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Examining the Martian Moons
The Mars-moon Exploration with GAmma rays and NEutrons (MEGANE) spectroscopy instrument will provide vital information on the composition of the Martian moons, Phobos and Deimos.
The Mars-moon Exploration with GAmma rays and NEutrons (MEGANE) spectroscopy instrument will provide vital information on the composition of the Martian moons, Phobos and Deimos.
Instrument Type
Gamma-Ray and Neutron
The Martian Moons eXploration (MMX) mission is being developed by the Japan Aerospace Exploration Agency (JAXA). The MMX spacecraft will visit the Martian moon Phobos, land on the surface, collect a surface sample, and then deliver that sample to Earth. On behalf of NASA, APL is leading and building one of the spacecraft’s science instruments: a gamma-ray and neutron spectrometer named MEGANE (pronounced “meh-gah-nay”) that will measure the elemental composition of Phobos. MEGANE’s compositional measurements will provide key information to help determine whether Phobos is a captured asteroid or the result of a larger body hitting Mars.
MEGANE consists of a gamma-ray spectrometer (GRS) and a neutron spectrometer (NS). The GRS uses a high-purity germanium sensor designed and built in partnership with Lawrence Livermore National Laboratory, and is the state-of-the-art technology for achieving high-sensitivity gamma-ray spectral measurements. The NS uses two helium-3 gas proportional sensors to measure neutrons in three broad energy ranges. MEGANE builds on experience from the gamma-ray and neutron spectrometer (GRNS) on NASA’s MESSENGER mission to the planet Mercury and will utilize many aspects of the Psyche GRNS, developed for NASA’s Psyche mission.
Learn more about the different components of MEGANE below. Click the images to view larger versions.
All photos: NASA/JAXA/Johns Hopkins APL/Ed Whitman
The neutron spectrometer on the MEGANE instrument has sensors filled with an isotope of helium gas that will detect cosmic-ray-generated neutrons emitted by Phobos to provide composition information regarding Phobos’ surface.
The gamma-ray spectrometer sensor on the MEGANE instrument contains a high-purity germanium crystal to detect gamma rays that will reveal the elemental composition of Phobos.
The MEGANE Data Processing Unit serves as the electronics “brain” for MEGANE. It operates the sensors by processing sensor commands and then passes the sensor data to the MMX spacecraft for transmittal to Earth.
Launched in October 2026, MMX is a mission led by JAXA that will explore the two Martian moons, Phobos and Deimos, returning a sample from one of them and solving the mystery of where these small moons came from.
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