TY - JOUR
T1 - Mio—First Comprehensive Exploration of Mercury’s Space Environment
T2 - Mission Overview
AU - Murakami, Go
AU - Hayakawa, Hajime
AU - Ogawa, Hiroyuki
AU - Matsuda, Shoya
AU - Seki, Taeko
AU - Kasaba, Yasumasa
AU - Saito, Yoshifumi
AU - Yoshikawa, Ichiro
AU - Kobayashi, Masanori
AU - Baumjohann, Wolfgang
AU - Matsuoka, Ayako
AU - Kojima, Hirotsugu
AU - Yagitani, Satoshi
AU - Moncuquet, Michel
AU - Wahlund, Jan Erik
AU - Delcourt, Dominique
AU - Hirahara, Masafumi
AU - Barabash, Stas
AU - Korablev, Oleg
AU - Fujimoto, Masaki
N1 - Funding Information:
The authors wish to express sincere appreciation to all the members in the PI teams, the Mio science working group, the project teams of JAXA and ESA, and the industries for their long contributions to science managements, spacecraft developments, testing, and operations planning. Especially the authors would like to thank Dr. Hiroshi Yamakawa, Dr. Toshifumi Mukai, Dr. Hiroshi Matsumoto, Dr. Jean-Louis Bougeret, Dr. Lars Blomberg, Dr. Ken’ichi Nogami, Dr. Hiromi Shibata, and Dr. Jean-Andre Sauvaud for their efforts to the mission from the beginning.
Publisher Copyright:
© 2020, Springer Nature B.V.
PY - 2020/10/1
Y1 - 2020/10/1
N2 - 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.
AB - 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.
KW - BepiColombo
KW - Exosphere
KW - Magnetosphere
KW - Mercury
KW - Mercury Magnetospheric Orbiter (MMO)
KW - Mio
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U2 - 10.1007/s11214-020-00733-3
DO - 10.1007/s11214-020-00733-3
M3 - Review article
AN - SCOPUS:85082336712
SN - 0038-6308
VL - 216
JO - Space Science Reviews
JF - Space Science Reviews
IS - 7
M1 - 113
ER -