Using sophisticated computer simulations, team has discovered new insights into the chemical composition of the dust grains that formed in the solar system 4.5 billion years ago. Researchers from Swinburne Uni of Technology, Melbourne and the Uni of Lyon, France, calculated a 2D map of the dust chemistry in the solar nebula, the thin dusty disk that surrounded the young sun and out of which the planet formed.
It is expected that refractories (high temperature materials) should be located close to the young sun, while volatile materials (such as ices and sulphur compounds) should form far from the sun where temperatures are cooler...
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