Ryugu’s Anhydrous Ingredients and Their Spectral Link to Primitive Dust from the Outer Solar System

Autor: R. Brunetto, C. Lantz, Y. Fukuda, A. Aléon-Toppani, T. Nakamura, Z. Dionnet, D. Baklouti, F. Borondics, Z. Djouadi, S. Rubino, K. Amano, M. Matsumoto, Y. Fujioka, T. Morita, M. Kukuiri, E. Kagawa, M. Matsuoka, R. Milliken, H. Yurimoto, T. Noguchi, R. Okazaki, H. Yabuta, H. Naraoka, K. Sakamoto, S. Tachibana, T. Yada, M. Nishimura, A. Nakato, A. Miyazaki, K. Yogata, M. Abe, T. Okada, T. Usui, M. Yoshikawa, T. Saiki, S. Tanaka, F. Terui, S. Nakazawa, S. Watanabe, Y. Tsuda

Publikováno v: The Astrophysical Journal Letters, Vol 951, Iss 2, p L33 (2023)

Ryugu is a second-generation C-type asteroid formed by the reassembly of fragments of a previous larger body in the main asteroid belt. While the majority of Ryugu samples returned by Hayabusa2 are composed of a lithology dominated by aqueously alter

Externí odkaz: https://doaj.org/article/6dc532b03acd451ca587e40d3c2fa00e

The noble gas and nitrogen relationship between Ryugu and carbonaceous chondrites

Autor: M.W. Broadley, D.J. Byrne, E. Füri, L. Zimmermann, B. Marty, R. Okazaki, T. Yada, F. Kitajima, S. Tachibana, K. Yogata, K. Sakamoto, H. Yurimoto, T. Nakamura, T. Noguchi, H. Naraoka, H. Yabuta, S. Watanabe, Y. Tsuda, M. Nishimura, A. Nakato, A. Miyazaki, M. Abe, T. Okada, T. Usui, M. Yoshikawa, T. Saiki, S. Tanaka, F. Terui, S. Nakazawa, H. Busemann, K. Hashizume, J.D. Gilmour, A. Meshik, M.E.I. Riebe, D. Krietsch, C. Maden, A. Ishida, P. Clay, S.A. Crowther, L. Fawcett, T. Lawton, O. Pravdivtseva, Y.N. Miura, J. Park, K. Bajo, Y. Takano, K. Yamada, S. Kawagucci, Y. Matsui, M. Yamamoto, K. Righter, S. Sakai, N. Iwata, N. Shirai, S. Sekimoto, M. Inagaki, M. Ebihara, R. Yokochi, K. Nishiizumi, K. Nagao, J.I Lee, A. Kano, M.W. Caffee, R. Uemura

Publikováno v: Broadley, M W, Byrne, D J, Füri, E, Zimmermann, L, Marty, B, Okazaki, R, Yada, T, Kitajima, F, Tachibana, S, Yogata, K, Sakamoto, K, Yurimoto, H, Nakamura, T, Noguchi, T, Naraoka, H, Yabuta, H, Watanabe, S, Tsuda, Y, Nishimura, M, Nakato, A, Miyazaki, A, Abe, M, Okada, T, Usui, T, Yoshikawa, M, Saiki, T, Tanaka, S, Terui, F, Nakazawa, S, Busemann, H, Hashizume, K, Gilmour, J D, Meshik, A, Riebe, M E I, Krietsch, D, Maden, C, Ishida, A, Clay, P, Crowther, S A, Fawcett, L, Lawton, T, Pravdivtseva, O, Miura, Y N, Park, J, Bajo, K, Takano, Y, Yamada, K, Kawagucci, S, Matsui, Y, Yamamoto, M, Righter, K, Sakai, S, Iwata, N, Shirai, N, Sekimoto, S, Inagaki, M, Ebihara, M, Yokochi, R, Nishiizumi, K, Nagao, K, Lee, J I, Kano, A, Caffee, M W & Uemura, R 2023, ' The noble gas and nitrogen relationship between Ryugu and carbonaceous chondrites ', Geochimica Et Cosmochimica Acta, vol. 345, pp. 62-74 . https://doi.org/10.1016/j.gca.2023.01.020
Geochimica et Cosmochimica Acta, 345

Carbonaceous chondrites are considered to have originated from C-type asteroids and represent some of the most primitive material in our solar system. Furthermore, since carbonaceous chondrites can contain significant quantities of volatile elements,

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::56494cb62819ddd0a2f01a6b76a2c921
https://doi.org/10.1016/j.gca.2023.01.020

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