Martian Moons eXploration (MMX) is a robotic space probe set for launch in 2026 to bring back the first samples from Mars' largest moon Phobos. Developed by the Japan Aerospace Exploration Agency (JAXA) and announced on 9 June 2015, MMX will land and collect samples from Phobos once or twice, along with conducting Deimos flyby observations and monitoring Mars's climate. The mission aims to provide key information to help determine whether the Martian moons are captured asteroids or the result of a larger body hitting Mars. JAXA and other Japanese government officials officially approved the MMX project to proceed into development on 19 February 2020. The probe arrived at Japan's Tanegashima Space Center on March 31, 2026, and it is expected to launch towards Mars in October 20, 2026 during the year's launch window.
Overview
The spacecraft will enter orbit around Mars before transferring to Phobos, where it will land once or twice and collect regolith samples using a pneumatic sampling system. The mission is designed to return at least 10 grams (0.35 oz) of material from the moon's surface. After departing Phobos, the spacecraft will conduct several flybys of Deimos before releasing a return capsule for Earth, with sample return planned for 2031. The spacecraft has a total launch mass of approximately 4,000 kilograms (8,800 lb), including about 1,900 kilograms (4,200 lb) of propellant. The spacecraft consists of three major elements: a 1,800-kilogram (4,000 lb) propulsion module, a 150-kilogram (330 lb) exploration module, and a 1,050-kilogram (2,310 lb) return module. Because Phobos and Deimos have insufficient mass to support conventional satellite orbits, MMX will operate in quasi-satellite orbits (QSOs), a class of trajectories that can remain stable for extended periods while staying in close proximity to the moons. The mission is led by Yasuhiro Kawakatsu.
International collaboration MMX is led by JAXA, with participation from NASA, France's CNES, Germany's DLR, and the European Space Agency (ESA), who are providing scientific instruments. NASA will contribute a neutron and gamma-ray spectrometer called MEGANE (an acronym for Mars-moon Exploration with GAmma rays and NEutrons, which also means "eyeglasses" in Japanese). CNES will provide the Near IR Spectrometer (NIRS4/MacrOmega). CNES is also contributing expertise in flight dynamics to plan the mission's orbiting and landing manoeuvres. Development and testing of key components, including the sampler, is ongoing. As of December 2023, MMX is scheduled to be launched in 2026, and will return to Earth five years later in 2031. ESA will provide deep space communication equipment: a transponder and power amplifier, and will provide ground station support from the Estrack network. The sample-return capsule will land in Australia.
Spacecraft instruments MMX will have seven scientific instruments:
TENGOO – TElescopic Nadir imager for GeOmOrphology, a narrow field camera for detailed terrain study OROCHI – Optical RadiOmeter composed of CHromatic Imagers, a wide field visible light camera LIDAR – Light Detection and Ranging, uses a laser to reflect light from the moon's surface, to study surface altitude and albedo MIRS – MMX InfraRed Spectrometer, a near-infrared observation device for characterizing the minerals that make up the moons of Mars. Developed in partnership with CNES, France MEGANE – (MEGANE means "eyeglasses" in Japanese) Mars-moon Exploration with GAmma rays and NEutrons, a gamma-ray and neutron spectrometer developed by NASA, Johns Hopkins Applied Physics Laboratory, and Lawrence Livermore National Laboratory CMDM – Circum-Martian Dust Monitor, a dust counting device for characterizing the environment around the Martian moons MSA – Mass Spectrum Analyzer, an instrument to study the ion environment around Mars JAXA will partner with the Japan Broadcasting Corporation (NHK) to develop the "Super Hi-Vision Camera" which combines a 4K and 8K camera, making it the first time that Mars will be imaged in 8K resolution. Images will be regularly transmitted back to Earth with flight data, in order to recreate MMX exploration around Mars and its moons. The original image data will be stored in a recording device in MMX's return capsule and brought back to Earth as part of the sample-return portion of the mission. The Gravity GradioMeter (GGM), Laser-Induced Breakdown Spectroscope (LIBS), Mission Survival Module (MSM) were proposed as additional instruments.
Idefix rover
Following a study by the French CNES space agency, it was decided that the spacecraft will deliver a small rover provided by CNES and the German Aerospace Center (DLR). IDEFIX is a rover weighing less than 30 kg, and is named after Idéfix, the French name for Dogmatix, Obelix's dog in the French comic Asterix. The name Idefix (without acute accent) is also used for the character in the German translation. Besides its native France the Asterix series has been particularly successful in Germany — out of 350 million comic books sold worldwide by 2013, 130 million were in the French original while 120 million were in German. It will be equipped with cameras, a radiometer, and a Raman spectrometer for in-situ surface exploration. The instruments are: two navigation cameras (NavCams), two cameras (WheelCams) "that will observe the interactions of the back and front wheels with the regolith", a Raman spectrometer (RAX) and a miniaturized radiometer (miniRad). Its objectives are to touch the surface of Phobos, to check the behaviour of the surface under mechanical actions and to relay this information to Earth. It must also demonstrate that it is possible to use wheeled locomotion on a body with such low gravity. Finally, it will take measurements in situ, observing the ground of Phobos at a resolution of 100 μm, and moving around on it.
Sampling
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