The MMX mission will travel to
Mars and survey the red planet’s two moons; Phobos and Deimos.
The spacecraft will explore both moons and collect a sample
from one of the moons to bring back to Earth.

NEW

2017.04.05
MMX website is now open

What’s MMX?

ISAS/JAXA plan to launch MMX in early 2020s.In order to retrieve the samples, MMX will need to complete a roundtrip to Mars, circle around the moon and land on its surface. The most complex and risky parts of this mission are the operations around the moons and the decent and landing. These heavily constrain the system design and have involved an in-depth study from the earliest stages of the mission.

The primary mission objective is to distinguish between the two leading hypothesise for the origin of Phobos and Deimos. The first of these suggests the moons are captured primitive asteroids, while the second proposes that they are the agglomerated fragments of a giant impact event on Mars.

The second objective is to characterise the conditions on and around the moons. This includes surface processes on Phobos and Deimos, the nature of the circum-Martian environment (the region where objects orbit around the planet) and the global and temporal dynamics of Mars’s atmosphere, such as dust, ice, clouds and water vapour.

Objective

Mars is the outermost rocky planet in our Solar System and marks the boundary between terrestrial planets with solid surfaces and thin atmospheres, and the gas giants worlds like Jupiter and Saturn.

Understanding the origin of our fourth planet’s moons will give clues to how the planets formed around our Sun and in turn, around other stars. If captured, these small satellites are evidence of the material that was scattered inwards towards the Sun by the gas giant planets. This would make them kin to the meteorites that struck the early Earth and possibly delivered water and organic compounds to our planet. Alternatively, Phobos and Deimos may be the remnants of a giant collision with Mars that threw material from the Martian surface to accumulate into the two moons. In this case, the moons may be a time capsule for early Martian conditions and reveal details on the giant impact process that is also thought to have formed our own Moon.

The goal of MMX mission is to reveal the origin of the Martian moons and progress our understanding of planetary system formation and primordial material transport around the boundary between the inner- and outer- early Solar System.

Science

Preliminary Mission Schedule:

Launch: September 2024
Mars Arrival: August 2025
Mars Departure: August 2028
Return to Earth: July 2029

  • 1. To reveal the origin of Phobos and Deimos
  • 2. Understand processes in the circum-Martian environment

Probe

CONFIGURATION

NOMINAL SCIENCE PAYLOAD

  • Neutron and Gamma-ray Spectrometer (NGRS)
  • Wide Angle Multiband Camera (WAM)
  • Near-Infrared Spectrometer (NIRS)
  • Telescopic Camera (TL)
  • Light Detection and Ranging (LIDAR)
  • Circum-Martian Dust Monitor (CMDM)
  • Mass Spectrum Analyzer (MSA)

Members

The MMX team at JAXA.