The Mars system revealed by the Martian Moons eXploration mission
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- 資料種別
- 記事
- 著者・編者
- Kazunori OgoharaHiromu NakagawaShohei Aoki
- 出版年月日等
- 2022-01-03
- 出版年（W3CDTF）
- 2022-01-03
- タイトル（掲載誌）
- EPS : Earth, Planets and Space
- 巻号年月日等（掲載誌）
- 74(1)
- 掲載巻
- 74(1)
- 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/s40623-021-01417-0
- 国立国会図書館永続的識別子
- info:ndljp/pid/12287069
- 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
- Japan Aerospace Exploration Agency (JAXA) plans a Phobos sample return mission (MMX: Martian Moons eXploration). In this study, we review the related works on the past climate of Mars, its evolution, and the present climate and weather to describe the scientific goals and strategies of the MMX mission regarding the evolution of the Martian surface environment. The MMX spacecraft will retrieve and return a sample of Phobos regolith back to Earth in 2029. Mars ejecta are expected to be accumulated on the surface of Phobos without being much shocked. Samples from Phobos probably contain all types of Martian rock from sedimentary to igneous covering all geological eras if ejecta from Mars could be accumulated on the Phobos surface. Therefore, the history of the surface environment of Mars can be restored by analyzing the returned samples. Remote sensing of the Martian atmosphere and monitoring ions escaping to space while the spacecraft is orbiting Mars in the equatorial orbit are also planned. The camera with multi-wavelength filters and the infrared spectrometer onboard the spacecraft can monitor rapid transport processes of water vapor, dust, ice clouds, and other species, which could not be traced by the previous satellites on the sun-synchronous polar orbit. Such time-resolved pictures of the atmospheric phenomena should be an important clue to understand both the processes of water exchange between the surface/underground reservoirs and the atmosphere and the drivers of efficient material transport to the upper atmosphere. The mass spectrometer with unprecedented mass resolution can observe ions escaping to space and monitor the atmospheric escape which has made the past Mars to evolve towards the cold and dry surface environment we know today. Together with the above two instruments, it can potentially reveal what kinds of atmospheric events can transport tracers (e.g., H2O) upward and enhance the atmospheric escape.
- DOI
- 10.1186/s40623-021-01417-0
- 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) 2021.This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder.
- 関連情報（URI）
- 参照
- 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 ModelDevelopment of observation strategies from mission design to operations: illustration with Mars moons Explorer infrared spectrometer (MIRS)Special issue “Martian Moons eXploration: the scientific investigations of Mars and its moons”In situ observations of ions and magnetic field around Phobos : the mass spectrum analyzer (MSA) for the Martian Moons eXploration (MMX) missionScience operation plan of Phobos and Deimos from the MMX spacecraftMartian moons exploration MMX : sample return mission to Phobos elucidating formation processes of habitable planetsDesign of telescopic nadir imager for geomorphology (TENGOO) and observation of surface reflectance by optical chromatic imager (OROCHI) for the Martian Moons Exploration (MMX)
- 参照
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Seasonality or Erosion by Superimposed Bedforms?Diurnal Variations of Dust During the 2018 Global Dust Storm Observed by the Mars Climate SounderAn Observational Overview of Dusty Deep Convection in Martian Dust StormsThe martian daytime convective boundary layer: Results from radio occultation measurements and a mesoscale modelCapture of solar wind alpha‐particles by the Martian atmosphereThree‐dimensional multifluid simulations of ionospheric loss at Mars from nominal solar wind conditions to magnetic cloud eventsIon Energization and Escape on Mars and VenusSurface and near-surface atmospheric temperatures for the Mars Exploration Rover landing sitesDust haze in Valles Marineris observed by HRSC and OMEGA on board Mars ExpressAtmosphere and Water Loss from Early Mars Under Extreme Solar Wind and Extreme Ultraviolet ConditionsNOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected PerformanceMeteoritic evidence for a previously unrecognized hydrogen reservoir on MarsCold Dense Ion Outflow Observed in the Martian‐Induced Magnetotail by MAVENEffects of a Weak Intrinsic Magnetic Field on Atmospheric Escape From MarsThe potential science and engineering value of samples delivered to Earth by Mars sample returnThe Importance of Phobos Sample Return for Understanding the Mars-Moon SystemIon Jets Within Current Sheets in the Martian MagnetosphereLoss and Fractionation of Noble Gas Isotopes and Moderately Volatile Elements from Planetary Embryos and Early Venus, Earth and MarsElevated atmospheric escape of atomic hydrogen from Mars induced by high-altitude waterMAVEN observations of tail current sheet flapping at MarsPhobos-2 results on the ionospheric plasma escape from MarsExposed subsurface ice sheets in the Martian mid-latitudesEffects of obliquity and water vapor/trace gas greenhouses in the early martian climateHeavy-ion flux enhancement in the vicinity of the Martian ionosphere during CIR passage: Mars Express ASPERA-3 observationsDiscovery of diffuse aurora on MarsRedox State of Mars' Upper Mantle and Crust from Eu Anomalies in Shergottite PyroxenesAn intense terminal epoch of widespread fluvial activity on early Mars: 1. 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products in SNC meteoritesMHD model results of solar wind interaction with Mars and comparison with MAVEN plasma observationsVolatiles Measured by the Phoenix Lander at the Northern Plains of MarsWater vapour in the atmosphere of MarsThe retrieval of altitude profiles of the Martian aerosol microphysical characteristics from the limb measurements of the Mars Express OMEGA spectrometerEffects of Global and Regional Dust Storms on the Martian Hot O Corona and Photochemical LossSeasonal variation of Martian pick-up ions: Evidence of breathing exosphereThe spatial distribution of planetary ion fluxes near Mars observed by MAVENMAVEN observations of a giant ionospheric flux rope near Mars resulting from interaction between the crustal and interplanetary draped magnetic fieldsStatistical analysis of the reflection of incident O<sup>+</sup> pickup ions at Mars: MAVEN observationsWhat Geology and Mineralogy Tell Us About Water on MarsThe Atmospheric Chemistry Suite (ACS) of Three Spectrometers 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- 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Crossref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CrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- 書誌ID（NDLBibID）
- 12287069