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In the case of our solar system, the formation of the planets may have been influenced by the different snow lines at different orbital distances from the sun. During the protoplanetary phase of the sun, frozen volatiles at certain snow lines would have given the protoplanetary dust a sticky outer layer, potentially accelerating planet formation through the process of agglomeration. For example, the water snow line for the sun can be found between the orbits of Mars and Jupiter; the CO snow line is at the orbit of Neptune. How does this factor into planetary formation at those distances?
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Author: - Kirjoittanut: Anonymous, 01/22/2020, |