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. 2023 Dec 22;382(6677):1411-1416.
doi: 10.1126/science.adg6304. Epub 2023 Dec 21.

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

Sarah S Zeichner  1 José C Aponte  2 Surjyendu Bhattacharjee  1 Guannan Dong  1 Amy E Hofmann  1   3 Jason P Dworkin  2 Daniel P Glavin  2 Jamie E Elsila  2 Heather V Graham  2 Hiroshi Naraoka  4 Yoshinori Takano  5 Shogo Tachibana  6   7 A. Tyler Karp  8   9   10 Kliti Grice  11 Alex I Holman  11 Katherine H Freeman  8 Hisayoshi Yurimoto  12 Tomoki Nakamura  13 Takaaki Noguchi  14 Ryuji Okazaki  4 Hikaru Yabuta  15 Kanako Sakamoto  7 Toru Yada  7 Masahiro Nishimura  7 Aiko Nakato  7 Akiko Miyazaki  7 Kasumi Yogata  7 Masanao Abe  7   16 Tatsuaki Okada  6   17 Tomohiro Usui  6   7 Makoto Yoshikawa  7   16 Takanao Saiki  7 Satoshi Tanaka  7   16 Fuyuto Terui  18 Satoru Nakazawa  7 Sei-Ichiro Watanabe  19 Yuichi Tsuda  7 Kenji Hamase  20 Kazuhiko Fukushima  21 Dan Aoki  21 Minako Hashiguchi  19 Hajime Mita  22 Yoshito Chikaraishi  23 Naohiko Ohkouchi  5 Nanako O Ogawa  5 Saburo Sakai  5 Eric T Parker  2 Hannah L McLain  2 Francois-Regis Orthous-Daunay  24 Véronique Vuitton  24 Cédric Wolters  24 Philippe Schmitt-Kopplin  25   26   27 Norbert Hertkorn  25   28 Roland Thissen  29 Alexander Ruf  30   31   32 Junko Isa  33   34 Yasuhiro Oba  23 Toshiki Koga  5 Toshihiro Yoshimura  5 Daisuke Araoka  35 Haruna Sugahara  7 Aogu Furusho  36 Yoshihiro Furukawa  13 Junken Aoki  37 Kuniyuki Kano  37 Shin-Ichiro M Nomura  38 Kazunori Sasaki  39   40 Hajime Sato  40 Takaaki Yoshikawa  41 Satoru Tanaka  42 Mayu Morita  42 Morihiko Onose  42 Fumie Kabashima  43 Kosuke Fujishima  33   44 Tomoya Yamazaki  23 Yuki Kimura  23 John M Eiler  1
Affiliations

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

Sarah S Zeichner et al. Science. .

Abstract

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

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