Chondritic unfractionated reservoir
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The CHondritic Unfractionated Reservoir or CHUR is a scientific model in astrophysics and geochemistry for the mean chemical composition of the part of the Solar Nebula from which, during the formation of the Solar System, chondrites formed. This hypothetic chemical reservoir is thought to have been similar in composition to the current photosphere of the Sun.
When the Sun formed from its protostar, around 4.56 billion years ago, the solar wind blew all gas particles from the central part of the Solar Nebula. In this way most lighter volatile elements (e.g. hydrogen, helium, oxygen, carbon), that had not yet condensed in the inner, warmer regions of the nebula, were lost. This fractionation process is the reason why the terrestrial planets and asteroid belt are relatively enriched in heavy elements in respect to the Sun or the gas planets.
A certain type of meteorites, C1-chondrites, have a chemical composition that is almost identical to the solar atmosphere (the photosphere), except for the abundances of light volatile elements. They are considered to have the same composition as the solar nebula after the solar wind fractionated the lighter elements and therefore are representative for the material from which the terrestrial planets, including the Earth, were formed.
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