complete within 100 million years of the collapse of the interstellar gas cloud. The bombardment of planetary and satellite surfaces by debris left over from the initial formation of the planets continued for another 600 million years, adding small quantities to the original size of the planets. The surfaces of Mercury and the Moon are witnesses to the ferocity of this age of meteors.

Click for larger image The energy released during meteor impacts was sufficient to cause vaporisation and extensive melting of the planet surfaces, transforming the original surface and producing volcanoes, craters, cracking and mountain formation on the early inner planets. Models of the planet-forming process suggest that several planets the size of the Moon or Mars must have been present in the early inner Solar System in addition to today’s planets. Collisions between the planets and moons would have had dramatic effects and could have produced many hard-to-explain phenomenon such as the high density of Mercury, the thinness of the Martian atmosphere, the retrograde rotation of Venus and formation of our own Moon.

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Origin of the Solar System
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