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Oxygen Isotopic Compositions of Asteroidal Materials returned from Itokawa by the Hayabusa Mission

Yurimoto, Hisayoshi; Abe, Ken-ichi; Abe, Masanao; Ebihara, Mitsuru; Fujimura, Akio; Hashiguchi, Minako; Hashizume, K; Ireland, Trevor; Itoh, Shoichi; Katayama, Juri; Kato, Chizu; Kawaguchi, Junichiro; Kawasaki, Noriyuki; Kitajima, Fumio; Kobayashi, Sachio; Meike, Tatsuji; Mukai, Toshifumi; Nagao, Keisuke; Nakamura, Tomoki; Naraoka, Hiroshi; Noguchi, Takaaki; Okazaki, Ryuji; Park, Changkun; Sakamoto, Naoya; Seto, Yusuke; Takei, Masashi; Tsuchiyama, Akira; Uesugi, Masayuki; Wakaki, Shigeyuki; Yada, Toru; Yamamoto, Kosuke; Yoshikawa, Makoto; Zolensky, Michael

Description

Meteorite studies suggest that each solar system object has a unique oxygen isotopic composition. Chondrites, the most primitive of meteorites, have been believed to be derived from asteroids, but oxygen isotopic compositions of asteroids themselves have

CollectionsANU Research Publications
Date published: 2011
Type: Journal article
URI: http://hdl.handle.net/1885/29177
Source: Science
DOI: 10.1126/science.1207776

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