Polycyclic aromatic hydrocarbons in samples of Ryugu formed in the interstellar medium

Fluoranthene Murchison meteorite Carbonaceous chondrite Polycyclic aromatic hydrocarbon Carbon fibers
DOI: 10.1126/science.adg6304 Publication Date: 2023-12-21T19:03:38Z
ABSTRACT
Polycyclic aromatic hydrocarbons (PAHs) contain ≲20% of the carbon in interstellar medium. They are potentially produced circumstellar environments (at temperatures ≳1000 kelvin), by reactions within cold (~10 kelvin) clouds, or processing carbon-rich dust grains. We report isotopic properties PAHs extracted from samples asteroid Ryugu and meteorite Murchison. The doubly-13C substituted compositions (Δ2×13C values) naphthalene, fluoranthene, pyrene 9 to 51‰ higher than values expected for a stochastic distribution isotopes. Δ2×13C if formed environment, but consistent with formation By contrast, phenanthrene anthracene have higher-temperature reactions.
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