Mio—First Comprehensive Exploration of Mercury’s Space Environment: Mission Overview

被引:0
作者
Go Murakami
Hajime Hayakawa
Hiroyuki Ogawa
Shoya Matsuda
Taeko Seki
Yasumasa Kasaba
Yoshifumi Saito
Ichiro Yoshikawa
Masanori Kobayashi
Wolfgang Baumjohann
Ayako Matsuoka
Hirotsugu Kojima
Satoshi Yagitani
Michel Moncuquet
Jan-Erik Wahlund
Dominique Delcourt
Masafumi Hirahara
Stas Barabash
Oleg Korablev
Masaki Fujimoto
机构
[1] Japan Aerospace Exploration Agency,Institute of Space and Astronautical Science
[2] Tohoku University,Planetary Plasma and Atmospheric Research Center, Graduate School of Science
[3] The University of Tokyo,Department of Complexity Science and Engineering
[4] Chiba Institute of Technology,Planetary Exploration Research Center
[5] Austrian Academy of Sciences,Space Research Institute
[6] Kyoto University,Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science
[7] Kyoto University,Research Institute for Sustainable Humanosphere
[8] Kanazawa University,Advanced Research Center for Space Science and Technology
[9] CNRS,LESIA, Observatoire de Paris, Université PSL
[10] Swedish Institute of Space Physics,Institute of Space
[11] CNRS-Universite d’Orleans-CNES,Earth Environmental Research
[12] Nagoya University,undefined
[13] Swedish Institute of Space Physics,undefined
[14] IKI-RAS Space Research Institute of Russian Academy of Science,undefined
来源
Space Science Reviews | 2020年 / 216卷
关键词
Mercury; Magnetosphere; Exosphere; BepiColombo; Mercury Magnetospheric Orbiter (MMO); Mio;
D O I
暂无
中图分类号
学科分类号
摘要
Mercury has a unique and complex space environment with its weak global magnetic field, intense solar wind, tenuous exosphere, and magnetospheric plasma particles. This complex system makes Mercury an excellent science target to understand effects of the solar wind to planetary environments. In addition, investigating Mercury’s dynamic magnetosphere also plays a key role to understand extreme exoplanetary environment and its habitability conditions against strong stellar winds. BepiColombo, a joint mission to Mercury by the European Space Agency and Japan Aerospace Exploration Agency, will address remaining open questions using two spacecraft, Mio and the Mercury Planetary Orbiter. Mio is a spin-stabilized spacecraft designed to investigate Mercury’s space environment, with a powerful suite of plasma instruments, a spectral imager for the exosphere, and a dust monitor. Because of strong constraints on operations during its orbiting phase around Mercury, sophisticated observation and downlink plans are required in order to maximize science outputs. This paper gives an overview of the Mio spacecraft and its mission, operations plan, and data handling and archiving.
引用
收藏
相关论文
共 558 条
[11]  
Russell C.L.(2004)The BepiColombo/MMO model payload and operation plan Adv. Space Res. 33 238-10,154
[12]  
Hori T.(2010)The plasma wave investigation (PWI) onboard the BepiColombo/MMO: first measurement of electric fields, electromagnetic waves, and radio waves around Mercury Planet. Space Sci. 58 10,147-2876
[13]  
Kasahara Y.(2020)Plasma Wave Investigation (PWI) aboard BepiColombo Mio on the trip to the first measurement of electric fields, electromagnetic waves, and radio waves around Mercury Space Sci. Rev. 216 2851-79
[14]  
Kumamoto A.(2020)Mission Data Processor aboard the BepiColombo Mio spacecraft: design and scientific operation concept Space Sci. Rev. 216 72-27
[15]  
Matsuoka A.(2017)A dynamic model of Mercury’s magnetospheric magnetic field Geophys. Res. Lett. 44 3-94
[16]  
Miyashita Y.(2015)Comprehensive survey of energetic electron events in Mercury’s magnetosphere with data from the MESSENGER Gamma-Ray and Neutron Spectrometer J. Geophys. Res. 120 92-613
[17]  
Miyoshi Y.(2016)MESSENGER X-ray observations of magnetosphere-surface interaction on the nightside of Mercury Planet. Space Sci. 125 610-443
[18]  
Shinohara I.(2013)Science objectives and rationale for the Radiation Belt Storm Probes mission Space Sci. Rev. 179 397-70
[19]  
Teramoto M.(2008)Mercury’s exosphere: observations MESSENGER’s first Mercury flyby Science 321 93-9
[20]  
Faden J.B.(2009)Mercury’s exosphereduring MESSENGER’s second flyby: detection of magnesium and distinct distributions of neutral species Science 324 101-115