Asteroid Ryugu before the Hayabusa2 encounter
国立国会図書館館内限定公開
収録元データベースで確認する
国立国会図書館デジタルコレクション
デジタルデータあり
公開元のウェブサイトで確認する
DOI[10.1186/s40645-018-0237-y]のデータに遷移します
全国の図書館の所蔵
国立国会図書館以外の全国の図書館の所蔵状況を表示します。
所蔵のある図書館から取寄せることが可能かなど、資料の利用方法は、ご自身が利用されるお近くの図書館へご相談ください
書誌情報
この資料の詳細や典拠（同じ主題の資料を指すキーワード、著者名）等を確認できます。
- 資料種別
- 記事
- 著者・編者
- Koji WadaMatthias GrottPatrick Michel
- 出版年月日等
- 2018-12-11
- 出版年（W3CDTF）
- 2018-12-11
- タイトル（掲載誌）
- Progress in earth and planetary science
- 巻号年月日等（掲載誌）
- 5(82)
- 掲載巻
- 5(82)
- ISSN（掲載誌）
- 2197-4284
- ISSN-L（掲載誌）
- 2197-4284
- 本文の言語コード
- eng
- DOI
- 10.1186/s40645-018-0237-y
- 国立国会図書館永続的識別子
- info:ndljp/pid/11249480
- コレクション（共通）
- コレクション（障害者向け資料：レベル1）
- コレクション（個別）
- 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
- 収集根拠
- オンライン資料収集制度
- 受理日（W3CDTF）
- 2019-03-05T23:10:26+09:00
- 保存日（W3CDTF）
- 2019-03-05
- 記録形式（IMT）
- application/pdf
- オンライン閲覧公開範囲
- 国立国会図書館内限定公開
- デジタル化資料送信
- 図書館・個人送信対象外
- 遠隔複写可否（NDL）
- 可
- 掲載誌（国立国会図書館永続的識別子）
- info:ndljp/pid/11018906
- 連携機関・データベース
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- 要約等
- I tried that how did musicians act in Osaka-kabuki during the Edo period. Concretely it clarifies relation between actors and musicians. I tried clarifying that by the social network analysis. It is a Result, to the first, the existence is clarified between actors and musicians,to the second, It agrees between the actor grope and the musician group. And to the third, it is some differs in Nagauta music and Gidayu music.
- 関連情報（URI）
- 連携機関・データベース
- 国立情報学研究所 : CiNii Research
- 提供元機関・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CiNii Articles
- 書誌ID（NDLBibID）
- 11249480
- NII論文ID
- 110008428229
- 要約等
- Asteroid (162173) Ryugu is the target object of Hayabusa2, an asteroid exploration and sample return mission led by Japan Aerospace Exploration Agency (JAXA). Ground-based observations indicate that Ryugu is a C-type near-Earth asteroid with a diameter of less than 1km, but the knowledge of its detailed properties is very limited prior to Hayabusa2 observation. This paper summarizes our best understanding of the physical and dynamical properties of Ryugu based on ground-based remote sensing and theoretical modeling before the Hayabusa2's arrival at the asteroid. This information is used to construct a design reference model of the asteroid that is used for the formulation of mission operation plans in advance of asteroid arrival. Particular attention is given to the surface properties of Ryugu that are relevant to sample acquisition. This reference model helps readers to appropriately interpret the data that will be directly obtained by Hayabusa2 and promotes scientific studies not only for Ryugu itself and other small bodies but also for the solar system evolution that small bodies shed light on.
