Martian moons exploration MMX : sample return mission to Phobos elucidating formation processes of habitable planets
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DOI[10.1186/s40623-021-01545-7]のデータに遷移します
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- 資料種別
- 記事
- 著者・編者
- Kiyoshi KuramotoYasuhiro KawakatsuMasaki Fujimoto
- 出版年月日等
- 2022-01-20
- 出版年（W3CDTF）
- 2022-01-20
- タイトル（掲載誌）
- EPS : Earth, Planets and Space
- 巻号年月日等（掲載誌）
- 74(12)
- 掲載巻
- 74(12)
- ISSN（掲載誌）
- 1880-5981
- ISSN-L（掲載誌）
- 1343-8832
- 本文の言語コード
- eng
- DOI
- 10.1186/s40623-021-01545-7
- 国立国会図書館永続的識別子
- info:ndljp/pid/12287080
- 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）
- 2022-05-18T20:14:28+09:00
- 保存日（W3CDTF）
- 2022-04-27
- 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/12287068
- 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
- コレクション : 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
- DOI
- 10.1186/s40623-021-01545-710.21203/rs.3.rs-163944/v1
- 関連情報（URI）
- 参照
- Optical Pulse Detection IC LIDARX Integrated in MMX-LIDARInsights into the origins of Phobos and Deimos based on a spectral comparison with small bodies and Martian materialsGeochemical and dynamical views on the origin of Earth's atmosphere and oceansSpectro-photometry of Phobos simulantsStable carbon isotope evolution of formaldehyde on early MarsOrigin of Phobos and Deimos Awaiting Direct ExplorationStable Orbiting Around Small Moons Using J2-Perturbed Elliptic Restricted ProblemSimulation of gravity field estimation of Phobos for Martian Moon eXploration (MMX)Modeling 4.3 billion years of water history on PhobosMixing model of Phobos’ bulk elemental composition for the determination of its origin: Multivariate analysis of MMX/MEGANE dataCuration protocol of Phobos sample returned by Martian Moons eXplorationSpecial issue “Martian Moons eXploration: the scientific investigations of Mars and its moons”Fraunhofer line-based wavelength-calibration method without calibration targets for planetary lander instrumentsOptimizing Image Compression Ratio for Generating Highly Accurate Local Digital Terrain Models: Experimental Study for Martian Moons eXploration MissionHeliocentric Distance Dependence of Zodiacal Light Observed by Hayabusa2#Exploring the Recycling Model of Phobos Formation: Rubble-pile Satellites*Strong Depletion of <sup>13</sup>C in CO Induced by Photolysis of CO<sub>2</sub> in the Martian Atmosphere, Calculated by a Photochemical ModelPreliminary design of Martian Moons eXploration (MMX)The MMX rover : performing in situ surface investigations on PhobosThe Mars system revealed by the Martian Moons eXploration missionStray light analysis by ray tracing simulation for the wide-angle multiband camera OROCHI onboard the Martian Moons eXploration (MMX) spacecraftIn situ science on Phobos with the Raman spectrometer for MMX (RAX) : preliminary design and feasibility of Raman measurementsMMX geodesy investigations : science requirements and observation strategyScience operation plan of Phobos and Deimos from the MMX spacecraftDesign of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)In situ observations of ions and magnetic field around Phobos : the mass spectrum analyzer (MSA) for the Martian Moons eXploration (MMX) missionSurface environment of Phobos and Phobos simulant UTPSMIRS : an imaging spectrometer for the MMX mission
- 参照
- The MMX rover : performing in situ surface investigations on PhobosThe Mars system revealed by the Martian Moons eXploration missionIn situ science on Phobos with the Raman spectrometer for MMX (RAX) : preliminary design and feasibility of Raman measurementsMMX geodesy investigations : science requirements and observation strategyScience operation plan of Phobos and Deimos from the MMX spacecraftDesign of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)Light detection and ranging (LIDAR) laser altimeter for the Martian Moons Exploration (MMX) spacecraftIn situ observations of ions and magnetic field around Phobos : the mass spectrum analyzer (MSA) for the Martian Moons eXploration (MMX) missionSmall-scale topographic irregularities on Phobos : image and numerical analyses for MMX missionSurface environment of Phobos and Phobos simulant UTPSMIRS : an imaging spectrometer for the MMX missionSearching for life on Mars and its moonsAnalytical protocols for Phobos regolith samples returned by the Martian Moons eXploration (MMX) missionImplantation of Martian atmospheric ions within the regolith of PhobosCollisional formation of top-shaped asteroids and implications for the origins of Ryugu and BennuThe Importance of Phobos Sample Return for Understanding the Mars-Moon SystemTiming of thermal metamorphism in CM chondrites: Implications for Ryugu and Bennu future sample returnThe composition of MarsMorphology and Morphometry of Sub-kilometer Craters on the Nearside of Phobos and Implications for Regolith PropertiesTransport of impact ejecta from Mars to its moons as a means to reveal Martian historyMeasuring the Elemental Composition of Phobos: The Mars‐moon Exploration with GAmma rays and NEutrons (MEGANE) Investigation for the Martian Moons eXploration (MMX) MissionPhobos Surface Sputtering as Inferred From MAVEN Ion ObservationsThe geomorphology, color, and thermal properties of Ryugu: Implications for parent-body processesHayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top–shaped rubble pileLoss of the Martian atmosphere to space: Present-day loss rates determined from MAVEN observations and integrated loss through timeThe OSIRIS-REx Spacecraft and the Touch-and-Go Sample Acquisition Mechanism (TAGSAM)Mars’ growth stunted by an early giant planet instabilityThermal and impact histories of 25143 Itokawa recorded in Hayabusa particlesIn situ observations of dust particles in Martian dust belts using a large-sensitive-area dust sensorOn the Impact Origin of Phobos and Deimos. IV. Volatile DepletionMission analysis for the Martian Moons Explorer (MMX) missionOrigin of Phobos and Deimos by the impact of a Vesta-to-Ceres sized body with MarsHydrogen escape from Mars enhanced by deep convection in dust stormsSolar Wind Sputtering Rates of Small Bodies and Ion Mass Spectrometry Detection of Secondary IonsFormation of an Ultracarbonaceous Antarctic Micrometeorite through Minimum Aqueous Alteration in a Small Porous Icy BodyOn the Impact Origin of Phobos and Deimos. I. Thermodynamic and Physical AspectsGlobal Mars‐solar wind coupling and ion escapeCollisional history of asteroid ItokawaAn ongoing satellite–ring cycle of Mars and the origins of Phobos and DeimosHayabusa2 Sampler: Collection of Asteroidal Surface MaterialAccretion of Phobos and Deimos in an extended debris disc stirred by transient moonsThe Phobos neutral and ionized torusOrigin of Earth’s oceans: An assessment of the total amount, history and supply of water<sup>40</sup>Ar/<sup>39</sup>Ar age of material returned from asteroid 25143 ItokawaPetrology on MarsFormation of Phobos and Deimos via a giant impactStrong water isotopic anomalies in the martian atmosphere: Probing current and ancient reservoirs67P/Churyumov-Gerasimenko, a Jupiter family comet with a high D/H ratioPhobos and DeimosMeteoritic evidence for a previously unrecognized hydrogen reservoir on MarsSpacecraft exploration of Phobos and DeimosThe surface geology and geomorphology of PhobosThe age of Phobos and its largest crater, StickneyThe Phobos information systemThe meteoroid environment and impacts on PhobosCharacter and origin of Phobos’ groovesMartian planetary heavy ion sputtering of PhobosRelationship between regolith particle size and porosity on small bodiesSpectral absorptions on Phobos and Deimos in the visible/near infrared wavelengths and their compositional constraintsSolar System evolution from compositional mapping of the asteroid beltA Habitable Fluvio-Lacustrine Environment at Yellowknife Bay, Gale Crater, MarsMars impact ejecta in the regolith of Phobos: Bulk concentration and distributionSystem design of the Hayabusa 2—Asteroid sample return mission to 1999 JU3Oxygen three-isotope ratios of silicate particles returned from asteroid Itokawa by the Hayabusa spacecraft: A strong link with equilibrated LL chondritesVolatile, Isotope, and Organic Analysis of Martian Fines with the Mars Curiosity RoverAbundance and Isotopic Composition of Gases in the Martian Atmosphere from the Curiosity Rover<sup>26</sup>Al‐<sup>26</sup>Mg isotope systematics of the first solids