Science operation plan of Phobos and Deimos from the MMX spacecraft
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Published:2021-12
Issue:1
Volume:73
Page:
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ISSN:1880-5981
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Container-title:Earth, Planets and Space
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language:en
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Short-container-title:Earth Planets Space
Author:
Nakamura TomokiORCID, Ikeda Hitoshi, Kouyama Toru, Nakagawa Hiromu, Kusano Hiroki, Senshu Hiroki, Kameda Shingo, Matsumoto Koji, Gonzalez-Franquesa Ferran, Ozaki Naoya, Takeo Yosuke, Baresi Nicola, Oki Yusuke, Lawrence David J., Chabot Nancy L., Peplowski Patrick N., Barucci Maria Antonietta, Sawyer Eric, Yokota Shoichiro, Terada Naoki, Ulamec Stephan, Michel Patrick, Kobayashi Masanori, Sasaki Sho, Hirata Naru, Wada Koji, Miyamoto Hideaki, Imamura Takeshi, Ogawa Naoko, Ogawa Kazunori, Iwata Takahiro, Imada Takane, Otake Hisashi, Canalias Elisabet, Lorda Laurence, Tardivel Simon, Mary Stéphane, Kunugi Makoto, Mitsuhashi Seiji, Doressoundiram Alain, Merlin Frédéric, Fornasier Sonia, Reess Jean-Michel, Bernardi Pernelle, Imai Shigeru, Ito Yasuyuki, Ishida Hatsumi, Kuramoto Kiyoshi, Kawakatsu Yasuhiro
Abstract
AbstractThe 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.
Graphical Abstract
Funder
MMX project NASA Discovery Program CNES
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Geology
Cited by
31 articles.
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