Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/30832
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Kitazato, K. | en_US |
dc.contributor.author | Milliken, R. E. | en_US |
dc.contributor.author | Iwata, T. | en_US |
dc.contributor.author | Abe, M. | en_US |
dc.contributor.author | Ohtake, M. | en_US |
dc.contributor.author | Matsuura, S. | en_US |
dc.contributor.author | Arai, T. | en_US |
dc.contributor.author | Nakauchi, Y. | en_US |
dc.contributor.author | Nakamura, T. | en_US |
dc.contributor.author | Matsuoka, M. | en_US |
dc.contributor.author | Senshu, H. | en_US |
dc.contributor.author | Hirata, N. | en_US |
dc.contributor.author | Hiroi, T. | en_US |
dc.contributor.author | Pilorget, C. | en_US |
dc.contributor.author | Brunetto, R. | en_US |
dc.contributor.author | Poulet, F. | en_US |
dc.contributor.author | Riu, L. | en_US |
dc.contributor.author | Bibring, J. -P. | en_US |
dc.contributor.author | Takir, D. | en_US |
dc.contributor.author | Domingue, D. L. | en_US |
dc.contributor.author | Vilas, F. | en_US |
dc.contributor.author | Barucci, M. A. | en_US |
dc.contributor.author | PERNA, Davide | en_US |
dc.contributor.author | PALOMBA, Ernesto | en_US |
dc.contributor.author | GALIANO, ANNA | en_US |
dc.contributor.author | Tsumura, K. | en_US |
dc.contributor.author | Osawa, T. | en_US |
dc.contributor.author | Komatsu, M. | en_US |
dc.contributor.author | Nakato, A. | en_US |
dc.contributor.author | Takato, N. | en_US |
dc.contributor.author | Matsunaga, T. | en_US |
dc.contributor.author | Takagi, Y. | en_US |
dc.contributor.author | Matsumoto, K. | en_US |
dc.contributor.author | Kouyama, T. | en_US |
dc.contributor.author | Yokota, Y. | en_US |
dc.contributor.author | Tatsumi, E. | en_US |
dc.contributor.author | Sakatani, N. | en_US |
dc.contributor.author | Yamamoto, Y. | en_US |
dc.contributor.author | Okada, T. | en_US |
dc.contributor.author | Sugita, S. | en_US |
dc.contributor.author | Honda, R. | en_US |
dc.contributor.author | Morota, T. | en_US |
dc.contributor.author | Kameda, S. | en_US |
dc.contributor.author | Sawada, H. | en_US |
dc.contributor.author | Honda, C. | en_US |
dc.contributor.author | Yamada, M. | en_US |
dc.contributor.author | Suzuki, H. | en_US |
dc.contributor.author | Yoshioka, K. | en_US |
dc.contributor.author | Hayakawa, M. | en_US |
dc.contributor.author | Ogawa, K. | en_US |
dc.contributor.author | Cho, Y. | en_US |
dc.contributor.author | Shirai, K. | en_US |
dc.contributor.author | Shimaki, Y. | en_US |
dc.contributor.author | Yamaguchi, A. | en_US |
dc.contributor.author | Ogawa, N. | en_US |
dc.contributor.author | Terui, F. | en_US |
dc.contributor.author | Yamaguchi, T. | en_US |
dc.contributor.author | Takei, Y. | en_US |
dc.contributor.author | Saiki, T. | en_US |
dc.contributor.author | Nakazawa, S. | en_US |
dc.contributor.author | Tanaka, S. | en_US |
dc.contributor.author | Yoshikawa, M. | en_US |
dc.contributor.author | Watanabe, S. | en_US |
dc.contributor.author | Tsuda, Y. | en_US |
dc.date.accessioned | 2021-04-21T14:13:19Z | - |
dc.date.available | 2021-04-21T14:13:19Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0036-8075 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30832 | - |
dc.description.abstract | The near-Earth asteroid 162173 Ryugu, the target of the Hayabusa2 sample-return mission, is thought to be a primitive carbonaceous object. We report reflectance spectra of Ryugu’s surface acquired with the Near-Infrared Spectrometer (NIRS3) on Hayabusa2, to provide direct measurements of the surface composition and geological context for the returned samples. A weak, narrow absorption feature centered at 2.72 micrometers was detected across the entire observed surface, indicating that hydroxyl (OH)-bearing minerals are ubiquitous there. The intensity of the OH feature and low albedo are similar to thermally and/or shock-metamorphosed carbonaceous chondrite meteorites. There are few variations in the OH-band position, which is consistent with Ryugu being a compositionally homogeneous rubble-pile object generated from impact fragments of an undifferentiated aqueously altered parent body. | en_US |
dc.language.iso | eng | en_US |
dc.title | The surface composition of asteroid 162173 Ryugu from Hayabusa2 near-infrared spectroscopy | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1126/science.aav7432 | en_US |
dc.identifier.scopus | 2-s2.0-85064039118 | en_US |
dc.identifier.url | https://science.sciencemag.org/content/364/6437/272 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 364 | en_US |
dc.relation.issue | 6437 | en_US |
dc.relation.firstpage | 272 | en_US |
dc.relation.lastpage | 275 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | SCIENCE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019Sci...364..272K | en_US |
dc.relation.fund | H2020 | en_US |
dc.relation.project | AstroFIt2 (Astronomy Fellowships in Italy 2) | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | mixedopen | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0002-4545-3850 | - |
crisitem.author.orcid | 0000-0002-9101-6774 | - |
crisitem.author.orcid | 0000-0001-8740-0653 | - |
crisitem.project.grantno | 664931 | - |
crisitem.journal.journalissn | 0036-8075 | - |
crisitem.journal.ance | E151981 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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Kitazato_Science_2019.pdf | [Administrators only] | 849.23 kB | Adobe PDF | |
Kitazato_Science_2019_Preprint.pdf | preprint | 7.33 MB | Adobe PDF | Visualizza/apri |
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