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@ARTICLE{Nakamura:485848,
      author       = {Nakamura, T. and Matsumoto, M. and Amano, K. and Enokido,
                      Y. and Zolensky, M. E. and Mikouchi, T. and Genda, H. and
                      Tanaka, S. and Zolotov, M. Y. and Kurosawa, K. and Wakita,
                      S. and Hyodo, R. and Nagano, H. and Nakashima, D. and
                      Takahashi, Y. and Fujioka, Y. and Kikuiri, M. and Kagawa, E.
                      and Matsuoka, M. and Brearley, A. J. and Tsuchiyama, A. and
                      Uesugi, M. and Matsuno, J. and Kimura, Y. and Sato, M. and
                      Milliken, R. E. and Tatsumi, E. and Sugita, S. and Hiroi, T.
                      and Kitazato, K. and Brownlee, D. and Joswiak, D. J. and
                      Takahashi, M. and Ninomiya, K. and Takahashi, T. and Osawa,
                      T. and Terada, K. and Brenker, F. E. and Tkalcec, B. J. and
                      Vincze, L. and Brunetto, R. and Aléon-Toppani, A. and Chan,
                      Q. H. S. and Roskosz, M. and Viennet, J.-C. and Beck, P. and
                      Alp, E. E. and Michikami, T. and Nagaashi, Y. and Tsuji, T.
                      and Ino, Y. and Martinez, J. and Han, J. and Dolocan, A. and
                      Bodnar, R. J. and Tanaka, M. and Yoshida, H. and Sugiyama,
                      K. and King, A. J. and Fukushi, K. and Suga, H. and
                      Yamashita, S. and Kawai, T. and Inoue, K. and Nakato, A. and
                      Noguchi, T. and Vilas, F. and Hendrix, A. R. and
                      Jaramillo-Correa, C. and Domingue, D. L. and Dominguez, G.
                      and Gainsforth, Z. and Engrand, C. and Duprat, J. and
                      Russell, S. S. and Bonato, Alessio and Ma, C. and Kawamoto,
                      T. and Wada, T. and Watanabe, S. and Endo, R. and Enju, S.
                      and Riu, L. and Rubino, S. and Tack, P. and Takeshita, S.
                      and Takeichi, Y. and Takeuchi, A. and Takigawa, A. and
                      Takir, D. and Tanigaki, T. and Taniguchi, A. and Tsukamoto,
                      K. and Yagi, T. and Yamada, S. and Yamamoto, K. and
                      Yamashita, Y. and Yasutake, M. and Uesugi, K. and Umegaki,
                      I. and Chiu, I. and Ishizaki, T. and Okumura, S. and
                      Palomba, E. and Pilorget, C. and Potin, S. M. and Alasli, A.
                      and Anada, S. and Araki, Y. and Sakatani, N. and Schultz, C.
                      and Sekizawa, O. and Sitzman, S. D. and Sugiura, K. and Sun,
                      M. and Dartois, E. and De Pauw, E. and Dionnet, Z. and
                      Djouadi, Z. and Falkenberg, Gerald and Fujita, R. and
                      Fukuma, T. and Gearba, I. R. and Hagiya, K. and Hu, M. Y.
                      and Kato, T. and Kawamura, T. and Kimura, M. and Kubo, M. K.
                      and Langenhorst, F. and Lantz, C. and Lavina, B. and
                      Lindner, M. and Zhao, J. and Vekemans, B. and Baklouti, D.
                      and Bazi, B. and Borondics, F. and Nagasawa, S. and
                      Nishiyama, G. and Nitta, K. and Mathurin, J. and Matsumoto,
                      T. and Mitsukawa, I. and Miura, H. and Miyake, A. and
                      Miyake, Y. and Yurimoto, H. and Okazaki, R. and Yabuta, H.
