MPS-Participation in Bepi Colombo

BELA (Laseraltimeter on MPO)
SERENA (Particle spectrometer on MPO)
MIXS (X-ray spectrometer on MPO)
MPPE (Particle spectrometer on MMO)


  

MPS-Scientists, involved in Bepi Colombo

Christensen, Ulrich (BELA)
Krupp, Norbert (SERENA, MPPE)
Fränz, Markus (SERENA, MPPE)
Krüger, Harald (SERENA, MPPE)
Hilchenbach, Martin (MIXS)

Bepi Colombo: Mission to planet Mercury

The BepiColombo Mission to planet Mercury is a joint project between the European Space Agency ESA and the Japanese counterpart JAXA to be launched in August 2018 and orbiting Mercury from end of 2025 onwards. The project named after Guiseppe (Bepi) Colombo consists of two spacecraft:

  •   the Mercury Planetary Orbiter (MPO) provided by ESA and
  •   the Mercury Magnetospheric Orbiter (MMO) provided by JAXA

providing for the first time two-point measurements in the vicinity of the closest planet in our solar system.

MMO:

MMO<br />Total mass: 275 kg<br />Payload mass: 45 kg<br /><br />
MMO
Total mass: 275 kg
Payload mass: 45 kg

Science objectives

(from ESA website)

  • Origin and evolution of a planet close to the parent star
  • Mercury as a planet: form, interior, structure, geology, composition and craters
  • Mercury's vestigial atmosphere (exosphere): composition and dynamics
  • Mercury's magnetized envelope (magnetosphere): structure and dynamics
  • Origin of Mercury's magnetic field
  • Test of Einstein's theory of general relativity


The scientific objectives behind BepiColombo can be viewed by
considering the following 12 questions:

MPO<br />Total mass: 1150 kg<br />Payload mass: 80 kg
MPO
Total mass: 1150 kg
Payload mass: 80 kg
  1. What can we learn from Mercury about the composition of the solar nebula and the formation of the planetary system?
  2. Why is Mercury's normalized density markedly higher than that of all
    other terrestrial planets, Moon included?
  3. Is the core of Mercury liquid or solid?
  4. Is Mercury tectonically active today?
  5. Why such a small planet does possess an intrinsic magnetic field,
    while Venus, Mars and the Moon do not have any?
  6. Why do spectroscopic observations not reveal the presence of any
    iron, while this element is supposedly the major constituent of Mercury?
  7. Do the permanently shadowed craters of the polar regions contain
    sulphur or water ice?
  8. Is the unseen hemisphere of Mercury markedly different from that
    imaged by Mariner 10?
  9. What are the production mechanisms of the exosphere?
  10. In the absence of any ionosphere, how does the magnetic field
    interact with the solar wind?
  11. Is Mercury's magnetised environment characterised by features
    reminiscent of the aurorae, radiation belts and magnetospheric
    substorms observed at Earth?
  12. Since the advance of Mercury's perihelion was explained in terms of
    space-time curvature, can we take advantage of the proximity of the
    Sun to test general relativity with improved accuracy?


Mission Facts

Launch Date: 2018
Arrival Date: 2025
Mission End: Nominally 1 year in Mercury orbit
Launch Vehicle: Ariane 5
Launch Mass: 4100 kg
Cruise: Heliocentric transfer orbit
At Mercury: MPO polar orbit 400 × 1500 km, 2.3 hr period
MMO polar orbit 400 × 12 000 km, 9.3 hr period

BepiColombo MPO
http://sci.esa.int/science-e/www/area/index.cfm?fareaid=30

BepiColombo MMO <http://www.stp.isas.jaxa.jp/mercury/index-e.html


Messenger http://messenger.jhuapl.edu/> (Other Mercury mission)

 
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