Ryugu asteroid origins in the solar nebula decoded by carbonates

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Ryugu asteroid origins in the solar nebula decoded by carbonates
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Japan's Aerospace Exploration Agency sent the Hayabusa2 spacecraft to 162173 Ryugu in 2019, an asteroid in orbit near Earth that is comprised of rocky fragments originating from a larger parent body. Multiple rovers brought samples from the asteroid's surface back down to Earth for scientists to study.

C-rich compounds are preferentially released , 2) fractional crystallization where the formation of early carbonates changes the composition of the remaining reservoir from which subsequent carbonates can crystallize, 3) mixing of multiple carbon reservoirs with differentC ratios, and 4) varying oxygen and hydrogen caused changes in the isotopes forming carbon monoxide, carbon dioxide and methane, from which carbon is obtained for the crystals.

Similarly, fractional crystallization is ruled out, as is mixing ofTherefore, it is the latter scenario of varying oxygen that is suggested as the main driver of changes inC ratios. This resulted from the oxidation of iron in the rock by water and is measured based upon the production of hydrogen released from the water. The hypothesis matches observations of increasing iron in the meteorite with progressive alteration.

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