- DOI
- 10.1186/s40645-018-0237-y10.7892/boris.12270610.48550/arxiv.1804.03734
- オンライン閲覧公開範囲
- インターネット公開
- 著作権情報
- © The Author(s). 2018.This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
- 関連情報（URI）
- 参照
- Effects of dust layers on thermal emission from airless bodiesLaboratory experiments on agglomeration of particles in a granular streamThermophysical properties of the surface of asteroid 162173 Ryugu: Infrared observations and thermal inertia mappingSimulation of Seismic Wave Propagation on Asteroid Ryugu Induced by The Impact Experiment of The Hayabusa2 Mission: Limited Mass Transport by Low Yield Strength of Porous RegolithResurfacing processes constrained by crater distribution on RyuguMid-infrared emissivity of partially dehydrated asteroid (162173) Ryugu shows strong signs of aqueous alterationAnalysis of Cation Composition in Dolomites on the Intact Particles Sampled from Asteroid RyuguSpace weathering acts strongly on the uppermost surface of RyuguThe asteroid 162173 Ryugu: a cometary originHayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top–shaped rubble pileA generalised methodology for analytic construction of 1:1 resonances around irregular bodies: Application to the asteroid Ryugu’s ejecta dynamicsNumerical modelling of medium-speed impacts on a granular surface in a low-gravity environment application to Hayabusa2 sampling mechanismSpectral and Petrographic Properties of Inclusions in Carbonaceous Chondrites and Comparison with In Situ Images from Asteroid RyuguSimplified Simulated Materials of Asteroid Ryugu for Spacecraft Operations and Scientific EvaluationsResurfacing processes on asteroid (162173) Ryugu caused by an artificial impact of Hayabusa2's Small Carry-on ImpactorNumerical modeling of lander interaction with a low-gravity asteroid regolith surfaceLow thermal conductivity boulder with high porosity identified on C-type asteroid (162173) RyuguAnomalously porous boulders on (162173) Ryugu as primordial materials from its parent bodyThermally altered subsurface material of asteroid (162173) RyuguAligned fractures on asteroid Ryugu as an indicator of thermal fracturingOrigin of Phobos and Deimos Awaiting Direct ExplorationAn artificial impact on the asteroid (162173) Ryugu formed a crater in the gravity-dominated regimeThermophysical Properties of C-Type Asteroid 162173 Ryugu Revealed by the Thermal Infrared Imager TIR on Hayabusa2
- 参照
- Three‐dimensional microstructure of samples recovered from asteroid 25143 Itokawa: Comparison with LL5 and LL6 chondrite particlesFragment shapes in impact experiments ranging from cratering to catastrophic disruptionExperimental study on compression property of regolith analoguesHayabusa2 Mission OverviewPetrographic, chemical and spectroscopic evidence for thermal metamorphism in carbonaceous chondrites I: CI and CM chondritesCompressional stress effect on thermal conductivity of powdered materials: Measurements and their implication to lunar regolithNIRS3: The Near Infrared Spectrometer on Hayabusa2Relationship between regolith particle size and porosity on small bodiesThermal conductivity of lunar regolith simulant JSC-1A under vacuumIn search of the source of asteroid (101955) Bennu: Applications of the stochastic YORP modelSystem design of the Hayabusa 2—Asteroid sample return mission to 1999 JU3The Camera of the MASCOT Asteroid Lander on Board Hayabusa 2The Rubble-Pile Asteroid Itokawa as Observed by HayabusaOn the nucleus structure and activity of comet 67P/Churyumov-GerasimenkoThe MASCOT MagnetometerSPECTRAL CHARACTERISTICS OF HAYABUSA 2 NEAR-EARTH ASTEROID TARGETS 162173 1999 JU3 AND 2001 QC34Feasibility and Accuracy of Thermophysical Estimation of Asteroid 162173 Ryugu (1999 JU3) from the Hayabusa2 Thermal Infrared ImagerThe MASCOT Radiometer MARA for the Hayabusa 2 MissionDirectional characteristics of thermal-infrared beaming from atmosphereless planetary surfaces - a new thermophysical modelFractals and Chaos in Geology and GeophysicsPortrait of the Polana–Eulalia family complex: Surface homogeneity revealed from near-infrared spectroscopySeismic resurfacing by a single impact on the asteroid 433 ErosScientific Objectives of Small Carry-on Impactor (SCI) and Deployable Camera 3 Digital (DCAM3-D): Observation of an Ejecta Curtain and a Crater Formed on the Surface of Ryugu by an Artificial High-Velocity ImpactHayabusa-2 mission target asteroid 162173 Ryugu (1999 JU<sub>3</sub>): Searching for the object’s spin-axis orientationThermal conductivity model for powdered materials under vacuum based