NASA's MEGANE instrument will act as 'eyeglasses' to study Phobos in JAXA's MMX mission

The origins of Mars' moons remain unclear. Could NASA's MEGANE instrument on JAXA's MMX spacecraft finally reveal whether Phobos is a captured asteroid or debris from an ancient impact?
An artist’s illustration of Japan’s MMX spacecraft approaching Phobos near Mars. (Cover Image Source: JAXA)
An artist’s illustration of Japan’s MMX spacecraft approaching Phobos near Mars. (Cover Image Source: JAXA)

The nature of the two moons of Mars, Phobos and Deimos, still remain a big enigma for scientists. Researchers have two competing theories: these moons are asteroids captured by Mars' gravity, or they formed from debris left behind after a collision between Mars and another large object. To try and solve this mystery, NASA is contributing an instrument called MEGANE (Mars-moon Exploration with GAmma rays and NEutrons) to Japan's upcoming Martian Moons eXploration (MMX) mission, which aims to shed light on the origins of these moons.

An artist’s illustration of Japan’s Martian Moons eXploration (MMX) spacecraft near Phobos, with Mars in the background. (Image Source: JAXA)

JAXA's MMX mission to explore Martian moons

The Japan Aerospace Exploration Agency (JAXA) is scheduled to launch the Martian Moons eXploration (MMX) mission on October 19, 2026, at 3:41 p.m. EDT (4:41 a.m. local time on October 20) from the Tanegashima Space Center. The spacecraft is expected to reach the Martian system in August 2027 and conduct a detailed survey of its two moons, Phobos and Deimos.

Phobos, the larger of Mars’ two moons, imaged by NASA’s High Resolution Imaging Science Experiment (HiRISE) camera aboard the Mars Reconnaissance Orbiter. (Image Source: NASA/JPL Caltech/University of Arizona)

As part of the mission, the spacecraft will collect samples from the surface of Phobos and return them to Earth. Meanwhile, NASA's MEGANE instrument—which literally translates to eyeglasses in Japanese—will measure neutrons and gamma rays emitted from Phobos' surface to help scientists identify the chemical elements present there. As part of the agreement, NASA will also receive about 15% of the samples brought back from Phobos for preservation and study at its Johnson Space Center in Houston.

Deimos, the smaller of Mars’ two moons, in an enhanced-color image captured by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter on February 21, 2009. (Image Source: NASA/JPL-Caltech/University of Arizona)

“The samples from MMX will bring forth paradigm-shifting science on the Mars system for generations to come, especially as NASA prepares to send the first humans to Mars,” Nicky Fox, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington, said in a statement. “The NASA-JAXA sample curation partnership is extremely valuable, and I am proud that NASA Science is supporting MMX sample curation and will be sharing portions of these samples for study as we continue to expand humanity’s understanding of the universe for the benefit of all,” she added.

How MEGANE will study Phobos

The Johns Hopkins Applied Physics Laboratory developed MEGANE for the mission, and the instrument is designed to detect emissions produced when high-energy cosmic rays bombard a moon's surface. Scientists will study these emissions to learn which chemical elements are present on Phobos.

An artist’s illustration of NASA’s MEGANE instrument studying the surface of Phobos aboard Japan’s Martian Moons eXploration (MMX) mission. (Image Source: Johns Hopkins Applied Physics Laboratory (JHU APL)

MEGANE has two detectors that will take different measurements. One is a gamma-ray spectrometer, which will measure the energy of gamma rays. Since different elements emit gamma rays with specific energies, these measurements can help scientists identify the elements present on Phobos and estimate their abundance. On the other hand, the neutron spectrometer in MEGANE will measure neutrons at different energy levels, which will help scientists understand the hydrogen content of the surface material. Scientists will combine the data collected from these two detectors to glean insights into the composition of Phobos' surface, and the measurements could help evaluate the two competing theories about how the moons formed.

A detailed spherical view of Mars showing its dusty red surface, craters, and diverse geological formations against stars. Mars map image courtesy of NASA. (Getty Images| DigitalVision)

“Phobos and Deimos may be the remains of a massive impact on Mars that sent material into orbit around the planet, or they could be ancient asteroids that were captured by Mars’ gravity billions of years ago,” Tom Statler, MMX program executive and program scientist at NASA headquarters, said. “Having the answer will help illuminate that early era when Earth and the other inner planets may have been acquiring much of their water and organic compounds,” he added.

As part of its survey of the two Martian moons, the MMX mission will also deploy a French-German rover named Idefix on Phobos. After collecting samples from Phobos, the Japanese spacecraft is expected to return to Earth in 2031, marking the first ever Martian moon sample return.

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