Preparations have already begun for receiving the sample from Phobos that will be returned by MMX. We talk with Tomohiro Usui, lead of the Japanese curation team, about the preparations for the most precious of deliveries.
One of the main hypotheses for the formation of the moons of Mars is that the moons are captured small bodies, due to their resemblance to the D-type asteroids. But what are D-type asteroids and what would be the scientific importance of the MMX mission returning a sample from this asteroid class?
“With MMX, we will study a tiny moon,” says Hyodo. “But this is not only about the moon, it is also about Solar System material and material from Mars.” Dr Ryuki Hyodo shares the science behind JAXA’s upcoming MMX mission to the Martian moons, and the unique features of this journey to Mars’s domain.
A JAXA integrated PDR that considered all elements was conducted in February 2021. A large number of participants from inside and outside of JAXA were involved in the judging, and the transition to the next phase (Critical Design Phase) was approved.
When the Martian Moons eXploration (MMX) mission returns to Earth in 2029, the spacecraft will bring home a sample capsule containing material from the martian moon, Phobos. This material is expected to not only reveal the composition and history of the moons, but also contain grains ejected from Mars over the red planet’s history. New research now suggests that the sample may also include traces of Mars’s ancient atmosphere.
The Martian Moons eXploration Mission (MMX) will be collaborating with the UK-led Twinkle Space Telescope to elucidate the origin of the Martian moons, Phobos and Deimos.
