La mission est composée de deux satellites :

  • MPO : Mercury Planet Orbiter

  • MMO : Mercury Magnetospheric Orbiter

MPO : Mercury Planet Orbiter

Overview of the instruments

  • BELA - BepiColombo Laser Altimeter

  • ISA - Italian Spring Accelerometer

  • MERMAG - MPO-Magnetometer (MERMAG includes the magnetometer on the MMO)

  • MERTIS - Mercury Radiometer and Thermal Infrared Spectrometer

  • MGNS - Mercury Gamma-Ray and Neutron Spectrometer

  • MIXS - Mercury Imaging X-Ray Spectrometer

  • MORE - Mercury Orbiter Radio-Science Experiment

MMO : Mercury Magnetosphere Orbiter

The Mercury Magnetospheric Orbiter (MMO) is a spin-axis stabilised spacecraft with a rotation rate of 15 rpm or spin period of 4s; the spin axis will be nearly perpendicular to Mercury’s equator. Altitude range is currently expected to be from 590 km to 11639 km – the apoherm is nearly 6 planetary radii from planet’s centre.

Overview of the instruments

  • MDM - Mercury Dust Monitor

  • MGF - Magnetometer

  • MPPE - Mercury Plasma Particle Experiment

  • MSASI - Mercury Sodium Atmospheric Spectral Imager

  • PWI - Plasma Wave Investigation

MPPE : Mercury Plasma/Particle Experiment

Mercury Plasma Particle Experiment (MPPE) is a comprehensive instrument package for plasma, high-energy particle and energetic neutral atom measurements. It consists of seven sensors. The first six sensors perform in-situ observations and cover the charged particle species and the energy range of interest from the space plasma physics point of view.

For the electrons: two Mercury Electron Analyzers (MEA1 and MEA2) mounted 90º apart for highresolution coverage, and High Energy Particle instrument for electron (HEP-ele).

For the ions: Mercury Ion Analyzer (MIA), Mercury mass Spectrum Analyzer (MSA), and High Energy Particle instrument for ion (HEP-ion).

The final sensor, Energetic Neutrals Analyzer (ENA) will detect energetic neutrals created via charge-exchange and will provide us with remote information on how plasma and neutral gas interacts in the Hermean environment.

Science goals

  • Structure, dynamics and physical processes in Mercury’s magnetosphere

  • Formation and characteristics of the small-scale magnetosphere

  • Solar wind contribution to the magnetospheric plasmas

  • Stability of the plasma sheet

  • Substorms at Mercury

  • Particle acceleration, trapping, and loss

  • Interaction between surface, exosphere and magnetosphere

  • Collision-less shock physics in the inner heliosphere