Asteroid Ryugu before the Hayabusa2 encounter
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- Material Type
- 記事
- Author/Editor
- Koji WadaMatthias GrottPatrick Michel
- Publication, Distribution, etc.
- Publication Date
- 2018-12-11
- Publication Date (W3CDTF)
- 2018-12-11
- Periodical title
- Progress in earth and planetary science
- No. or year of volume/issue
- 5(82)
- Volume
- 5(82)
- ISSN (Periodical Title)
- 2197-4284
- ISSN-L (Periodical Title)
- 2197-4284
- Text Language Code
- eng
- DOI
- 10.1186/s40645-018-0237-y
- Persistent ID (NDL)
- info:ndljp/pid/11249480
- 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)
- 2019-03-05T23:10:26+09:00
- Date Captured (W3CDTF)
- 2019-03-05
- 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/11018906
- 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.
- 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.
- Related Material (URI)
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- 国立情報学研究所 : CiNii Research
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- 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
- Bibliographic ID (NDL)
- 11249480
- NAID
- 110008428229
- Summary, etc.
- 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
- Access Restrictions
- インターネット公開
- Rights (production)
- © 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.
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- Is Referenced By
- 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
- References
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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
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- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
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- Bibliographic ID (NDL)
- 11249480
- NAID
- 120006550271