on experimental studiesOPTICAL PROPERTIES OF (162173) 1999 JU3: IN PREPARATION FOR THE JAXA<i>HAYABUSA 2</i>SAMPLE RETURN MISSIONPreflight Calibration Test Results for Optical Navigation Camera Telescope (ONC-T) Onboard the Hayabusa2 SpacecraftDevelopment of the Laser Altimeter (LIDAR) for Hayabusa2The Small Carry-on Impactor (SCI) and the Hayabusa2 Impact ExperimentSystem Configuration and Operation Plan of Hayabusa2 DCAM3-D Camera System for Scientific Observation During SCI Impact ExperimentIrradiation History of Itokawa Regolith Material Deduced from Noble Gases in the Hayabusa SamplesThe MicrOmega Investigation Onboard Hayabusa2Regolith Migration and Sorting on Asteroid ItokawaThermal fatigue as the origin of regolith on small asteroidsDistribution of boulders and the gravity potential on asteroid ItokawaPhase II of the Small Main-Belt Asteroid Spectroscopic Survey A Feature-Based TaxonomyTHE ORIGIN OF ASTEROID 162173 (1999 JU<sub>3</sub>)Outgassing of icy bodies in the Solar System – II: Heat transport in dry, porous surface dust layersThe shape distribution of boulders on Asteroid 25143 Itokawa: Comparison with fragments from impact experimentsPhase reddening on near-Earth asteroids: Implications for mineralogical analysis, space weathering and taxonomic classificationImpact cratering experiments into quartzite, sandstone and tuff: The effects of projectile size and target properties on spallationSize-frequency statistics of boulders on global surface of asteroid 25143 ItokawaHeat capacities and entropies of silicate liquids and glassesStatic and dynamic angles of repose in loose granular materials under reduced gravityTheory of Reflectance and Emittance SpectroscopyMASCOT—The Mobile Asteroid Surface Scout Onboard the Hayabusa2 MissionDust Detection Mode of the Hayabusa2 LIDARPerformance of Hayabusa2 DCAM3-D Camera for Short-Range Imaging of SCI and Ejecta Curtain Generated from the Artificial Impact Crater Formed on Asteroid 162137 Ryugu (1999 JU 3 $\mbox{JU}_{3}$ )Small-scale topography of 25143 Itokawa from the Hayabusa laser altimeterGround-based characterization of Hayabusa2 mission target asteroid 162173 Ryugu: constraining mineralogical composition in preparation for spacecraft operationsOptical observations of NEA 162173 (1999 JU3) during the 2011-2012 apparitionThermal metamorphism of the C, G, B, and F asteroids seen from the 0.7 μm, 3 μm, and UV absorption strengths in comparison with carbonaceous chondritesDeployable Camera (DCAM3) System for Observation of Hayabusa2 Impact ExperimentSpectral reflectance properties of carbonaceous chondrites 4: Aqueously altered and thermally metamorphosed meteoritesPhysical properties of ordinary chondritesLatitudinal dependence of asteroid regolith formation by thermal fatigueModeling the Structure of High Porosity AsteroidsDebiased Orbital and Absolute Magnitude Distribution of the Near-Earth ObjectsThe nature of ponded deposits on ErosDetermination of the effective thermal conductivity of granular materials under varying pressure conditionsImaging of Small-Scale Features on 433 Eros from NEAR: Evidence for a Complex RegolithIntroducing the Eulalia and new Polana asteroid families: Re-assessing primitive asteroid families in the inner Main Belt3D shape of asteroid (6) Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondritesThe shapes of fragments from catastrophic disruption events: Effects of target shape and impact speedApollo lunar heat flow experiment revisited: A critical reassessment of the in situ thermal conductivity determinationThermal Infrared Imaging Experiments of C-Type Asteroid 162173 Ryugu on Hayabusa2Itokawa Dust Particles: A Direct Link Between S-Type Asteroids and Ordinary ChondritesAlbedo Observation by Hayabusa2 LIDAR: Instrument Performance and Error EvaluationThermal Imaging Performance of TIR Onboard the Hayabusa2 SpacecraftDetectability of hydrous minerals using ONC-T camera onboard the Hayabusa2 spacecraftRotational characterization of Hayabusa II target Asteroid (162173) 1999 JU3Spectral and rotational properties of near-Earth asteroid (162173) Ryugu, target of the Hayabusa2 sample return missionAn extension of the Bus asteroid taxonomy into the near-infraredPole and Global Shape of 25143 ItokawaInterpretation of thermal emission. I. The effect of roughness for spatially resolved atmosphereless bodiesSpectral Properties of Near-Earth Objects: Palomar and IRTF Results for 48 Objects Including Spacecraft Targets (9969) Braille and (10302) 1989 MLStony meteorite thermal properties and their