@article{oai:repo.qst.go.jp:00084936,
 author = {Nakamura, Tomoki and Ikeda, Hitoshi and Kouyama, Toru and Nakagawa, Hiromu and Kusano, Hiroki and Senshu, Hiroki and Kameda, Shingo and Matsumoto, Koji and Ferran, Gonzalez-Franquesa and Ozaki, Naoya and Takeo, Yosuke and Baresi, Nicola and Oki, Yusuke and J. Lawrence, David and L. Chabot, Nancy and N. Peplowski, Patrick and Antonietta Barucci, Maria and Sawyer, Eric and Yokota, Shoichiro and Terada, Naoki and Ulamec, Stephan and Michel, Patrick and Kobayashi, Masanori and Sasaki, Sho and Hirata, Naru and Wada, Koji and Miyamoto, Hideaki and Imamura, Takeshi and Ogawa, Naoko and Ogawa, Kazunori and Iwata, Takahiro and Imada, Takane and Otake, Hisashi and Canalias, Elisabet and Lorda, Laurence and Tardivel, Simon and Stéphane, Mary and Kunugi, Makoto and Mitsuhashi, Seiji and Doressoundiram, Alain and Frédéric, Merlin and Fornasier, Sonia and Jean-Michel, Reess and Bernardi, Pernelle and Imai, Shigeru and Ito, Yasuyuki and Ishida, Hatsumi and Kuramoto, Kiyoshi and Kawakatsu, Yasuhiro and Hiroki, Kusano},
 journal = {Earth, Planets and Space},
 month = {Dec},
 note = {The science operations of the spacecraft and remote sensing instruments for the Martian Moon eXploration (MMX) mission are discussed by the mission operation working team. In this paper, we describe the Phobos observations during the first 1.5 years of the spacecraft’s stay around Mars, and the Deimos observations before leaving the Martian system. In the Phobos observation, the spacecraft will be placed in low-altitude quasi-satellite orbits on the equatorial plane of Phobos and will make high-resolution topographic and spectroscopic observations of the Phobos surface from five different altitudes orbits. The spacecraft will also attempt to observe polar regions of Phobos from a three-dimensional quasi-satellite orbit moving out of the equatorial plane of Phobos. From these observations, we will constrain the origin of Phobos and Deimos and select places for landing site candidates for sample collection. For the Deimos observations, the spacecraft will be injected into two resonant orbits and will perform many flybys to observe the surface of Deimos over as large an area as possible.},
 title = {Science operation plan of Phobos and Deimos from the MMX spacecraft},
 volume = {73},
 year = {2021}
}