AI Article Synopsis

  • The analysis of samples from the asteroid Ryugu reveals a rich diversity of soluble organic molecules, indicating complex chemistry on this C-type asteroid.
  • The study utilizes methods like mass spectrometry and nuclear magnetic resonance spectroscopy to explore the molecular characteristics of the samples, highlighting various polarities and sizes.
  • Findings suggest a water-rich environment for Ryugu's parent body, evidenced by compounds like ammonium ions and sulfidic substances, pointing to processes like carbonization and low-temperature aqueous alteration that contribute to the organic complexity.

Article Abstract

The sample from the near-Earth carbonaceous asteroid (162173) Ryugu is analyzed in the context of carbonaceous meteorites soluble organic matter. The analysis of soluble molecules of samples collected by the Hayabusa2 spacecraft shines light on an extremely high molecular diversity on the C-type asteroid. Sequential solvent extracts of increasing polarity of Ryugu samples are analyzed using mass spectrometry with complementary ionization methods and structural information confirmed by nuclear magnetic resonance spectroscopy. Here we show a continuum in the molecular size and polarity, and no organomagnesium molecules are detected, reflecting a low temperature and water-rich environment on the parent body approving earlier mineralogical and chemical data. High abundance of sulfidic and nitrogen rich compounds as well as high abundance of ammonium ions confirm the water processing. Polycyclic aromatic hydrocarbons are also detected in a structural continuum of carbon saturations and oxidations, implying multiple origins of the observed organic complexity, thus involving generic processes such as earlier carbonization and serpentinization with successive low temperature aqueous alteration.

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Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC10579312PMC
http://dx.doi.org/10.1038/s41467-023-42075-yDOI Listing

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