relationship with meteorite chemical and physical statesDetailed Images of Asteroid 25143 Itokawa from HayabusaOSIRIS-REx: Sample Return from Asteroid (101955) BennuAre Low-Albedo Asteroids Thermally Metamorphosed?Expected shape distribution of asteroids obtained from laboratory impact experimentsThe preliminary analysis of the 4179 Toutatis snapshots of the Chang’E-2 flybyMethodology for finding and evaluating safe landing sites on small bodiesThe Brazil nut effect and its application to asteroidsSmall-Scale Topography of 433 Eros from Laser Altimetry and ImagingEffect of solid conductivity on radiative heat transfer in packed bedsSubsurface emissions from Mercury - VLA radio observations at 2 and 6 centimetersNear Earth Asteroid Rendezvous:Temperature-dependent thermal inertia of homogeneous Martian regolithThe stratification of regolith on celestial objectsImpact History of Eros: Craters and BouldersImages of Asteroid 21 Lutetia: A Remnant Planetesimal from the Early Solar SystemShoemaker crater as the source of most ejecta blocks on the asteroid 433 ErosMathilde: Size, Shape, and GeologyNear-infrared spectroscopy of 1999 JU<sub>3</sub>, the target of the Hayabusa 2 missionBlock distributions on ItokawaScaling forces to asteroid surfaces: The role of cohesionCorrelation of mechanical and thermal properties of the lunar surfaceGranular physics in low-gravity environments using discrete element methodPhotometric models of disk-integrated observations of the OSIRIS-REx target Asteroid (101955) BennuAswan site on comet 67P/Churyumov-Gerasimenko: Morphology, boulder evolution, and spectrophotometryThe formation of Ca‐, Fe‐rich silicates in reduced and oxidized <scp>CV</scp> chondrites: The roles of impact‐modified porosity and permeability, and heterogeneous distribution of water icesSpectral slope variations for OSIRIS-REx target Asteroid (101955) Bennu: Possible evidence for a fine-grained regolith equatorial ridgeA survey of possible impact structures on 25143 ItokawaA Particulate Thermophysical Model of the Lunar SoilThermophysical property models for lunar regolithHydrated Minerals on Asteroids:Radiative heat transfer at the nanoscaleSurface roughness and three-dimensional heat conduction in thermophysical modelsAsteroidal catastrophic collisions simulated by hypervelocity impact experimentsThermal diffusivity of lunar rocks under atmospheric and vacuum conditionsSize-frequency distribution of boulders ≥7 m on comet 67P/Churyumov-GerasimenkoSurface energy and the contact of elastic solidsThe Ginger-shaped Asteroid 4179 Toutatis: New Observations from a Successful Flyby of Chang'e-2Boulders on LutetiaPhotometric, spectral phase and temperature effects on 4 Vesta and HED meteorites: Implications for the Dawn missionThermal conductivity of particulate basalt as a function of density in simulated lunar and Martian environmentsCollision and gravitational reaccumulation: Possible formation mechanism of the asteroid ItokawaDark inclusions in Allende, Leoville, and Vigarano: Evidence for nebular oxidation of CV3 constituentsNumerical simulations of oscillation-driven regolith motion: Brazil-nut effectVisible spectroscopy of the Polana–Eulalia family complex: Spectral homogeneityEjecta Blocks on 243 Ida and on Other AsteroidsA three-parameter magnitude phase function for asteroidsReduced and unstratified crust in CV chondrite parent bodyThe porosity of the upper lunar regolithTHERMAL TOMOGRAPHY OF ASTEROID SURFACE STRUCTUREThe geology of 433 ErosResolved spectrophotometric properties of the Ceres surface from Dawn Framing Camera imagesThe measurement of meteorite heat capacity at low temperatures using liquid nitrogen vaporizationPhobos: Regolith and ejecta blocks investigated with Mars Orbiter Camera imagesPrediction of the porosity of multi-component mixtures of cohesive and non-cohesive particlesA new method to determine the grain size of planetary regolithWhat is controlling the reflectance spectra (0.35–150 µm) of hydrated (and dehydrated) carbonaceous chondrites?Phobos, Deimos, and the Moon: Size and distribution of crater ejecta blocksNumerical modeling of lander interaction with a low-gravity asteroid regolith surfaceNear-Earth asteroid surface roughness depends on compositional classThe Shape of 433 Eros from the NEAR-Shoemaker Laser Rangefinder均一径球形ランダム充てん粒子集合体の配位数に関する一考察
- 連携機関・データベース
- 国立情報学研究所 : CiNii Research
- 提供元機関・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CrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- 書誌ID（NDLBibID）
- 11249480
- NII論文ID
- 120006550271