Martian Moons Exploration MMX: Sample Return Mission to Phobos Elucidating Formation Processes of Habitable Planets

Author:

Kuramoto Kiyoshi1ORCID,Kawakatsu Yasuhiro2,Fujimoto Masaki2,Araya Akito3,Barucci Maria Antonietta4,Genda Hidenori5,Hirata Naru6,Ikeda Hitoshi2,Imamura Takeshi3,Helbert Jörn7,Kameda Shingo8,Kobayashi Masanori9,Kusano Hiroki10,Lawrence David J.11,Matsumoto Koji12,Michel Patrick13,Miyamoto Hideaki3,Morota Tomokatsu3,Nakagawa Hiromu14,Nakamura Tomoki15,Ogawa Kazunori2,Otake Hisashi2,Ozaki Masanobu2,Russel Sara16,Sasaki Sho17,Sawada Hirotaka2,Senshu Hiroki18,Tachibana Shogo3,Terada Naoki14,Ulamec Stephan19,Usui Tomohiro2,Wada Koji18,Watababe Sei-ichiro20,Yokota Shoichiro17

Affiliation:

1. Hokkaido University

2. JAXA

3. The University of Tokyo: Tokyo Daigaku

4. Paris Observatory: Observatoire de Paris

5. Tokyo Institute of Technology

6. The University of Aizu: Aizu Daigaku

7. Deutsches Zentrum fur Luft- und Raumfahrt DLR

8. Rikkyo University

9. Chiba Institute of Technology

10. National Institutes for Quantum and Radiological Science and Technology

11. Johns Hopkins University Applied Physics Laboratory

12. National Astronomical Observatory of Japan

13. Universite Cote d'Azur

14. Tohoku University: Tohoku Daigaku

15. Tohoku University

16. Natural History Museum

17. Osaka University: Osaka Daigaku

18. Chiba Institute of Technology: Chiba Kogyo Daigaku

19. Deutsches Zentrum für Luft- und Raumfahrt DRL

20. Nagoya University: Nagoya Daigaku

Abstract

Abstract Martian moons exploration, MMX, is the new sample return mission planned by the Japan Aerospace Exploration Agency (JAXA) targeting the two Martian moons with a scheduled launch in 2024 and a return to the Earth in 2029. The major scientific objectives of this mission are to determine the origin of Phobos and Deimos, to elucidate the early Solar System evolution in terms of volatile delivery across the snow line to the terrestrial planets having habitable surface environments, and to explore the evolutionary processes of both moons and Mars surface environment. To achieve these objectives, during a stay in circum-Martian space over about 3 years MMX will collect samples from Phobos along with close-up observations of this inner moon and carry out multiple flybys of Deimos to make comparative observations of this outer moon. Simultaneously, successive observations of the Martian atmosphere will also be made by utilizing the advantage of quasi-equatorial spacecraft orbits along the moons’ orbits.

Publisher

Research Square Platform LLC

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