in the early solar systemRocket dust storms and detached dust layers in the Martian atmosphereA new method to determine the grain size of planetary regolithThe bombardment history of the Moon as recorded by <sup>40</sup>Ar‐<sup>39</sup>Ar chronologyAnalysis of disk‐resolved OMEGA and CRISM spectral observations of Phobos and DeimosEvidence for the late formation of hydrous asteroids from young meteoritic carbonatesStable-isotopic anomalies and the accretionary assemblage of the Earth and Mars: A subordinate role for carbonaceous chondritesThe Chemical Composition of Comets—Emerging Taxonomies and Natal HeritageThe origin of the Martian moons revisitedItokawa Dust Particles: A Direct Link Between S-Type Asteroids and Ordinary ChondritesIrradiation History of Itokawa Regolith Material Deduced from Noble Gases in the Hayabusa SamplesOxygen Isotopic Compositions of Asteroidal Materials Returned from Itokawa by the Hayabusa MissionA low mass for Mars from Jupiter’s early gas-driven migrationHf–W–Th evidence for rapid growth of Mars and its status as a planetary embryoAre Phobos and Deimos the result of a giant impact?Backscattered solar wind protons by PhobosA comparison of global models for the solar wind interaction with MarsTHE ORBITS AND MASSES OF THE MARTIAN SATELLITES AND THE LIBRATION OF PHOBOSHf–W chronology of the accretion and early evolution of asteroids and terrestrial planetsFirst direct detection of ions originating from the Moon by MAP‐PACE IMA onboard SELENE (KAGUYA)A survey of possible impact structures on 25143 ItokawaSolar cosmic ray records in lunar rock 6445553Mn–53Cr systematics of the early Solar System revisitedCoupled 142Nd–143Nd evidence for a protracted magma ocean in MarsWater vapor mapping on Mars using OMEGA/Mars ExpressThe Rubble-Pile Asteroid Itokawa as Observed by HayabusaGlobal Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express DataThe global effects of impact-induced seismic activity on fractured asteroid surface morphologyISM observation of Phobos reinvestigated: Identification of a mixture of olivine and low‐calcium pyroxeneMars atmospheric escape and evolution; interaction with the solar windNear-Infrared Spectrophotometry of Phobos and DeimosEvidence for recent climate change on Mars from the identification of youthful near-surface ground iceOligarchic Growth of ProtoplanetsMartian Dust Belts: Waiting for DiscoveryThe Surface of Deimos: Contribution of Materials and Processes to Its Unique AppearanceSolar wind measurements near Mars and their implication in the Red Planet environmentWater On MarsMars Atmospheric Loss and Isotopic Fractionation by Solar-Wind-Induced Sputtering and Photochemical EscapeThe origin of Phobos' grooves and crater chainsGravity, Tides, and Topography on Small Satellites and Asteroids: Application to Surface Features of the Martian SatellitesOxygen Isotopes in MeteoritesThe Stickney Impact of Phobos: A Dynamical ModelShock metamorphism of ordinary chondritesEvolution of the water regime of PhobosThe shapes of small satellitesCompositions of chondritesRelease of Juvenile Water on Mars: Estimated Amounts and Timing Associated with VolcanismCollisional balance of the meteoritic complexOrbital evolution and origin of the Martian satellitesTidal rigidity of phobosThe compositional classification of chondrites—I. The carbonaceous chondrite groupsThe Moons of MarsSpectral evidence for a carbonaceous chondrite surface composition on DeimosSurface features of Phobos and DeimosProperties and effects of dust particles suspended in the Martian atmosphereGas drag in primordial circumplanetary envelopes: A mechanism for satellite captureCapture of Phobos and Deimos by photoatmospheric dragViking First Encounter of Phobos: Preliminary ResultsThe Composition of Phobos: Evidence for Carbonaceous Chondrite Surface from Spectral AnalysisThe dynamical evolution and origin of the Martian moonsViking observations of Phobos and Deimos: Preliminary resultsPhotometric properties of the Martian satellitesDynamical characteristics of Phobos and DeimosInclination of satellite orbits about an oblate precessing planet
- 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
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