A micro-Raman and infrared study of several Hayabusa category 3 (organic) particles
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DOI[10.1186/s40623-015-0182-6]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Fumio KitajimaMasayuki UesugiYuzuru Karouji
- Publication, Distribution, etc.
- Publication Date
- 2015-02-11
- Publication Date (W3CDTF)
- 2015-02-11
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 67(20)
- Volume
- 67(20)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-015-0182-6
- Persistent ID (NDL)
- info:ndljp/pid/9381150
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2015-06-08T22:01:55+09:00
- Date Captured (W3CDTF)
- 2015-04-20
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/9227920
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- Three category 3 (organic) particles (RB-QD04-0001, RB-QD04-0047-02, and RA-QD02-0120) and so-called ‘white object’ found in the sample container have been examined by micro-Raman and infrared (IR) spectroscopy. In addition, several artificial substances that could occur as possible contaminants and chondritic insoluble organic matter (IOM) prepared from the Murchison CM2 chondrite were analyzed. The Raman spectra of the particles show broad G-band and weak D-band. The G-band parameters plot in the disordered region and close to the artifact produced from a Viton glove after laser exposure rather than chondritic IOM. The particles were therefore originally at low maturity level, suggesting that they have not experienced strong heating and are therefore not related to the LL4-6 parent body. The IR spectra are not similar to that of chondritic IOM. Furthermore, the particles cannot be identified as some artificial carbonaceous substances, including the white object, which are the possible contaminants, examined in this investigation. Although it cannot be determined exactly whether the three category 3 particles are extraterrestrial, the limited IR and Raman results in this investigation strongly suggest their terrestrial origin. Although they could not be directly related to the artificial contaminants examined in this investigation, they may yet be reaction products from similar substances that flew on the mission. In particular, RB-QD04-0047-02 shows several infrared spectral absorption bands in common with the ‘white object.’ This may relate to the degradation of a polyimide/polyamide resin.
- DOI
- 10.1186/s40623-015-0182-6
- Access Restrictions
- インターネット公開
- Rights (production)
- Creative Commons Attribution 4.0 International© 2015 Kitajima et al.
- Related Material
- A Micro-Raman and Infrared Study of Several Hayabusa Category 3 (organic) Particles
- Related Material (URI)
- Is Referenced By
- Further characterization of carbonaceous materials in Hayabusa‐returned samples to understand their originAstrophysical Sites that Can Produce Enantiomeric Amino AcidsHayabusa2 Sample Catcher and Container: Metal-Seal System for Vacuum Encapsulation of Returned Samples with Volatiles and Organic Compounds Recovered from C-Type Asteroid RyuguThe Importance of Phobos Sample Return for Understanding the Mars-Moon SystemConcerns of Organic Contamination for Sample Return Space MissionsOrganic matter and water from asteroid ItokawaInfrared absorption spectra from organic matter in the asteroid Ryugu samples: Some unique properties compared to unheated carbonaceous chondritesChemical assessment of the explosive chamber in the projector system of Hayabusa2 for asteroid samplingAnalytical protocols for Phobos regolith samples returned by the Martian Moons eXploration (MMX) missionThe Earth, Planets and Space special issue : "Science of solar system materials examined from Hayabusa and future missions"Amino acid compositions in heated carbonaceous chondrites and their compound-specific nitrogen isotopic ratiosEnvironmental assessment in the prelaunch phase of Hayabusa2 for safety declaration of returned samples from the asteroid (162173) Ryugu : background monitoring and risk management during development of the sampler system
- References
- H, C, and N isotopic compositions of Hayabusa category 3 organic samplesSequential analysis of carbonaceous materials in Hayabusa-returned samples for the determination of their originOxygen Isotopic Compositions of Asteroidal Materials Returned from Itokawa by the Hayabusa MissionIncipient Space Weathering Observed on the Surface of Itokawa Dust ParticlesIrradiation History of Itokawa Regolith Material Deduced from Noble Gases in the Hayabusa SamplesCharacterization of insoluble organic matter in primitive meteorites by microRaman spectroscopyHayabusa‐returned sample curation in the Planetary Material Sample Curation Facility of JAXAThree-Dimensional Structure of Hayabusa Samples: Origin and Evolution of Itokawa RegolithNeutron Activation Analysis of a Particle Returned from Asteroid ItokawaCarbon isotopic composition of acetic acid generated by hydrous pyrolysis of macromolecular organic matter from the Murchison meteoriteItokawa Dust Particles: A Direct Link Between S-Type Asteroids and Ordinary ChondritesCompositional diversity in insoluble organic matter in type 1, 2 and 3 chondrites as detected by infrared spectroscopyCarbon in the matrices of ordinary chondritesIdentification of molecular-cloud material in interplanetary dust particlesDeveloping space weathering on the asteroid 25143 ItokawaOrganics Captured from Comet 81P/Wild 2 by the Stardust SpacecraftPrecursor and metamorphic condition effects on Raman spectra of poorly ordered carbonaceous matter in chondrites and coalsOrganic thermometry for chondritic parent bodiesPreliminary organic compound analysis of microparticles returned from Asteroid 25143 Itokawa by the Hayabusa missionX-ray absorption near edge structure spectroscopic study of Hayabusa category 3 carbonaceous particles
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 学術機関リポジトリデータベース学術機関リポジトリデータベース雑誌記事索引データベースCrossrefCiNii Articles科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース学術機関リポジトリデータベースCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- Bibliographic ID (NDL)
- 9381150
- NAID
- 120006800833