MSASI is a high-dispersion Fabry-Perot imager working in the spectral range around sodium D2 emission (589 nm). MSASI will address a wealth of fundamental scientific questions pertaining to the Mercury's exosphere: abundance, distribution and dynamics of sodium in the exosphere.

No public data available yet

PWI will provide remote-sensing observations of electric fields, plasma waves, and radio waves in the Hermean magnetosphere and exosphere. The PWI consists of three sets of receivers (Electric Waveform Onboard, EWO, Spectroscopie Ondes Radio & Bruit Electrostatique Thermique, SORBET, and Active Measurement of Mercury's Plasma, AM2P), connected to two sets of electric field sensors (Mercury Electric Diled In-Situ Tool, MEFISTO and Wire-Probe anTenna, WPT) and two kinds of magnetic field sensors (Low Frequency Search Coils, LF-SC and Dual-Band Search Coil, DB-SC).

No public data available yet

The BepiColombo Laser Altimeter will characterize and measure the figure, topography, and surface morphology of Mercury. It will provide absolute topographic height and position with respect to a Mercury centered coordinate system.

No public data available yet

This 3-axis accelerometer will measure inertial accelerations produced on the MPO structure by the incoming solar visible radiation and by the planet albedo. In combination with MORE, ISA will give information on Mercury's interior structure and test Einstein's theory of the General Relativity.

No public data available yet

Detailed investigations of the planetary magnetic field, its source and its interactions with the solar wind, contributing to our understanding of the origin, evolution and current state of the planetary interior.

No public data available yet

MGNS will measure the elemental composition of the Hermean surface / sub-surface. In addition MGNS will determine the regional distribution of volatile depositions in permanently shadowed areas at the poles, and provide a map of column density of these depositions.

No public data available yet

MIXS will produce global elemental abundance maps of the key-rock forming elements on Mercury's surface to an accuracy of 10-20%. MIXS will also try to confirm whether the auroral zone, where energetic particles interact with the surface, is an intense source of continuum and line X-rays.

No public data available yet

MORE data will help to determine the gravity field of Mercury as well as its internal structure, and the size and physical state of its core. With ISA, it will test theories of gravity with unprecedented accuracy. It will also measure the gravitational oblateness of the Sun.

No public data available yet

This instrument comprises two Neutral Particle Analyzers (ELENA and STROFIO) and two Ion Spectrometers (MIPA and PICAM) that will study the composition, distribution, source and sink processes of Mercury's neutral and charged particle environment.

No public data available yet

SIXS will perform measurements of X-rays and particles of solar origin at Mercury. The instrument will be used to calibrate data from MIXS, and will also study temporal and spectral variability of the solar X-ray corona, and the behaviour and classification of solar flares.

No public data available yet

The BepiColombo Monitoring Cameras are a set of three cameras mounted to the Mercury Transfer Module to monitor deployment and actuation of various spacecraft components (solar arrays, antennae, magnetometer boom) etc.

Data are released approximately one-week after downlink and are available here