                      and Naraoka, H. and Sakamoto, K. and Tachibana, S. and
                      Connolly, H. C. and Lauretta, D. S. and Yoshitake, M. and
                      Yoshikawa, M. and Yoshikawa, K. and Yoshihara, K. and
                      Yokota, Y. and Yogata, K. and Yano, H. and Yamamoto, Y. and
                      Yamamoto, D. and Yamada, M. and Yamada, T. and Yada, T. and
                      Wada, K. and Usui, T. and Tsukizaki, R. and Terui, F. and
                      Takeuchi, H. and Takei, Y. and Iwamae, A. and Soejima, H.
                      and Shirai, K. and Shimaki, Y. and Senshu, H. and Sawada, H.
                      and Saiki, T. and Ozaki, M. and Ono, G. and Okada, T. and
                      Ogawa, N. and Ogawa, K. and Noguchi, R. and Noda, H. and
                      Nishimura, M. and Namiki, N. and Nakazawa, S. and Morota, T.
                      and Miyazaki, A. and Miura, A. and Mimasu, Y. and Matsumoto,
                      K. and Kumagai, K. and Kouyama, T. and Kikuchi, S. and
                      Kawahara, K. and Kameda, S. and Iwata, T. and Ishihara, Y.
                      and Ishiguro, M. and Ikeda, H. and Hosoda, S. and Honda, R.
                      and Honda, C. and Hitomi, Y. and Hirata, N. and Hirata, N.
                      and Hayashi, T. and Hayakawa, M. and Hatakeda, K. and
                      Furuya, S. and Fukai, R. and Fujii, A. and Cho, Y. and
                      Arakawa, M. and Abe, M. and Watanabe, S. and Tsuda, Y.},
      title        = {{F}ormation and evolution of carbonaceous asteroid {R}yugu:
                      {D}irect evidence from returned samples},
      journal      = {Science / Science now},
      volume       = {379},
      number       = {6634},
      issn         = {0036-8075},
      address      = {Washington, DC},
      publisher    = {Assoc.},
      reportid     = {PUBDB-2022-06897},
      pages        = {787},
      year         = {2023},
      note         = {Volltext angefordert, online first},
      abstract     = {Samples of the carbonaceous asteroid Ryugu were brought to
                      Earth by the Hayabusa2 spacecraft. We analyzed seventeen
                      Ryugu samples measuring 1-8 mm. CO$_2$-bearing water
                      inclusions are present within a pyrrhotite crystal,
                      indicating that Ryugu’s parent asteroid formed in the
                      outer Solar System. The samples contain low abundances of
                      materials that formed at high temperatures, such as
                      chondrules and Ca, Al-rich inclusions. The samples are rich
                      in phyllosilicates and carbonates, which formed by aqueous
                      alteration reactions at low temperature, high pH, and
                      water/rock ratios < 1 (by mass). Less altered fragments
                      contain olivine, pyroxene, amorphous silicates, calcite, and
                      phosphide. Numerical simulations, based on the mineralogical
                      and physical properties of the samples, indicate Ryugu’s
                      parent body formed ~ 2 million years after the beginning of
                      Solar System formation.},
      cin          = {DOOR ; HAS-User / FS-PETRA-S},
      ddc          = {320},
      cid          = {I:(DE-H253)HAS-User-20120731 /
                      I:(DE-H253)FS-PETRA-S-20210408},
      pnm          = {631 - Matter – Dynamics, Mechanisms and Control
                      (POF4-631) / 6G3 - PETRA III (DESY) (POF4-6G3) /
                      FS-Proposal: II-20210018 EC (II-20210018-EC)},
      pid          = {G:(DE-HGF)POF4-631 / G:(DE-HGF)POF4-6G3 /
                      G:(DE-H253)II-20210018-EC},
      experiment   = {EXP:(DE-H253)P-P06-20150101},
      typ          = {PUB:(DE-HGF)16},
      pubmed       = {pmid:36137011},
      UT           = {WOS:000981670800002},
      doi          = {10.1126/science.abn8671},
      url          = {https://bib-pubdb1.desy.de/record/485848},
}