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Formation and evolution of carbonaceous asteroid Ryugu: Direct evidence from returned samples
Science ( IF 56.9 ) Pub Date : 2022-09-22 , DOI: 10.1126/science.abn8671
T Nakamura 1 , M Matsumoto 1 , K Amano 1 , Y Enokido 1 , M E Zolensky 2 , T Mikouchi 3 , H Genda 4 , S Tanaka 5, 6 , M Y Zolotov 7 , K Kurosawa 8 , S Wakita 9 , R Hyodo 5 , H Nagano 10 , D Nakashima 1 , Y Takahashi 11, 12 , Y Fujioka 1 , M Kikuiri 1 , E Kagawa 1 , M Matsuoka 13, 14 , A J Brearley 15 , A Tsuchiyama 16, 17, 18 , M Uesugi 19 , J Matsuno 16 , Y Kimura 20 , M Sato 11 , R E Milliken 21 , E Tatsumi 11, 22 , S Sugita 8, 11 , T Hiroi 21 , K Kitazato 23 , D Brownlee 24 , D J Joswiak 24 , M Takahashi 1 , K Ninomiya 25 , T Takahashi 26, 27 , T Osawa 28 , K Terada 29 , F E Brenker 30 , B J Tkalcec 30 , L Vincze 31 , R Brunetto 32 , A Aléon-Toppani 32 , Q H S Chan 33 , M Roskosz 34 , J-C Viennet 34 , P Beck 35 , E E Alp 36 , T Michikami 37 , Y Nagaashi 1, 38 , T Tsuji 39, 40 , Y Ino 5, 41 , J Martinez 2 , J Han 42 , A Dolocan 43 , R J Bodnar 44 , M Tanaka 45 , H Yoshida 11 , K Sugiyama 46 , A J King 47 , K Fukushi 48 , H Suga 49 , S Yamashita 50, 51 , T Kawai 11 , K Inoue 48 , A Nakato 5 , T Noguchi 52, 53 , F Vilas 54 , A R Hendrix 54 , C Jaramillo-Correa 55 , D L Domingue 54 , G Dominguez 56 , Z Gainsforth 57 , C Engrand 58 , J Duprat 34 , S S Russell 47 , E Bonato 59 , C Ma 60 , T Kawamoto 61 , T Wada 1 , S Watanabe 5, 26 , R Endo 62 , S Enju 63 , L Riu 64 , S Rubino 32 , P Tack 31 , S Takeshita 65 , Y Takeichi 50, 51, 66 , A Takeuchi 19 , A Takigawa 11 , D Takir 2 , T Tanigaki 67 , A Taniguchi 68 , K Tsukamoto 1 , T Yagi 69 , S Yamada 70 , K Yamamoto 71 , Y Yamashita 69 , M Yasutake 19 , K Uesugi 19 , I Umegaki 65, 72 , I Chiu 25 , T Ishizaki 5 , S Okumura 52 , E Palomba 73 , C Pilorget 32, 74 , S M Potin 13, 75 , A Alasli 10 , S Anada 71 , Y Araki 76 , N Sakatani 5, 70 , C Schultz 21 , O Sekizawa 49 , S D Sitzman 77 , K Sugiura 4 , M Sun 17, 18, 78 , E Dartois 79 , E De Pauw 31 , Z Dionnet 32 , Z Djouadi 32 , G Falkenberg 80 , R Fujita 10 , T Fukuma 81 , I R Gearba 43 , K Hagiya 82 , M Y Hu 36 , T Kato 71 , T Kawamura 83 , M Kimura 50, 51 , M K Kubo 84 , F Langenhorst 85 , C Lantz 32 , B Lavina 86 , M Lindner 30 , J Zhao 36 , B Vekemans 31 , D Baklouti 32 , B Bazi 31 , F Borondics 87 , S Nagasawa 26, 27 , G Nishiyama 11 , K Nitta 49 , J Mathurin 88 , T Matsumoto 52 , I Mitsukawa 52 , H Miura 89 , A Miyake 52 , Y Miyake 65 , H Yurimoto 90 , R Okazaki 91 , H Yabuta 92 , H Naraoka 91 , K Sakamoto 5 , S Tachibana 5, 11 , H C Connolly 93 , D S Lauretta 94 , M Yoshitake 5 , M Yoshikawa 5, 6 , K Yoshikawa 95 , K Yoshihara 5 , Y Yokota 5 , K Yogata 5 , H Yano 5, 6 , Y Yamamoto 5, 6 , D Yamamoto 5 , M Yamada 8 , T Yamada 5 , T Yada 5 , K Wada 8 , T Usui 5, 11 , R Tsukizaki 5 , F Terui 96 , H Takeuchi 5, 6 , Y Takei 5 , A Iwamae 97 , H Soejima 5, 97 , K Shirai 5 , Y Shimaki 5 , H Senshu 8 , H Sawada 5 , T Saiki 5 , M Ozaki 5, 6 , G Ono 95 , T Okada 5, 98 , N Ogawa 5 , K Ogawa 5 , R Noguchi 99 , H Noda 100 , M Nishimura 5 , N Namiki 6, 100 , S Nakazawa 5 , T Morota 11 , A Miyazaki 5 , A Miura 5 , Y Mimasu 5 , K Matsumoto 6, 100 , K Kumagai 5, 97 , T Kouyama 101 , S Kikuchi 8, 100 , K Kawahara 5 , S Kameda 5, 70 , T Iwata 5, 6 , Y Ishihara 102 , M Ishiguro 103 , H Ikeda 95 , S Hosoda 5 , R Honda 104, 105 , C Honda 23 , Y Hitomi 5, 97 , N Hirata 38 , N Hirata 23 , T Hayashi 5 , M Hayakawa 5 , K Hatakeda 5, 97 , S Furuya 11 , R Fukai 5 , A Fujii 5 , Y Cho 11 , M Arakawa 38 , M Abe 5, 6 , S Watanabe 106 , Y Tsuda 5
Affiliation  

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.

中文翻译:

碳质小行星 Ryugu 的形成和演化:来自返回样本的直接证据

隼鸟 2 号宇宙飞船将碳质小行星 Ryugu 的样本带到了地球。我们分析了 17 个尺寸为 1-8 毫米的 Ryugu 样品。一氧化碳2个含水包裹体存在于磁黄铁矿晶体内,表明龙宫的母体小行星形成于外太阳系。这些样品含有在高温下形成的低丰度材料,例如陨石球粒和富含钙、铝的包裹体。样品富含页硅酸盐和碳酸盐,它们是在低温、高 pH 值和水/岩石比 < 1(按质量计)下通过水蚀变反应形成的。变化较小的碎片包含橄榄石、辉石、无定形硅酸盐、方解石和磷化物。基于样品的矿物学和物理特性的数值模拟表明,龙宫的母体形成于太阳系形成开始后约 200 万年。
更新日期:2022-09-22
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