*Toshihiro Yoshimura1, Yoshinori Takano1, Hiroshi Naraoka2, Toshiki Koga1, Daisuke Araoka3, Nanako O. Ogawa1, Philippe Schmitt-Kopplin4,5, Norbert Hertkorn4, Yasuhiro Oba6, Jason P. Dworkin7, José C. Aponte7, Takaaki Yoshikawa8, Satoru Tanaka9, Naohiko Ohkouchi1, Minako Hashiguchi10, Hannah McLain7, Eric T. Parker7, Saburo Sakai1, Mihoko Yamaguchi11, Takahiro Suzuki11, Tetsuya Yokoyama12, Hisayoshi Yurimoto6, Tomoki Nakamura13, Takaaki Noguchi14, Ryuji Okazaki2, Hikaru Yabuta15, Kanako Sakamoto16, Toru Yada16, Masahiro Nishimura16, Aiko Nakato16, Akiko Miyazaki16, Kasumi Yogata16, Masanao Abe16, Tatsuaki Okada16, Tomohiro Usui16, Makoto Yoshikawa16, Takanao Saiki16, Satoshi Tanaka16, Fuyuto Terui17, Satoru Nakazawa16, Sei-ichiro Watanabe16, Yuichi Tsuda16, Shogo Tachibana18,16, Hayabusa2-initial-analysis SOM team
(1.Japan Agency for Marine-Earth Science and Technology, 2.Kyushu University, 3.National Institute of Advanced Industrial Science and Technology, 4.Helmholtz Zentrum München, 5.Technische Universität München, 6.Hokkaido University, 7.NASA Goddard Space Flight Center, 8.HORIBA Advanced Techno, 9.HORIBA Techno Service Co., 10.Nagoya University, 11.Thermo Fisher Scientific Inc., 12.Tokyo Institute of Technology, 13.Tohoku University, 14.Kyoto University, 15.Hiroshima University, 16.Japan Aerospace Exploration Agency, 17.Kanagawa Institute of Technology, 18.University of Tokyo)
Keywords:Hayabusa 2, Ryugu, sulfur-bearing soluble organic matters, salt
Samples of the carbonaceous asteroid (162173) Ryugu, collected by the Hayabusa 2 spacecraft, provide information on its similarities to CI chondrites and evidence for extensive aqueous alteration (e.g. Yokoyama et al., 2023; Nakamura et al., 2023). There is also evidence that organic matter has also undergone aqueous alteration and that the organic molecules are present as salts on the Ryugu surface (Naraoka et al., 2023). Based on the results of sequential solvent extraction of components with different solubilities, such that salts, carbonates and phyllosilicates (via hot water, formic acid and hydrochloric acid extracts, respectively), this study reports on the elemental distribution of major cations and anions on the Ryugu matrix and the diversity of sulfur-bearing soluble organic molecules. Sodium was the most abundant element (~90%) in the salt fraction of Ryugu, and was probably the main electrolyte when salts were precipitated. Here we show the element partitioning of the major component ions by sequential extractions of salts, carbonates, and phyllosilicate-bearing fractions to reveal primordial brine composition of the primitive asteroid. Sodium is the dominant electrolyte of the salt fraction extract. Anions and NH4+ are more abundant in the salt fraction than in the carbonate and phyllosilicate fractions, with molar concentrations in the order SO42− > Cl− > S2O32− > NO3− > NH4+. The salt fraction extracts contains anionic soluble sulfur-bearing species such as Sn-polythionic acids (n < 6), Cn-alkylsulfonates, alkylthiosulfonates, hydroxyalkylsulfonates, and hydroxyalkylthiosulfonates (n < 7). The sulfur-bearing soluble compounds may have driven the molecular evolution of prebiotic organic material transforming simple organic molecules into hydrophilic and amphiphilic molecules, suggesting that they may have directly influenced the chemical behaviour of organic matter.