Abstract
The infrared spectral characteristics of organic-rich acid residues prepared from Ryugu samples returned by the JAXA Hayabusa2 mission generally match those from unheated carbonaceous chondrite meteorites, but the residues from Ryugu are richer in methyl and methylene functional groups and have higher CH2/CH3 ratios. Moreover, two distinct outlier carbonaceous phases are found; one with spectral characteristics of N-H functional groups, likely amides, and a second phase containing less nitrogen. Such infrared characteristics of Ryugu organic matter might indicate the pristine nature of the freshly collected samples and reflect the near-surface chemistry in the parent asteroid.
Original language | English |
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Pages (from-to) | 1845-1858 |
Number of pages | 14 |
Journal | Meteoritics and Planetary Science |
Volume | 59 |
Issue number | 8 |
DOIs | |
Publication status | Published - 2024 Aug |