Article in Science advances, 2023. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.
0numbers the graph read from it
0cells of the map it votes in
2citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it
What it found
Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.
The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.
2 · The registry
The trial behind it
Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.
Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.
PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.
5 · Who and what money
Authors and funding
49 authors.
Kana AmanoDepartment of Earth Science, Tohoku University, Sendai 980-8578, Japan.ORCID 0000-0003-4466-4426
Moe MatsuokaGeological Survey of Japan, National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8567, Japan.ORCID 0000-0003-1091-3041
Sandra M PotinFaculty of Aerospace Engineering, Delft University of Technology, 2629 HS Delft, Netherlands.ORCID 0000-0001-6907-3409
Takahiro HiroiDepartment of Earth, Environmental, and Planetary Sciences, Brown University, Providence, RI 02912, USA.ORCID 0000-0003-2866-9091
Eri TatsumiInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0002-6142-9842
Ralph E MillikenDepartment of Earth, Environmental, and Planetary Sciences, Brown University, Providence, RI 02912, USA.ORCID 0000-0003-3240-4918
Eric QuiricoInstitut de Planétologie et d'Astrophysique de Grenoble (IPAG), CNRS, Université Grenoble Alpes, Grenoble 38000, France.ORCID 0000-0003-2768-0694
Pierre BeckInstitut de Planétologie et d'Astrophysique de Grenoble (IPAG), CNRS, Université Grenoble Alpes, Grenoble 38000, France.ORCID 0000-0002-6532-5602
Hisayoshi YurimotoDepartment of Earth and Planetary Sciences, Hokkaido University, Sapporo 060-0810, Japan.ORCID 0000-0003-0702-0533
Takaaki NoguchiDivision of Earth and Planetary Sciences, Kyoto University, Kyoto 606-8502, Japan.ORCID 0000-0001-7211-2595
Ryuji OkazakiDepartment of Earth and Planetary Sciences, Kyushu University, Fukuoka 819-0395, Japan.ORCID 0000-0003-0177-7527
Hikaru YabutaDepartment of Earth and Planetary Systems Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan.ORCID 0000-0002-4625-5362
Hiroshi NaraokaDepartment of Earth and Planetary Sciences, Kyushu University, Fukuoka 819-0395, Japan.ORCID 0000-0002-2373-8759
Kanako SakamotoInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0001-5138-5324
Shogo TachibanaDepartment of Earth and Planetary Science, The University of Tokyo, Tokyo 113-0033, Japan.ORCID 0000-0002-4603-9440
Toru YadaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0002-7971-510X
Masahiro NishimuraInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0003-3143-8171
Aiko NakatoInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0003-2392-1497
Akiko MiyazakiInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0001-7427-2285
Kasumi YogataInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0002-3717-9185
Masanao AbeInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0003-4780-800X
Tatsuaki OkadaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0001-6381-8107
Tomohiro UsuiInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0002-4653-293X
Makoto YoshikawaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0002-3118-7475
Takanao SaikiInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0003-3100-420X
Satoshi TanakaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0002-4874-0417
Fuyuto TeruiDepartment of Mechanical Engineering, Kanagawa Institute of Technology, Atsugi 243-0292, Japan.ORCID 0000-0001-6422-0983
Satoru NakazawaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0003-4250-1826
Sei-Ichiro WatanabeDepartment of Earth and Environmental Sciences, Nagoya University, Nagoya 464-8601, Japan.ORCID 0000-0002-5820-2102
Yuichi TsudaInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.ORCID 0000-0002-9161-6171
Funding
No grant is acknowledged in the PubMed record.
6 · The paper itself
Abstract
The carbonaceous asteroid Ryugu has been explored by the Hayabusa2 spacecraft to elucidate the actual nature of hydrous asteroids. Laboratory analyses revealed that the samples from Ryugu are comparable to unheated CI carbonaceous chondrites; however, reflectance spectra of Ryugu samples and CIs do not coincide. Here, we demonstrate that Ryugu sample spectra are reproduced by heating Orgueil CI chondrite at 300°C under reducing conditions, which caused dehydration of terrestrial weathering products and reduction of iron in phyllosilicates. Terrestrial weathering of CIs accounts for the spectral differences between Ryugu sample and CIs, which is more severe than space weathering that likely explains those between asteroid Ryugu and the collected samples. Previous assignments of CI chondrite parent bodies, i.e., chemically most primitive objects in the solar system, are based on the spectra of CI chondrites. This study indicates that actual spectra of CI parent bodies are much darker and flatter at ultraviolet to visible wavelengths than the spectra of CI chondrites.
Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.
Reassigning CI chondrite parent bodies based on reflectance spectroscopy of samples from carbonaceous asteroid Ryugu and meteorites. · full record | OpenQuestion